{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,3,6]],"date-time":"2026-03-06T03:58:07Z","timestamp":1772769487489,"version":"3.50.1"},"reference-count":56,"publisher":"IOP Publishing","issue":"06","license":[{"start":{"date-parts":[[2024,6,19]],"date-time":"2024-06-19T00:00:00Z","timestamp":1718755200000},"content-version":"vor","delay-in-days":18,"URL":"http:\/\/creativecommons.org\/licenses\/by\/4.0\/"},{"start":{"date-parts":[[2024,6,19]],"date-time":"2024-06-19T00:00:00Z","timestamp":1718755200000},"content-version":"tdm","delay-in-days":18,"URL":"https:\/\/iopscience.iop.org\/info\/page\/text-and-data-mining"}],"content-domain":{"domain":["iopscience.iop.org"],"crossmark-restriction":false},"short-container-title":["J. Cosmol. Astropart. Phys."],"published-print":{"date-parts":[[2024,6,1]]},"abstract":"Abstract<\/jats:title>\n Xenon scintillation has been widely used in rare event detection\n experiments, such as in neutrinoless double beta decay, double electron\n captures and dark matter searches. Nonetheless, experimental values for primary scintillation yield in gaseous xenon (GXe) remain scarce and dispersed. The mean\n energy required to produce a scintillation photon, w<\/jats:italic>\n sc<\/jats:sub>, in GXe in the absence of recombination has been measured to be in the range of\n 34\u2013111 eV. Lower w<\/jats:italic>\n sc<\/jats:sub>-values were reported for \u03b1-particles\n when compared to electrons produced by \u03b3<\/jats:italic>- or x-rays. Since w<\/jats:italic>\n sc<\/jats:sub> is expected to be similar for x-, \u03b3<\/jats:italic>-rays or electrons and almost equal to that obtained for \u03b1-particles, the above difference can not be understood. In addition, at present one may also pose the question of a dependence of w<\/jats:italic>\n sc<\/jats:sub> on photon energy.\n We carried out a systematic study on the absolute primary scintillation yield in GXe under reduced electric fields in the 70\u2013300 V cm-1<\/jats:sup> bar-1<\/jats:sup> range and near atmospheric pressure, 1.2 bar, supported by a robust geometrical efficiency simulation model.\n\n We were able to clear-out the above standing problems: w<\/jats:italic>\n sc<\/jats:sub> was determined for x\/\u03b3<\/jats:italic>-rays in the 5.9\u201360 keV energy range as well as for \u03b1-particles in the 1.5\u20132.5 MeV range, and no significant dependency neither on radiation type nor on energy has been observed. Our experimental w<\/jats:italic>\n sc<\/jats:sub>-values agree well with both up-to-date simulations and literature data obtained for \u03b1-particles. The discrepancy between our results and the experimental values found in the literature for x\/\u03b3<\/jats:italic>-rays is discussed in this work and attributed to unaddressed large systematic errors in those previous studies.\n These findings can be extrapolated to other gases, and have impact on experiments such as double beta decay, double electron capture and directional dark matter searches while also on potential future detection systems such as DUNE-Gas.\n\n Only assuming the VUV emission band as is the case of most of the literature values, a mean w<\/jats:italic>\n sc<\/jats:sub>-value of 38.7 \u00b1 0.6 (sta.)+7.7<\/jats:sup>\n -7.2<\/jats:sub> (sys.) eV was obtained. If the UV-VIS emission band is to be considered, the average energy to produce a photon was determined to be w<\/jats:italic>\n 2nd<\/jats:sup>\n <\/jats:sub> = 43.5 \u00b1 0.7 (sta.)+8.7<\/jats:sup>\n -8.1<\/jats:sub> (sys.) eV and w<\/jats:italic>\n 3rd<\/jats:sup>\n <\/jats:sub> = 483 \u00b1 7 (sta.+110<\/jats:sup>\n -105<\/jats:sub> (sys.) eV, in the VUV and UV-VIS bands, respectively.<\/jats:p>","DOI":"10.1088\/1475-7516\/2024\/06\/041","type":"journal-article","created":{"date-parts":[[2024,6,19]],"date-time":"2024-06-19T13:45:15Z","timestamp":1718804715000},"page":"041","update-policy":"https:\/\/doi.org\/10.1088\/crossmark-policy","source":"Crossref","is-referenced-by-count":9,"title":["Understanding the xenon primary scintillation yield for cutting-edge rare event experiments"],"prefix":"10.1088","volume":"2024","author":[{"ORCID":"https:\/\/orcid.org\/0000-0002-1218-181X","authenticated-orcid":false,"given":"C.A.O.","family":"Henriques","sequence":"first","affiliation":[]},{"ORCID":"https:\/\/orcid.org\/0000-0003-3579-5715","authenticated-orcid":false,"given":"J.M.R.","family":"Teixeira","sequence":"additional","affiliation":[]},{"ORCID":"https:\/\/orcid.org\/0000-0002-1957-2274","authenticated-orcid":false,"given":"P.A.O.C.","family":"Silva","sequence":"additional","affiliation":[]},{"ORCID":"https:\/\/orcid.org\/0000-0003-2920-7067","authenticated-orcid":false,"given":"R.D.P.","family":"Mano","sequence":"additional","affiliation":[]},{"ORCID":"https:\/\/orcid.org\/0000-0002-8841-6523","authenticated-orcid":false,"given":"J.M.F.","family":"dos Santos","sequence":"additional","affiliation":[]},{"ORCID":"https:\/\/orcid.org\/0000-0002-1912-2804","authenticated-orcid":false,"given":"C.M.B.","family":"Monteiro","sequence":"additional","affiliation":[]}],"member":"266","published-online":{"date-parts":[[2024,6,19]]},"reference":[{"key":"b7518bf6013cda1079722108332128ecc","doi-asserted-by":"publisher","first-page":"052","DOI":"10.1007\/JHEP10(2019)052","article-title":"Demonstration of the event identification capabilities of the NEXT-White detector","volume":"10","author":"NEXT Collaboration","year":"2019","journal-title":"JHEP"},{"key":"b5c25f1ef37450f206488b969a6a635f8","doi-asserted-by":"publisher","DOI":"10.1016\/j.nima.2019.162803","article-title":"AXEL: High-pressure Xe gas TPC for BG-free 0\u03bd2\u03b2 decay search","volume":"958","author":"Obara","year":"2020","journal-title":"Nucl. 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