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<front>
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<journal-id journal-id-type="publisher-id">ptep</journal-id>
<journal-title-group>
<journal-title>Progress of Theoretical and Experimental Physics</journal-title>
</journal-title-group>
<issn pub-type="epub">2050-3911</issn>
<publisher>
<publisher-name>Oxford University Press</publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.1093/ptep/ptz153</article-id>
<article-id pub-id-type="publisher-id">ptz153</article-id>
<article-id pub-id-type="arxiv">arXiv:1812.09671</article-id>
<article-categories>
<subj-group subj-group-type="category-toc-heading">
<subject>Papers</subject>
<subj-group subj-group-type="category-toc-heading">
<subject>Experimental Particle Physics</subject>
</subj-group>
</subj-group>
<subj-group subj-group-type="category-journal-collection">
<subject>PTEP/C50</subject>
<subject>PTEP/D29</subject>
<subject>PTEP/D50</subject>
</subj-group>
</article-categories>
<title-group>
<article-title>A meta-analysis of neutron lifetime measurements</article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name><surname>Rajan</surname> <given-names>Ashwani</given-names></name>
<xref ref-type="aff" rid="AFF1"/>
</contrib>
<contrib contrib-type="author" corresp="yes">
<name><surname>Desai</surname> <given-names>Shantanu</given-names></name>
<xref ref-type="aff" rid="AFF2"/>
<xref ref-type="corresp" rid="COR1"/>
<email xlink:type="simple">shntn05@gmail.com</email>
</contrib>
</contrib-group>
<aff id="AFF1"><institution>Department of Physics, Indian Institute of Technology</institution>, Guwahati, Assam-781039, <country country="IN">India</country></aff>
<aff id="AFF2"><institution>Department of Physics, Indian Institute of Technology</institution>, Hyderabad, Telangana-502285, <country country="IN">India</country></aff>
<author-notes>
<corresp id="COR1">E-mail: <email>shntn05@gmail.com</email></corresp>
</author-notes>
<pub-date pub-type="cover">
<month>01</month>
<year>2020</year>
</pub-date>
<pub-date pub-type="collection">
<day>01</day>
<month>01</month>
<year>2020</year>
</pub-date>
<pub-date pub-type="epub" iso-8601-date="2020-01-23">
<day>23</day>
<month>01</month>
<year>2020</year>
</pub-date>
<volume>2020</volume>
<issue>1</issue>
<elocation-id>013C01</elocation-id>
<history>
<date date-type="received">
<day>12</day>
<month>10</month>
<year>2018</year>
</date>
<date date-type="rev-recd">
<day>13</day>
<month>11</month>
<year>2019</year>
</date>
<date date-type="accepted">
<day>19</day>
<month>11</month>
<year>2019</year>
</date>
</history>
<permissions>
<copyright-statement>&#x00A9; The Author(s) 2020. Published by Oxford University Press on behalf of the Physical Society of Japan.</copyright-statement>
<copyright-year>2020</copyright-year>
<license license-type="cc-by" xlink:href="http://creativecommons.org/licenses/by/4.0/">
<license-p>This is an Open Access article distributed under the terms of the Creative Commons Attribution License (<ext-link ext-link-type="uri" xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://creativecommons.org/licenses/by/4.0/">http://creativecommons.org/licenses/by/4.0/</ext-link>), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.</license-p>
<license-p>Funded by SCOAP<sup>3</sup></license-p>
</license>
</permissions>
<self-uri xlink:href="ptz153.pdf"/>
<abstract abstract-type="abstract">
<title>Abstract</title>
<p>We calculate the median as well as weighted mean central estimates for the neutron lifetime from a subset of measurements compiled in the 2019 update of the Particle Data Group (PDG). We then reconstruct the error distributions for the residuals using three different central estimates and then check for consistency with a Gaussian distribution. We find that although the error distributions using the weighted mean as well as median estimate are consistent with a Gaussian distribution, the Student&#x2019;s <inline-formula><tex-math notation="LaTeX" id="ImEquation1"><![CDATA[$t$]]></tex-math></inline-formula> and Cauchy distribution provide a better fit. This median statistic estimate of the neutron lifetime from these measurements is given by <inline-formula><tex-math notation="LaTeX" id="ImEquation2"><![CDATA[$881.5 \pm 0.47$]]></tex-math></inline-formula> seconds. This can be used as an alternate estimate of the neutron lifetime. We also note that the discrepancy between beam and bottle-based measurements using median statistics of the neutron lifetime persists with a significance between 4 <inline-formula><tex-math notation="LaTeX" id="ImEquation3"><![CDATA[$\sigma$]]></tex-math></inline-formula> and 8 <inline-formula><tex-math notation="LaTeX" id="ImEquation4"><![CDATA[$\sigma$]]></tex-math></inline-formula>, depending on which combination of measurements is used.</p>
</abstract>
<kwd-group kwd-group-type="jel">
<kwd>C50</kwd>
<kwd>D29</kwd>
<kwd>D50</kwd>
</kwd-group>
<counts>
<page-count count="9"/>
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</front>
<body>
<sec id="SEC1"><title>1. Introduction</title>
<p>The precise measurement and theoretical estimate of the neutron lifetime is of paramount importance for both particle physics and astrophysics [<xref ref-type="bibr" rid="B1">1</xref>,<xref ref-type="bibr" rid="B2">2</xref>]. The current weighted average of seven neutron lifetime measurements, reported in the 2019 version of the Particle Data Group [<xref ref-type="bibr" rid="B3">3</xref>] (PDG, hereafter)<sup><xref ref-type="fn" rid="FN1">1</xref></sup> using the seven best measurements is <inline-formula><tex-math notation="LaTeX" id="ImEquation5"><![CDATA[$879.4 \pm 0.6$]]></tex-math></inline-formula> seconds. At face value, the weighted mean error from these measurements is equal to 0.4 seconds. Therefore, the reduced <inline-formula><tex-math notation="LaTeX" id="ImEquation6"><![CDATA[$\chi^2$]]></tex-math></inline-formula> value for a constant neutron lifetime is equal to 14.6 for six degrees of freedom, corresponding to a <inline-formula><tex-math notation="LaTeX" id="ImEquation7"><![CDATA[$p$]]></tex-math></inline-formula>-value of 0.023 [<xref ref-type="bibr" rid="B4">4</xref>]. If we define the significance as the number of standard deviations a Gaussian variable would fluctuate in one direction corresponding to this <inline-formula><tex-math notation="LaTeX" id="ImEquation8"><![CDATA[$p$]]></tex-math></inline-formula>-value, then the observed <inline-formula><tex-math notation="LaTeX" id="ImEquation9"><![CDATA[$p$]]></tex-math></inline-formula>-value corresponds to a <inline-formula><tex-math notation="LaTeX" id="ImEquation10"><![CDATA[$2 \, \sigma$]]></tex-math></inline-formula> [<xref ref-type="bibr" rid="B5">5</xref>] discrepancy for a constant value of the neutron lifetime. Therefore, the PDG has scaled the weighted mean error by a scale factor equal to <inline-formula><tex-math notation="LaTeX" id="ImEquation11"><![CDATA[$\sqrt{\chi^2/\nu}$]]></tex-math></inline-formula>, where <inline-formula><tex-math notation="LaTeX" id="ImEquation12"><![CDATA[$\nu$]]></tex-math></inline-formula> is the total degrees of freedom. With this multiplicative scale factor of 1.6, the total error is now equal to the reported value of 0.6 seconds. Therefore, the subset of neutron lifetime measurements vetted by the PDG are inconsistent with a constant value at 2 <inline-formula><tex-math notation="LaTeX" id="ImEquation13"><![CDATA[$\sigma$]]></tex-math></inline-formula> significance.</p>
<p>The theoretical neutron lifetime is a function of the axial vector to vector coupling ratio as well as the CKM matrix element <inline-formula><tex-math notation="LaTeX" id="ImEquation14"><![CDATA[$V_{ub}$]]></tex-math></inline-formula> [<xref ref-type="bibr" rid="B6">6</xref>,<xref ref-type="bibr" rid="B7">7</xref>]. The most recent theoretical estimate of the neutron lifetime is between 875.3 and 891.2 seconds, within <inline-formula><tex-math notation="LaTeX" id="ImEquation15"><![CDATA[$3 \, \sigma$]]></tex-math></inline-formula> [<xref ref-type="bibr" rid="B6">6</xref>]. Theoretical uncertainties in the neutron lifetime calculation, and expected improvements in the near future, have recently been reviewed in Ref. [<xref ref-type="bibr" rid="B7">7</xref>].</p>
<p>Neutron lifetime measurement techniques can be broadly classified into two types: &#x201C;bottle&#x201D;- and &#x201C;beam&#x201D;-based measurements. In the bottle method, ultra-cold neutrons are stored in a container (which consists of either some bottle or a trap), and the neutron lifetime is measured by fitting the surviving neutrons to a decaying exponential. In the beam method, on the other hand, the numbers of neutrons and protons are produced from <inline-formula><tex-math notation="LaTeX" id="ImEquation16"><![CDATA[$\beta$]]></tex-math></inline-formula>-decay, and the lifetime is obtained from the neutron decay rate. More details about these techniques can be found in Refs. [<xref ref-type="bibr" rid="B1">1</xref>,<xref ref-type="bibr" rid="B2">2</xref>].</p>
<p>However, there is a long-standing discrepancy between these two methods used for neutron lifetime measurements [<xref ref-type="bibr" rid="B8">8</xref>]. As of 2018, the current value from two beam experiments [<xref ref-type="bibr" rid="B9">9</xref>,<xref ref-type="bibr" rid="B10">10</xref>] included in the 2018 edition of PDG<sup><xref ref-type="fn" rid="FN2">2</xref></sup> is equal to <inline-formula><tex-math notation="LaTeX" id="ImEquation17"><![CDATA[$888 \pm 2.0$]]></tex-math></inline-formula> seconds [<xref ref-type="bibr" rid="B6">6</xref>], and the same from five bottle experiments [<xref ref-type="bibr" rid="B11">11</xref>&#x2013;<xref ref-type="bibr" rid="B15">15</xref>] is equal to <inline-formula><tex-math notation="LaTeX" id="ImEquation18"><![CDATA[$879.6 \pm 0.6$]]></tex-math></inline-formula> seconds [<xref ref-type="bibr" rid="B6">6</xref>]. This is a formally a 4 <inline-formula><tex-math notation="LaTeX" id="ImEquation19"><![CDATA[$\sigma$]]></tex-math></inline-formula> discrepancy, and as pointed out in Fornal and Grienstein [<xref ref-type="bibr" rid="B6">6</xref>] (F18 hereafter) could either be evidence of uncontrolled systematics or could point to new physics. Another possibility, however, not mentioned in the above works, is that the measurements could contain non-Gaussian errors, and consequently the weighted mean cannot be used as the central estimate.</p>
<p>The central estimate of the neutron lifetime mentioned in PDG, as well as all other works which analyze this discrepancy, has been obtained from a weighted average of all the measurements. The central estimate of a quantity using weighted measurements makes the following main assumptions [<xref ref-type="bibr" rid="B16">16</xref>]: (i) individual data points are statistically independent and contain no systematic effects; (ii) the errors are Gaussianly distributed. If any of the measurements contain catastrophic outliers or unaccounted systematic effects, then the second assumption is automatically violated. In that case, the weighted mean can produce extremely biased results. On the other hand, median statistics do not incorporate the individual measurement errors, and hence are unaffected by the presence of a few outliers. Secondly, even if the errors are not correctly estimated, as shown using simulations of Zeldovich&#x2019;s thought experiment involving watches [<xref ref-type="bibr" rid="B17">17</xref>], a median estimate gives a more robust estimate. Even if a dataset is drawn from a distribution with infinite variance such as a Cauchy distribution, the median is a more robust central estimate [<xref ref-type="bibr" rid="B16">16</xref>]. Many additional pitfalls in using the weighted mean as a central estimate, and how using the median value ameliorates these problems, can be found in Refs. [<xref ref-type="bibr" rid="B16">16</xref>,<xref ref-type="bibr" rid="B17">17</xref>] and the references therein. The only assumption used for median-statistic-based estimates is that the measurements are independent and free of systematic errors.</p>
<p>In the last decade, Ratra and collaborators have shown that the error distributions for a whole slew of astrophysical and cosmological measurements are inconsistent with a Gaussian distribution [<xref ref-type="bibr" rid="B16">16</xref>&#x2013;<xref ref-type="bibr" rid="B26">26</xref>]. The datasets they explored for this purpose included measurements of <inline-formula><tex-math notation="LaTeX" id="ImEquation20"><![CDATA[$H_0$]]></tex-math></inline-formula> [<xref ref-type="bibr" rid="B20">20</xref>], lithium-7 measurements [<xref ref-type="bibr" rid="B21">21</xref>] (see also Ref. [<xref ref-type="bibr" rid="B27">27</xref>]), distance to the Large Magellanic Cloud [<xref ref-type="bibr" rid="B22">22</xref>], the distance to the Galactic Center [<xref ref-type="bibr" rid="B28">28</xref>], deuterium abundance [<xref ref-type="bibr" rid="B25">25</xref>], etc. For each of these datasets, they have fitted the data to a variety of probability distributions. From all these studies, they inferred that the error distribution is non-Gaussian. Consequently, they have argued that median statistics should be used for the central estimates of these parameters instead of the weighted mean [<xref ref-type="bibr" rid="B16">16</xref>,<xref ref-type="bibr" rid="B17">17</xref>]. To the best of our knowledge, no one has investigated the Gaussianity of the neutron lifetime measurements (or for that matter any other datasets in PDG). The importance of doing such tests has been stressed in a number of works [<xref ref-type="bibr" rid="B16">16</xref>,<xref ref-type="bibr" rid="B23">23</xref>,<xref ref-type="bibr" rid="B24">24</xref>,<xref ref-type="bibr" rid="B29">29</xref>]. Due to the non-Gaussanity of the error residuals for the aforementioned astrophysical datasets, median statistics have been used to obtain central estimates of some of these quantities such as the Hubble constant [<xref ref-type="bibr" rid="B16">16</xref>,<xref ref-type="bibr" rid="B17">17</xref>,<xref ref-type="bibr" rid="B19">19</xref>], Newton&#x2019;s gravitational constant [<xref ref-type="bibr" rid="B17">17</xref>], the mean matter density [<xref ref-type="bibr" rid="B18">18</xref>], and other cosmological parameters [<xref ref-type="bibr" rid="B23">23</xref>]. Alternately, one can use the method recently proposed by Cowan, where the uncertainty in the systematic errors has been modeled using probabilistic distributions [<xref ref-type="bibr" rid="B30">30</xref>].</p>
<p>Given the importance of the physics implications of these discrepancies in the neutron lifetime measurements, and to obtain a more robust estimate, which can be easily compared with the theoretical estimate, we revisit the issue of checking for non-Gaussianity of the errors and to obtain a more robust central estimate from the vetted measurements in PDG. The outline of this manuscript is as follows. The dataset used for our analysis is described in Sect. <xref ref-type="sec" rid="SEC2">2</xref>. Our analysis procedure and results are described in Sect. <xref ref-type="sec" rid="SEC3">3</xref>. We discuss the discrepacy between beam- and bottle-based measurements in Sect. <xref ref-type="sec" rid="SEC4">4</xref>. We conclude in Sect. <xref ref-type="sec" rid="SEC5">5</xref>.</p>
</sec>
<sec id="SEC2"><title>2. Neutron lifetime data</title>
<p>We briefly review the neutron lifetime measurements used for this analysis. The 2019 edition of PDG lists a total of 27 measurements from 1972 to the present. From these measurements, only seven have been used by the PDG to obtain the central estimate. Using these seven measurements, a weighted mean central value of <inline-formula><tex-math notation="LaTeX" id="ImEquation21"><![CDATA[$879.4 \pm 0.6$]]></tex-math></inline-formula> s was estimated, wherein the error has been rescaled by a factor of 1.6. All of these are bottle-based experiments. The corresponding value from the 2018 PDG edition was <inline-formula><tex-math notation="LaTeX" id="ImEquation22"><![CDATA[$880.2 \pm 1.0$]]></tex-math></inline-formula> s, with five of them been bottle based and two beam based. The remaining measurements were ignored either because the error bars for some of the pre-1980 measurements were large, or if the results from the old measurements were reanalyzed, and lastly because some of the measurements were withdrawn. However, a few measurements have also been culled without any explanation. For our analysis, we also include all older measurements, except if they were reanalyzed or withdrawn. We also include one additional measurement [<xref ref-type="bibr" rid="B31">31</xref>], which was not included in either the 2018 or 2019 PDG. In all, we have collected a total of 19 measurements for our analysis, which are tabulated in <xref ref-type="table" rid="T1">Table 1</xref>. We note that in addition to these direct experimental measurements of neutron lifetime, there are also cosmological constraints on the measurements of neutron lifetime [<xref ref-type="bibr" rid="B32">32</xref>]. We do not include them in our analysis, however, as these results are model dependent, and not direct experimental measurements.</p>
<table-wrap id="T1" orientation="portrait" position="float"><label>Table 1.</label>
<caption><p>Summary of the 19 measurements used for the analysis. PDG18 refers to the 2018 published version of PDG, and PDG19 refers to the 2019 online update. The last eight are listed in PDG, but not used to calculate the weighted mean neutron lifetime by either PDG edition [<xref ref-type="bibr" rid="B3">3</xref>]. The first three measurements are used only in the 2019 edition to calculate the weighted average. The two beam-based measurements [<xref ref-type="bibr" rid="B9">9</xref>,<xref ref-type="bibr" rid="B10">10</xref>] are only used for the 2018 PDG estimate.</p></caption>
<table frame="hsides" rules="groups">
<thead>
<tr>
<th align="left">Reference</th>
<th align="center">Neutron lifetime (secs)</th>
<th align="center">Type</th>
<th align="left">Comment</th>
</tr>
</thead>
<tbody>
<tr>
<td align="left">Ezhov 18 [<xref ref-type="bibr" rid="B37">37</xref>]</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation23"><![CDATA[$878.3 \pm 1.6 \pm 1.0$]]></tex-math></inline-formula></td>
<td align="center">Bottle</td>
<td align="left">Only in PDG19</td>
</tr>
<tr>
<td align="left">Serebrov 17 [<xref ref-type="bibr" rid="B38">38</xref>]</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation24"><![CDATA[$881.5 \pm 0.7 \pm 0.6$]]></tex-math></inline-formula></td>
<td align="center">Bottle</td>
<td align="left">Only in PDG19</td>
</tr>
<tr>
<td align="left">Pattie 17 [<xref ref-type="bibr" rid="B39">39</xref>]</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation25"><![CDATA[$877.7 \pm 0.7 + 0.4/-0.2$]]></tex-math></inline-formula></td>
<td align="center">Bottle</td>
<td align="left">Only in PDG19</td>
</tr>
<tr>
<td align="left">Leung 16 [<xref ref-type="bibr" rid="B31">31</xref>]</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation26"><![CDATA[$887 \pm 39$]]></tex-math></inline-formula></td>
<td align="center">Bottle</td>
<td align="left">Neither PDG18 nor PDG19</td>
</tr>
<tr>
<td align="left">Arzumanov 15 [<xref ref-type="bibr" rid="B15">15</xref>]</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation27"><![CDATA[$880.2 \pm 1.2$]]></tex-math></inline-formula></td>
<td align="center">Bottle</td>
<td align="left">PDG</td>
</tr>
<tr>
<td align="left">Yue 13 [<xref ref-type="bibr" rid="B10">10</xref>]</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation28"><![CDATA[$887.7 \pm 1.2 \pm 1.9$]]></tex-math></inline-formula></td>
<td align="center">Beam</td>
<td align="left">Only in PDG18</td>
</tr>
<tr>
<td align="left">Steyerl 12 [<xref ref-type="bibr" rid="B14">14</xref>]</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation29"><![CDATA[$882.5 \pm 1.4 \pm 1.5$]]></tex-math></inline-formula></td>
<td align="center">Bottle</td>
<td align="left">PDG</td>
</tr>
<tr>
<td align="left">Pichlmaier 10 [<xref ref-type="bibr" rid="B13">13</xref>]</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation30"><![CDATA[$880.7 \pm 1.3 \pm 1.2$]]></tex-math></inline-formula></td>
<td align="center">Bottle</td>
<td align="left">PDG</td>
</tr>
<tr>
<td align="left">Serebrov 05 [<xref ref-type="bibr" rid="B12">12</xref>]</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation31"><![CDATA[$878.5 \pm 0.7 \pm 0.3$]]></tex-math></inline-formula></td>
<td align="center">Bottle</td>
<td align="left">PDG</td>
</tr>
<tr>
<td align="left">Byrne 96 [<xref ref-type="bibr" rid="B9">9</xref>]</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation32"><![CDATA[$889.2\pm 3.0 \pm 3.8$]]></tex-math></inline-formula></td>
<td align="center">Beam</td>
<td align="left">Only in PDG18</td>
</tr>
<tr>
<td align="left">Mampe 93 [<xref ref-type="bibr" rid="B11">11</xref>]</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation33"><![CDATA[$882.6 \pm 2.7$]]></tex-math></inline-formula></td>
<td align="center">Bottle</td>
<td align="left">PDG</td>
</tr>
<tr>
<td align="left">Alfikmenov 90 [<xref ref-type="bibr" rid="B40">40</xref>]</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation34"><![CDATA[$888.4 \pm 2.9$]]></tex-math></inline-formula></td>
<td align="center">Bottle</td>
<td align="left">PDG (but not used)</td>
</tr>
<tr>
<td align="left">Kossakowski 89 [<xref ref-type="bibr" rid="B41">41</xref>]</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation35"><![CDATA[$878 \pm 27 \pm 14$]]></tex-math></inline-formula></td>
<td align="center">Beam</td>
<td align="left">PDG (but not used)</td>
</tr>
<tr>
<td align="left">Paul 89 [<xref ref-type="bibr" rid="B42">42</xref>]</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation36"><![CDATA[$877 \pm 10$]]></tex-math></inline-formula></td>
<td align="center">Bottle</td>
<td align="left">PDG (but not used)</td>
</tr>
<tr>
<td align="left">Last 88 [<xref ref-type="bibr" rid="B43">43</xref>]</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation37"><![CDATA[$876 \pm 10 \pm 19$]]></tex-math></inline-formula></td>
<td align="center">Beam</td>
<td align="left">PDG (but not used)</td>
</tr>
<tr>
<td align="left">Spivak 88 [<xref ref-type="bibr" rid="B44">44</xref>]</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation38"><![CDATA[$891 \pm 9$]]></tex-math></inline-formula></td>
<td align="center">Beam</td>
<td align="left">PDG (but not used)</td>
</tr>
<tr>
<td align="left">Kosvintsev 86 [<xref ref-type="bibr" rid="B45">45</xref>]</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation39"><![CDATA[$903 \pm 13$]]></tex-math></inline-formula></td>
<td align="center">Bottle</td>
<td align="left">PDG (but not used)</td>
</tr>
<tr>
<td align="left">Kosvintsev 86 [<xref ref-type="bibr" rid="B45">45</xref>]</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation40"><![CDATA[$875 \pm 95$]]></tex-math></inline-formula></td>
<td align="center">Bottle</td>
<td align="left">PDG (but not used)</td>
</tr>
<tr>
<td align="left">Christensen 72 [<xref ref-type="bibr" rid="B46">46</xref>]</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation41"><![CDATA[$918 \pm 14$]]></tex-math></inline-formula></td>
<td align="center">Beam</td>
<td align="left">PDG (but not used)</td>
</tr>
</tbody>
</table>
</table-wrap>
</sec>
<sec id="SEC3"><title>3. Analysis</title>
<p>The first step in analyzing the Gaussianity of the error measurements of a dataset is to obtain a central estimate using the available data. For this analysis, we use all 19 measurements tabulated in <xref ref-type="table" rid="T1">Table 1</xref>. We do not check for Gaussianity of the beam- and bottle-based measurements separately, as the total number of data points in each category is too small for a robust test. However, once the number of measurements in each category grows, this should also be tested to check for systematics in each category. We note that in Ref. [<xref ref-type="bibr" rid="B25">25</xref>] a similar analysis was done using 15 deuterium abundance measurements. Similar to the works by Ratra et al. (e.g. Ref. [<xref ref-type="bibr" rid="B25">25</xref>], P18 hereafter), we consider two central estimates: the weighted mean and the median.</p>
<p>The median value (<inline-formula><tex-math notation="LaTeX" id="ImEquation42"><![CDATA[$\tau_{\rm med}$]]></tex-math></inline-formula>) corresponds to the 50% percentile value, for which half of the data points are below and half above. The standard deviation of the median depends upon the distribution it is sampled from. A number of methods have been proposed in the literature to calculate the sample variance of the median [<xref ref-type="bibr" rid="B33">33</xref>&#x2013;<xref ref-type="bibr" rid="B35">35</xref>]. For this work, to estimate the 68% confidence interval on the median we use the methodology in P18, based on Ref. [<xref ref-type="bibr" rid="B16">16</xref>], as the estimate is made using only the data and is independent of the sampling distribution. The weighted mean central value (<inline-formula><tex-math notation="LaTeX" id="ImEquation43"><![CDATA[$\tau_{\rm wm}$]]></tex-math></inline-formula>) using the observed neutron lifetime measurements (<inline-formula><tex-math notation="LaTeX" id="ImEquation44"><![CDATA[$\tau_i$]]></tex-math></inline-formula>) is given by [<xref ref-type="bibr" rid="B36">36</xref>]
<disp-formula id="ptz153M1"><label>(1)</label><tex-math notation="LaTeX" id="Equation1"><![CDATA[$$\begin{equation}
\tau_{\rm wm} = \frac{\sum \limits_{i=1}^N \tau_i/\sigma_i^2}{\sum \limits_{i=1}^N 1/\sigma_i^2},
\end{equation}$$]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation45"><![CDATA[$\sigma_i$]]></tex-math></inline-formula> denotes the total error in each measurement. The total weighted mean error is given by
<disp-formula id="ptz153M2"><label>(2)</label><tex-math notation="LaTeX" id="Equation2"><![CDATA[$$\begin{equation}
\sigma_{\rm M}^2 = \frac{1}{\sum \limits_{i=1}^N 1/\sigma_i^2}.
\end{equation}$$]]></tex-math></disp-formula></p>
<p>From the measurements in <xref ref-type="table" rid="T1">Table 1</xref>, the weighted mean estimate is found to be <inline-formula><tex-math notation="LaTeX" id="ImEquation46"><![CDATA[$\tau_{\rm wm} = 879.97 \pm 0.39$]]></tex-math></inline-formula> seconds, and the median estimate is calculated to be <inline-formula><tex-math notation="LaTeX" id="ImEquation47"><![CDATA[$\tau_{\rm med} = 881.5\pm 0.47$]]></tex-math></inline-formula> seconds.</p>
<sec id="SEC3.1"><title>3.1. Error distributions</title>
<p>Once we have a central estimate for the neutron lifetime (<inline-formula><tex-math notation="LaTeX" id="ImEquation48"><![CDATA[$\tau_{\rm CE}$]]></tex-math></inline-formula>) using one of the above three methods, we calculate the residual error using [<xref ref-type="bibr" rid="B25">25</xref>,<xref ref-type="bibr" rid="B28">28</xref>]
<disp-formula id="ptz153M3"><label>(3)</label><tex-math notation="LaTeX" id="Equation3"><![CDATA[$$\begin{equation}
N_{\sigma_i} =\frac{\tau_i-\tau_{\rm CE}}{\sqrt{\sigma_i^2+\sigma_{\rm CE}^2}} .
\label{eq:nsigma}
\end{equation}$$]]></tex-math></disp-formula></p>
<p>In the above equation, <inline-formula><tex-math notation="LaTeX" id="ImEquation49"><![CDATA[$\sigma_{\rm CE}$]]></tex-math></inline-formula> is the error in the central estimate and <inline-formula><tex-math notation="LaTeX" id="ImEquation50"><![CDATA[$\sigma_i$]]></tex-math></inline-formula> is the error in the individual measurement. Similar to Refs. [<xref ref-type="bibr" rid="B25">25</xref>,<xref ref-type="bibr" rid="B26">26</xref>,<xref ref-type="bibr" rid="B28">28</xref>], we denote our error distribution for the median (<inline-formula><tex-math notation="LaTeX" id="ImEquation51"><![CDATA[$\tau_{\rm med}$]]></tex-math></inline-formula>) and the weighted mean (<inline-formula><tex-math notation="LaTeX" id="ImEquation52"><![CDATA[$\tau_{\rm wm}$]]></tex-math></inline-formula>) calculated from Eq. <xref ref-type="disp-formula" rid="ptz153M3">3</xref> by <inline-formula><tex-math notation="LaTeX" id="ImEquation53"><![CDATA[$N_{\sigma_i}^{\rm med}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation54"><![CDATA[$N_{\sigma_i}^{\rm wm+}$]]></tex-math></inline-formula> respectively. If the central estimate is determined from the weighted mean, one must also account for correlations, and the modified version of the error distribution that accounts for these correlations is given by [<xref ref-type="bibr" rid="B28">28</xref>]
<disp-formula id="ptz153M4"><label>(4)</label><tex-math notation="LaTeX" id="Equation4"><![CDATA[$$\begin{equation}
N_{\sigma_i}^{\rm wm-} =\frac{\tau_i-\tau_{\rm CE}}{\sqrt{\sigma_i^2-\sigma_{\rm CE}^2}} .
\end{equation}$$]]></tex-math></disp-formula></p>
<p>Each of these three sets of <inline-formula><tex-math notation="LaTeX" id="ImEquation55"><![CDATA[$|N_{\sigma}|$]]></tex-math></inline-formula> histograms is then symmetrized around zero. We then fit the symmetrized histogram of <inline-formula><tex-math notation="LaTeX" id="ImEquation56"><![CDATA[$|N_{\sigma_i}|$]]></tex-math></inline-formula> to multiple probability distributions as described in the next subsection.</p>
</sec>
<sec id="SEC3.2"><title>3.2. Fits to probability distributions</title>
<p>We fit the symmetrized histograms for each of the <inline-formula><tex-math notation="LaTeX" id="ImEquation57"><![CDATA[$|N_{\sigma}|$]]></tex-math></inline-formula> to a Gaussian distribution as well as to variants of Gaussian distributions, such as Cauchy, Laplacian, and Student&#x2019;s <inline-formula><tex-math notation="LaTeX" id="ImEquation58"><![CDATA[$t$]]></tex-math></inline-formula> distribution, to see which of these is most compatible with the data. This is similar in spirit to recent works by Ratra et al., such as P18 and references therein. We briefly review this procedure; more details can be found in P18.</p>
<p>The Gaussian distribution we consider has zero mean and standard deviation equal to unity:
<disp-formula id="ptz153M5"><label>(5)</label><tex-math notation="LaTeX" id="Equation5"><![CDATA[$$\begin{equation}
P(N) = \frac{1}{\sqrt{2\pi}}\exp(-|N|^2/2) .
\label{eq:gauss}
\end{equation}$$]]></tex-math></disp-formula></p>
<p>The second distribution we consider is the Laplacian distribution, which has a sharp peak and longer tails than a Gaussian distribution and is described by
<disp-formula id="ptz153M6"><label>(6)</label><tex-math notation="LaTeX" id="Equation6"><![CDATA[$$\begin{equation}
P(N) = \frac{1}{2}\exp(-|N|) .
\label{eq:laplace}
\end{equation}$$]]></tex-math></disp-formula></p>
<p>The third distribution we will use is the Cauchy or Lorentz distribution. It has longer and thicker tails compared to a Gaussian distribution. It is described by
<disp-formula id="ptz153M7"><label>(7)</label><tex-math notation="LaTeX" id="Equation7"><![CDATA[$$\begin{equation}
P(N) = \frac{1}{\pi(1+|N|^2)} .
\label{eq:cauchy}
\end{equation}$$]]></tex-math></disp-formula></p>
<p>Finally, we use the Student&#x2019;s <inline-formula><tex-math notation="LaTeX" id="ImEquation59"><![CDATA[$t$]]></tex-math></inline-formula> distribution characterized by <inline-formula><tex-math notation="LaTeX" id="ImEquation60"><![CDATA[$n$]]></tex-math></inline-formula> (which is sometimes referred to as &#x201C;degrees of freedom&#x201D;) and is given by
<disp-formula id="ptz153M8"><label>(8)</label><tex-math notation="LaTeX" id="Equation8"><![CDATA[$$\begin{equation}
P(N) = \frac{\Gamma[(n+1)/2]}{\sqrt{\pi n}\Gamma(n/2)(1+|N|^2/n)^{(n+1)/2}} .
\label{eq:student}
\end{equation}$$]]></tex-math></disp-formula></p>
<p>For <inline-formula><tex-math notation="LaTeX" id="ImEquation61"><![CDATA[$n=1$]]></tex-math></inline-formula> the Student&#x2019;s <inline-formula><tex-math notation="LaTeX" id="ImEquation62"><![CDATA[$t$]]></tex-math></inline-formula> distribution is same as the Cauchy distribution, and it is equal to the Gaussian distribution for <inline-formula><tex-math notation="LaTeX" id="ImEquation63"><![CDATA[$n=\infty$]]></tex-math></inline-formula>. For our analysis we vary <inline-formula><tex-math notation="LaTeX" id="ImEquation64"><![CDATA[$n$]]></tex-math></inline-formula> from 2 to 2000. Note that the Student&#x2019;s <inline-formula><tex-math notation="LaTeX" id="ImEquation65"><![CDATA[$t$]]></tex-math></inline-formula> distribution for the error residuals can be obtained by modeling the error in systematic errors as a gamma distribution [<xref ref-type="bibr" rid="B30">30</xref>].</p>
<p>In addition to comparing the error distributions to the probability distribution functions (PDFs) in Eqs. <xref ref-type="disp-formula" rid="ptz153M5">5</xref>&#x2013; <xref ref-type="disp-formula" rid="ptz153M8">8</xref>, which mainly depend on <inline-formula><tex-math notation="LaTeX" id="ImEquation66"><![CDATA[$|N|$]]></tex-math></inline-formula>, we also compare to these distributions after replacing <inline-formula><tex-math notation="LaTeX" id="ImEquation67"><![CDATA[$N$]]></tex-math></inline-formula> by <inline-formula><tex-math notation="LaTeX" id="ImEquation68"><![CDATA[$N/S$]]></tex-math></inline-formula>, where <inline-formula><tex-math notation="LaTeX" id="ImEquation69"><![CDATA[$S$]]></tex-math></inline-formula> is an arbitrary scale factor, which we vary from 0.001 to 2.5 in steps of size 0.01.</p>
<p>The comparison is done using the one-sample unbinned Kolmogorov&#x2013;Smirnov (K&#x2013;S) test [<xref ref-type="bibr" rid="B47">47</xref>]. The K&#x2013;S test is based on the <inline-formula><tex-math notation="LaTeX" id="ImEquation70"><![CDATA[$D$]]></tex-math></inline-formula> statistic, which measures the maximum distance between two cumulative distributions. The K&#x2013;S test is widely used in both astrophysics and particle physics to compare a dataset to a wide range of probability distributions, as it is agnostic to the distribution against which it is being tested, and does not depend on the size of the sample. Furthermore, critical values based upon the <inline-formula><tex-math notation="LaTeX" id="ImEquation71"><![CDATA[$D$]]></tex-math></inline-formula> statistic have been calculated in the literature and can be easily computed for any value of <inline-formula><tex-math notation="LaTeX" id="ImEquation72"><![CDATA[$D$]]></tex-math></inline-formula>. This test is also invariant to reparameterization of the data. The one-sample K&#x2013;S test can therefore serve as a goodness-of-fit test. Although some concerns have been raised regarding incorrect usage of the K&#x2013;S test in the astrophysics literature, as well as other caveats and limitations of this test [<xref ref-type="bibr" rid="B48">48</xref>], these do not apply in our case, and hence we use the K&#x2013;S test to evaluate the compatibility of the error residuals with various distributions. In this case, the two distributions are the error histograms and the parent PDF to which it is compared. From the <inline-formula><tex-math notation="LaTeX" id="ImEquation73"><![CDATA[$D$]]></tex-math></inline-formula> statistic, the K&#x2013;S test also provides a <inline-formula><tex-math notation="LaTeX" id="ImEquation74"><![CDATA[$p$]]></tex-math></inline-formula>-value, whose analytic formula can be found in any statistics work [<xref ref-type="bibr" rid="B25">25</xref>,<xref ref-type="bibr" rid="B47">47</xref>]. For this work we used the <monospace>scipy</monospace> module in <monospace>Python</monospace> for the computations. The higher the <inline-formula><tex-math notation="LaTeX" id="ImEquation75"><![CDATA[$p$]]></tex-math></inline-formula>-value, the more similar the two distributions, whereas a low <inline-formula><tex-math notation="LaTeX" id="ImEquation76"><![CDATA[$p$]]></tex-math></inline-formula>-value indicates an inconsistency between the distributions. Our results for the comparison with all four distributions are summarized in <xref ref-type="table" rid="T2">Table 2</xref>.</p>
<table-wrap id="T2" orientation="portrait" position="float"><label>Table 2.</label>
<caption><p>Probabilities from the K&#x2013;S test for various distributions using the observed neutron lifetime measurements.<inline-formula><tex-math notation="LaTeX" id="ImEquation77"><![CDATA[$^*$]]></tex-math></inline-formula></p></caption>
<table frame="hsides" rules="groups">
<thead>
<tr>
<th align="left">&#x00A0;</th>
<th align="center" colspan="3">Median (<inline-formula><tex-math notation="LaTeX" id="ImEquation78"><![CDATA[$\tau_{\rm med}$]]></tex-math></inline-formula>)</th>
<th align="center"></th>
<th align="center" colspan="3">Weighted mean (<inline-formula><tex-math notation="LaTeX" id="ImEquation79"><![CDATA[$\tau_{\rm wm+}$]]></tex-math></inline-formula>)</th>
<th align="center"></th>
<th align="center" colspan="3">Weighted mean (<inline-formula><tex-math notation="LaTeX" id="ImEquation80"><![CDATA[$\tau_{\rm wm-}$]]></tex-math></inline-formula>)</th>
</tr>
<tr>
<th align="left">Distribution</th>
<th align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation81"><![CDATA[$S$]]></tex-math></inline-formula></th>
<th align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation82"><![CDATA[$p$]]></tex-math></inline-formula></th>
<th align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation83"><![CDATA[$n$]]></tex-math></inline-formula></th>
<th align="center">&#x00A0;</th>
<th align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation84"><![CDATA[$S$]]></tex-math></inline-formula></th>
<th align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation85"><![CDATA[$p$]]></tex-math></inline-formula></th>
<th align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation86"><![CDATA[$n$]]></tex-math></inline-formula></th>
<th align="center">&#x00A0;</th>
<th align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation87"><![CDATA[$S$]]></tex-math></inline-formula></th>
<th align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation88"><![CDATA[$p$]]></tex-math></inline-formula></th>
<th align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation89"><![CDATA[$n$]]></tex-math></inline-formula></th>
</tr>
</thead>
<tbody>
<tr>
<td align="left">Gaussian</td>
<td align="center">1</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation90"><![CDATA[$0.299$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
<td align="center">&#x00A0;</td>
<td align="center">1</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation91"><![CDATA[$0.327$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
<td align="center">&#x00A0;</td>
<td align="center">1</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation92"><![CDATA[$0.186$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
</tr>
<tr>
<td align="left">&#x00A0;</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation93"><![CDATA[$1.317$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation94"><![CDATA[$0.875$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
<td align="center">&#x00A0;</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation95"><![CDATA[$1.378$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation96"><![CDATA[$0.974$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
<td align="center">&#x00A0;</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation97"><![CDATA[$1.562$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation98"><![CDATA[$0.958$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
</tr>
<tr>
<td align="left">Laplacian</td>
<td align="center">1</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation99"><![CDATA[$0.771$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
<td align="center">&#x00A0;</td>
<td align="center">1</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation100"><![CDATA[$0.691$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
<td align="center">&#x00A0;</td>
<td align="center">1</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation101"><![CDATA[$0.556$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
</tr>
<tr>
<td align="left">&#x00A0;</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation102"><![CDATA[$1.214$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation103"><![CDATA[$0.983$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
<td align="center">&#x00A0;</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation104"><![CDATA[$1.304$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation105"><![CDATA[$0.996$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
<td align="center">&#x00A0;</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation106"><![CDATA[$1.428$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation107"><![CDATA[$0.996$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
</tr>
<tr>
<td align="left">Cauchy</td>
<td align="center">1</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation108"><![CDATA[$0.878$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
<td align="center">&#x00A0;</td>
<td align="center">1</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation109"><![CDATA[$0.908$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
<td align="center">&#x00A0;</td>
<td align="center">1</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation110"><![CDATA[$0.925$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
</tr>
<tr>
<td align="left">&#x00A0;</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation111"><![CDATA[$0.786$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation112"><![CDATA[$0.997$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
<td align="center">&#x00A0;</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation113"><![CDATA[$0.817$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation114"><![CDATA[$0.982$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
<td align="center">&#x00A0;</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation115"><![CDATA[$0.85$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation116"><![CDATA[$0.980$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
</tr>
<tr>
<td align="left">Student&#x2019;s <inline-formula><tex-math notation="LaTeX" id="ImEquation117"><![CDATA[$t$]]></tex-math></inline-formula></td>
<td align="center">1</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation118"><![CDATA[$0.954$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation119"><![CDATA[$2$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
<td align="center">1</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation120"><![CDATA[$0.928$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation121"><![CDATA[$2$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
<td align="center">1</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation122"><![CDATA[$0.267$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation123"><![CDATA[$2$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td align="left">&#x00A0;</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation124"><![CDATA[$1.021$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation125"><![CDATA[$0.966$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation126"><![CDATA[$2$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation127"><![CDATA[$1.091$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation128"><![CDATA[$0.989$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation129"><![CDATA[$2$]]></tex-math></inline-formula></td>
<td align="center">&#x00A0;</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation130"><![CDATA[$1.201$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation131"><![CDATA[$0.987$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation132"><![CDATA[$2$]]></tex-math></inline-formula></td>
</tr>
</tbody>
</table>
<table-wrap-foot>
<fn id="tblfn1"><p><inline-formula><tex-math notation="LaTeX" id="ImEquation133"><![CDATA[$^*$]]></tex-math></inline-formula> <inline-formula><tex-math notation="LaTeX" id="ImEquation134"><![CDATA[$S$]]></tex-math></inline-formula>: The scale factor (other than 1) which maximizes <inline-formula><tex-math notation="LaTeX" id="ImEquation135"><![CDATA[$p$]]></tex-math></inline-formula>. <inline-formula><tex-math notation="LaTeX" id="ImEquation136"><![CDATA[$p$]]></tex-math></inline-formula>: The <inline-formula><tex-math notation="LaTeX" id="ImEquation137"><![CDATA[$p$]]></tex-math></inline-formula>-value that the data is derived from the PDF. <inline-formula><tex-math notation="LaTeX" id="ImEquation138"><![CDATA[$n$]]></tex-math></inline-formula>: The value <inline-formula><tex-math notation="LaTeX" id="ImEquation139"><![CDATA[$n$]]></tex-math></inline-formula> in the Student&#x2019;s <inline-formula><tex-math notation="LaTeX" id="ImEquation140"><![CDATA[$t$]]></tex-math></inline-formula> distribution.</p></fn>
</table-wrap-foot>
</table-wrap>
<p>We find that for all three estimates the Gaussian distribution is not the best fit, unless the scale factor is different from unity. The data are much more consistent with the Cauchy or Student&#x2019;s <inline-formula><tex-math notation="LaTeX" id="ImEquation141"><![CDATA[$t$]]></tex-math></inline-formula> distribution. However, none of the <inline-formula><tex-math notation="LaTeX" id="ImEquation142"><![CDATA[$p$]]></tex-math></inline-formula>-values for the Gaussian distribution are small enough to reject the null hypothesis.</p>
</sec>
</sec>
<sec id="SEC4"><title>4. Discrepancy between beam and bottle measurements</title>
<p>We now quantify the significance of the discrepancy between beam- and bottle-based experiments using central estimates based on the median statistics. We do this analysis using three different combinations of datasets for beam- and bottle-based experiments. A summary of these comparisons can be found in <xref ref-type="table" rid="T3">Table 3</xref>.</p>
<table-wrap id="T3" orientation="portrait" position="float"><label>Table 3.</label>
<caption><p>Summary of the significance of the discrepancies between beam and bottle-based measurements using median statistics. The first column refers to the datasets used. The second and third columns contain the median statistics estimate of the neutron lifetime(<inline-formula><tex-math notation="LaTeX" id="ImEquation143"><![CDATA[$\tau_N$]]></tex-math></inline-formula>) using bottle and beam-based measurements respectively, using <inline-formula><tex-math notation="LaTeX" id="ImEquation144"><![CDATA[$1\sigma$]]></tex-math></inline-formula> median error bars obtained using the procedure in Ref. [<xref ref-type="bibr" rid="B16">16</xref>]. The last column indicates the statistical significance of the discrepancy.</p></caption>
<table frame="hsides" rules="groups">
<thead>
<tr>
<th align="left">Dataset</th>
<th align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation145"><![CDATA[$\tau_N$]]></tex-math></inline-formula> (bottle-based)</th>
<th align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation146"><![CDATA[$\tau_N$]]></tex-math></inline-formula> (beam-based)</th>
<th align="center">Discrepancy</th>
</tr>
<tr>
<th align="left">&#x00A0;</th>
<th align="center">(s)</th>
<th align="center">(s)</th>
<th align="center">&#x00A0;</th>
</tr>
</thead>
<tbody>
<tr>
<td align="left">F18 [<xref ref-type="bibr" rid="B6">6</xref>]</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation147"><![CDATA[$880.7 \pm 1.3$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation148"><![CDATA[$888.45$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation149"><![CDATA[$6 \, \sigma$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td align="left">Data from <xref ref-type="table" rid="T1">Table 1</xref></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation150"><![CDATA[$880.7 \pm 1.2$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation151"><![CDATA[$888.45 \pm 1.65$]]></tex-math></inline-formula></td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation152"><![CDATA[$3.79 \, \sigma$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td align="left">Data from Table 1 with errors <inline-formula><tex-math notation="LaTeX" id="ImEquation153"><![CDATA[$<$]]></tex-math></inline-formula> 10 s</td>
<td align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation154"><![CDATA[$880.2 \pm 1.1$]]></tex-math></inline-formula></td>
<td align="center">889.2</td>
<td align="center">8.2 <inline-formula><tex-math notation="LaTeX" id="ImEquation155"><![CDATA[$\sigma$]]></tex-math></inline-formula></td>
</tr>
</tbody>
</table>
</table-wrap>
<p>We first use the same data points as in F18 [<xref ref-type="bibr" rid="B6">6</xref>], who argued for a <inline-formula><tex-math notation="LaTeX" id="ImEquation156"><![CDATA[$4.4 \, \sigma$]]></tex-math></inline-formula> discrepancy. We obtain a median estimate using the same bottle-based experiments considered in F18 [<xref ref-type="bibr" rid="B11">11</xref>&#x2013;<xref ref-type="bibr" rid="B15">15</xref>], and compare the same with the beam-based experiments therein [<xref ref-type="bibr" rid="B9">9</xref>,<xref ref-type="bibr" rid="B10">10</xref>]. The median lifetime of the five bottle-based experiments along with the <inline-formula><tex-math notation="LaTeX" id="ImEquation157"><![CDATA[$1 \, \sigma$]]></tex-math></inline-formula> median error bar is given by <inline-formula><tex-math notation="LaTeX" id="ImEquation158"><![CDATA[$880.7 \pm 1.3$]]></tex-math></inline-formula> seconds. The corresponding lifetime for the two beam-based experiments considered in F18 is <inline-formula><tex-math notation="LaTeX" id="ImEquation159"><![CDATA[$888.45$]]></tex-math></inline-formula> seconds. Since it is not possible to obtain a median error estimate with just two measurements, we do not quote its <inline-formula><tex-math notation="LaTeX" id="ImEquation160"><![CDATA[$1 \, \sigma$]]></tex-math></inline-formula> median uncertainty. The results do not change even after including the two additional bottle-based measurements [<xref ref-type="bibr" rid="B38">38</xref>,<xref ref-type="bibr" rid="B39">39</xref>] not used for their average. Therefore, considering the median statistics estimates, the discrepancy is about <inline-formula><tex-math notation="LaTeX" id="ImEquation161"><![CDATA[$6 \, \sigma$]]></tex-math></inline-formula>.</p>
<p>If we do this comparison by including all the measurements in <xref ref-type="table" rid="T3">Table 3</xref>, the median lifetime for all the bottle-based experiments is equal to <inline-formula><tex-math notation="LaTeX" id="ImEquation162"><![CDATA[$880.7 \pm 1.2$]]></tex-math></inline-formula> seconds. The corresponding number for all the beam-based experiments is <inline-formula><tex-math notation="LaTeX" id="ImEquation163"><![CDATA[$888.45 \pm 1.65$]]></tex-math></inline-formula> seconds. Therefore, comparing the median estimates between the beam- and bottle-based measurements amounts to a 3.79 <inline-formula><tex-math notation="LaTeX" id="ImEquation164"><![CDATA[$\sigma$]]></tex-math></inline-formula> discrepancy.</p>
<p>If we then redo this comparison for the subset of the measurements in <xref ref-type="table" rid="T1">Table 1</xref> having a total error less than 10 seconds, the median central estimate for all bottle-based experiments is <inline-formula><tex-math notation="LaTeX" id="ImEquation165"><![CDATA[$880.2 \pm 1.1$]]></tex-math></inline-formula> s. Since the total number of beam-based measurements in <xref ref-type="table" rid="T1">Table 1</xref> is a very small number (three), we can only obtain a central estimate, which is equal to 889.2 seconds. Therefore, the total discrepancy is about <inline-formula><tex-math notation="LaTeX" id="ImEquation166"><![CDATA[$8.2 \, \sigma$]]></tex-math></inline-formula>.</p>
<p>Hence, we infer that the discrepancy between beam- and bottle-based measurements persists, even when median statistics is used for the central estimate of the neutron lifetime.</p>
</sec>
<sec id="SEC5"><title>5. Conclusions</title>
<p>There has been a long-standing discrepancy in the literature related to neutron lifetime measurements between two different techniques, viz. bottle- and beam-based methods. As of 2019, the current discrepancy is about <inline-formula><tex-math notation="LaTeX" id="ImEquation167"><![CDATA[$4 \sigma$]]></tex-math></inline-formula> [<xref ref-type="bibr" rid="B6">6</xref>]. To get some insight into these issues, we carried out an extensive meta-analysis of the vetted neutron lifetime measurements compiled in the literature. We first used a compilation of 19 measurements of the neutron lifetime and their corresponding errors listed in the 2019 edition of PDG [<xref ref-type="bibr" rid="B3">3</xref>] (cf. <xref ref-type="table" rid="T1">Table 1</xref>), in order to ascertain the non-Gaussianity of the residuals and to obtain a central estimate. The error distributions were analyzed in the same way as previously done for a variety of astrophysical measurements by Ratra et al. [<xref ref-type="bibr" rid="B25">25</xref>,<xref ref-type="bibr" rid="B26">26</xref>,<xref ref-type="bibr" rid="B28">28</xref>]. For this purpose, the central estimate was obtained using both the weighted mean (with and without correlations) and the median value. The median estimate does not incorporate the errors in the neutron lifetime. We then fitted these residuals to four distributions, viz. Gaussian, Laplace, Cauchy, and Student&#x2019;s <inline-formula><tex-math notation="LaTeX" id="ImEquation168"><![CDATA[$t$]]></tex-math></inline-formula> distribution. The resulting fits are tabulated in <xref ref-type="table" rid="T2">Table 2</xref>.</p>
<p>We conclude from these observations that none of the <inline-formula><tex-math notation="LaTeX" id="ImEquation169"><![CDATA[$p$]]></tex-math></inline-formula>-values (obtained using all three central estimates) are small enough to reject the Gaussian distribution for the error residuals. However, the Student&#x2019;s <inline-formula><tex-math notation="LaTeX" id="ImEquation170"><![CDATA[$t$]]></tex-math></inline-formula> and Cauchy distributions provide a more robust fit than the Gaussian distribution.</p>
<p>Therefore, more data points are necessary to robustly determine if the error residuals are consistent with a Gaussian distribution. Nevertheless, it would be a useful exercise to obtain the central estimate of the neutron lifetime with median statistics, and to check if the discrepancy between beam- and bottle-based measurements persists using median statistics. The median value along with 1 <inline-formula><tex-math notation="LaTeX" id="ImEquation171"><![CDATA[$\sigma$]]></tex-math></inline-formula> error bars using the 19 measurements that we obtained is given by <inline-formula><tex-math notation="LaTeX" id="ImEquation172"><![CDATA[$881.5 \pm 0.47$]]></tex-math></inline-formula> seconds. This estimate is complementary to the PDG-based result obtained using weighted mean statistics, which includes the addition of an ad hoc scale factor. This value can be used as an alternate estimate of the observed neutron lifetime, and used for comparison with the theoretical estimate, which is currently between 875.3 and 891.2 seconds within <inline-formula><tex-math notation="LaTeX" id="ImEquation173"><![CDATA[$3 \, \sigma$]]></tex-math></inline-formula> [<xref ref-type="bibr" rid="B6">6</xref>]. Furthermore, this median value provides an alternate central estimate of the neutron lifetime, which can be used for comparison with theoretical estimates.</p>
<p>We then used the median estimate to evaluate the statistical significance of the discrepancy between beam- and bottle-based measurements. When we use the same measurements as in F18, the discrepancy exacerbates to 6 <inline-formula><tex-math notation="LaTeX" id="ImEquation174"><![CDATA[$\sigma$]]></tex-math></inline-formula>. If we consider all the measurements in <xref ref-type="table" rid="T1">Table 1</xref>, the discrepancy becomes <inline-formula><tex-math notation="LaTeX" id="ImEquation175"><![CDATA[$3.8 \, \sigma$]]></tex-math></inline-formula> (<inline-formula><tex-math notation="LaTeX" id="ImEquation176"><![CDATA[$8.2 \, \sigma$]]></tex-math></inline-formula>), depending on whether we include (exclude) measurements in this, with the total error less than 10 seconds.</p>
</sec>
</body>
<back>
<ack id="ack1">
<title>Acknowledgements</title>
<p>We are grateful to Tomasso Dorigo for his nice blog article about the F18 paper, which brought this problem to our attention. We also thank Bharat Ratra for explaining in detail the methodology used in P18 and also in his earlier works.</p>
</ack>
<sec>
<title>Funding</title>
<p>Open Access funding: SCOAP<inline-formula><tex-math notation="LaTeX" id="ImEquation177"><![CDATA[$^3$]]></tex-math></inline-formula>.</p>
</sec>
<fn-group>
<title>Footnotes</title>
<fn id="FN1"><p><sup>1</sup> At the time of writing, the 2019 PDG update on neutron lifetime measurements is only available online at <ext-link ext-link-type="uri" xlink:href="http://pdg.lbl.gov/2019/listings/rpp2019-list-n.pdf">http://pdg.lbl.gov/2019/listings/rpp2019-list-n.pdf</ext-link>. The published version [<xref ref-type="bibr" rid="B3">3</xref>] contains listings from 2018.</p></fn>
<fn id="FN2"><p><sup>2</sup> These two measurements are not used for the neutron lifetime estimate by the 2019 PDG edition.</p></fn>
</fn-group>
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