KATRIN: status and prospects for the neutrino mass and beyond
The Karlsruhe Tritium Neutrino (KATRIN) experiment is designed to measure a high-precision integral spectrum of the endpoint region of T 2 β decay, with the primary goal of probing the absolute mass scale of the neutrino. After a first tritium commissioning campaign in 2018, the experiment has been...
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| Veröffentlicht in: | J.Phys.G 2022-09, Vol.49 (10), p.100501 |
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| creator | Aker, M Balzer, M Batzler, D Beglarian, A Berlev, A Besserer, U Bieringer, B Block, F Bobien, S Bombelli, L Bornschein, L Chilingaryan, S Choi, W Cremonesi, O Debowski, K Díaz Barrero, D Doe, P J Dragoun, O Drexlin, G Edzards, F Eitel, K Ellinger, E Enomoto, S Felden, A Fiorini, C Fränkle, F M Franklin, G B Friedel, F Fulst, A Gavin, A S Glück, F Grande, A Gugiatti, M Gumbsheimer, R Hannen, V Helbing, K Hillesheimer, D Höhn, T Houdy, T Jansen, A Kellerer, J King, P Kleifges, M Klein, M Köllenberger, L Kopmann, A Korzeczek, M Krasch, B Krause, H Lebeda, O Lechner, P Lokhov, A Malcherek, E Manfrin, D Mark, M Marsteller, A Martin, E L Mazzola, E Melzer, C Mertens, S Mostafa, J Müller, K Neumann, H Niemes, S Oelpmann, P Parno, D S Pavan, M Pigliafreddo, A Priester, F Radford, D C Robertson, R G H Rodejohann, W Rodenbeck, C Röllig, M Ryšavý, M Schäfer, P Schimpf, L Schneidewind, S Schrank, M Schwemmer, A Šefčík, M Sibille, V Spanier, F Spreng, D Thorne, L A Thümmler, T Titov, N Trigilio, P Urban, K Voigt, P Weinheimer, C Weiss, E Welte, S Wiesinger, C Wilkerson, J F Wolf, J Wunderl, L Wüstling, S Xu, W Zadoroghny, S |
| description | The Karlsruhe Tritium Neutrino (KATRIN) experiment is designed to measure a high-precision integral spectrum of the endpoint region of T 2 β decay, with the primary goal of probing the absolute mass scale of the neutrino. After a first tritium commissioning campaign in 2018, the experiment has been regularly running since 2019, and in its first two measurement campaigns has already achieved a sub-eV sensitivity. After 1000 days of data-taking, KATRIN’s design sensitivity is 0.2 eV at the 90% confidence level. In this white paper we describe the current status of KATRIN; explore prospects for measuring the neutrino mass and other physics observables, including sterile neutrinos and other beyond-Standard-Model hypotheses; and discuss research-and-development projects that may further improve the KATRIN sensitivity. |
| doi_str_mv | 10.1088/1361-6471/ac834e |
| format | Article |
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Triangle Universities Nuclear Laboratory ; University of North Carolina, Chapel Hill, NC (United States) ; Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)</creatorcontrib><description>The Karlsruhe Tritium Neutrino (KATRIN) experiment is designed to measure a high-precision integral spectrum of the endpoint region of T 2 β decay, with the primary goal of probing the absolute mass scale of the neutrino. After a first tritium commissioning campaign in 2018, the experiment has been regularly running since 2019, and in its first two measurement campaigns has already achieved a sub-eV sensitivity. After 1000 days of data-taking, KATRIN’s design sensitivity is 0.2 eV at the 90% confidence level. In this white paper we describe the current status of KATRIN; explore prospects for measuring the neutrino mass and other physics observables, including sterile neutrinos and other beyond-Standard-Model hypotheses; and discuss research-and-development projects that may further improve the KATRIN sensitivity.</description><identifier>ISSN: 0954-3899</identifier><identifier>EISSN: 1361-6471</identifier><identifier>DOI: 10.1088/1361-6471/ac834e</identifier><identifier>CODEN: JPGPED</identifier><language>eng</language><publisher>United States: IOP Publishing</publisher><subject>Astrophysics ; beyond standard model ; High Energy Physics - Experiment ; Instrumentation and Detectors ; krypton ; neutrino ; neutrino mass ; neutrino mass, tritium, sterile neutrinos ; Nuclear Experiment ; NUCLEAR PHYSICS AND RADIATION PHYSICS ; Physics ; PHYSICS OF ELEMENTARY PARTICLES AND FIELDS ; sterile neutrino ; tritium beta decay</subject><ispartof>J.Phys.G, 2022-09, Vol.49 (10), p.100501</ispartof><rights>The Author(s). 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A</creatorcontrib><creatorcontrib>Gugiatti, M</creatorcontrib><creatorcontrib>Gumbsheimer, R</creatorcontrib><creatorcontrib>Hannen, V</creatorcontrib><creatorcontrib>Helbing, K</creatorcontrib><creatorcontrib>Hillesheimer, D</creatorcontrib><creatorcontrib>Höhn, T</creatorcontrib><creatorcontrib>Houdy, T</creatorcontrib><creatorcontrib>Jansen, A</creatorcontrib><creatorcontrib>Kellerer, J</creatorcontrib><creatorcontrib>King, P</creatorcontrib><creatorcontrib>Kleifges, M</creatorcontrib><creatorcontrib>Klein, M</creatorcontrib><creatorcontrib>Köllenberger, L</creatorcontrib><creatorcontrib>Kopmann, A</creatorcontrib><creatorcontrib>Korzeczek, M</creatorcontrib><creatorcontrib>Krasch, B</creatorcontrib><creatorcontrib>Krause, H</creatorcontrib><creatorcontrib>Lebeda, O</creatorcontrib><creatorcontrib>Lechner, P</creatorcontrib><creatorcontrib>Lokhov, A</creatorcontrib><creatorcontrib>Malcherek, E</creatorcontrib><creatorcontrib>Manfrin, D</creatorcontrib><creatorcontrib>Mark, M</creatorcontrib><creatorcontrib>Marsteller, A</creatorcontrib><creatorcontrib>Martin, E L</creatorcontrib><creatorcontrib>Mazzola, E</creatorcontrib><creatorcontrib>Melzer, C</creatorcontrib><creatorcontrib>Mertens, S</creatorcontrib><creatorcontrib>Mostafa, J</creatorcontrib><creatorcontrib>Müller, K</creatorcontrib><creatorcontrib>Neumann, H</creatorcontrib><creatorcontrib>Niemes, S</creatorcontrib><creatorcontrib>Oelpmann, P</creatorcontrib><creatorcontrib>Parno, D S</creatorcontrib><creatorcontrib>Pavan, M</creatorcontrib><creatorcontrib>Pigliafreddo, A</creatorcontrib><creatorcontrib>Priester, F</creatorcontrib><creatorcontrib>Radford, D C</creatorcontrib><creatorcontrib>Robertson, R G H</creatorcontrib><creatorcontrib>Rodejohann, W</creatorcontrib><creatorcontrib>Rodenbeck, C</creatorcontrib><creatorcontrib>Röllig, M</creatorcontrib><creatorcontrib>Ryšavý, M</creatorcontrib><creatorcontrib>Schäfer, P</creatorcontrib><creatorcontrib>Schimpf, L</creatorcontrib><creatorcontrib>Schneidewind, S</creatorcontrib><creatorcontrib>Schrank, M</creatorcontrib><creatorcontrib>Schwemmer, A</creatorcontrib><creatorcontrib>Šefčík, M</creatorcontrib><creatorcontrib>Sibille, V</creatorcontrib><creatorcontrib>Spanier, F</creatorcontrib><creatorcontrib>Spreng, D</creatorcontrib><creatorcontrib>Thorne, L A</creatorcontrib><creatorcontrib>Thümmler, T</creatorcontrib><creatorcontrib>Titov, N</creatorcontrib><creatorcontrib>Trigilio, P</creatorcontrib><creatorcontrib>Urban, K</creatorcontrib><creatorcontrib>Voigt, P</creatorcontrib><creatorcontrib>Weinheimer, C</creatorcontrib><creatorcontrib>Weiss, E</creatorcontrib><creatorcontrib>Welte, S</creatorcontrib><creatorcontrib>Wiesinger, C</creatorcontrib><creatorcontrib>Wilkerson, J F</creatorcontrib><creatorcontrib>Wolf, J</creatorcontrib><creatorcontrib>Wunderl, L</creatorcontrib><creatorcontrib>Wüstling, S</creatorcontrib><creatorcontrib>Xu, W</creatorcontrib><creatorcontrib>Zadoroghny, S</creatorcontrib><creatorcontrib>Carnegie Mellon Univ., Pittsburgh, PA (United States)</creatorcontrib><creatorcontrib>Duke Univ., Durham, NC (United States). Triangle Universities Nuclear Laboratory</creatorcontrib><creatorcontrib>University of North Carolina, Chapel Hill, NC (United States)</creatorcontrib><creatorcontrib>Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)</creatorcontrib><title>KATRIN: status and prospects for the neutrino mass and beyond</title><title>J.Phys.G</title><addtitle>JPG</addtitle><addtitle>J. Phys. G: Nucl. Part. Phys</addtitle><description>The Karlsruhe Tritium Neutrino (KATRIN) experiment is designed to measure a high-precision integral spectrum of the endpoint region of T 2 β decay, with the primary goal of probing the absolute mass scale of the neutrino. After a first tritium commissioning campaign in 2018, the experiment has been regularly running since 2019, and in its first two measurement campaigns has already achieved a sub-eV sensitivity. After 1000 days of data-taking, KATRIN’s design sensitivity is 0.2 eV at the 90% confidence level. In this white paper we describe the current status of KATRIN; explore prospects for measuring the neutrino mass and other physics observables, including sterile neutrinos and other beyond-Standard-Model hypotheses; and discuss research-and-development projects that may further improve the KATRIN sensitivity.</description><subject>Astrophysics</subject><subject>beyond standard model</subject><subject>High Energy Physics - Experiment</subject><subject>Instrumentation and Detectors</subject><subject>krypton</subject><subject>neutrino</subject><subject>neutrino mass</subject><subject>neutrino mass, tritium, sterile neutrinos</subject><subject>Nuclear Experiment</subject><subject>NUCLEAR PHYSICS AND RADIATION PHYSICS</subject><subject>Physics</subject><subject>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</subject><subject>sterile neutrino</subject><subject>tritium beta 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Publishing</general><scope>O3W</scope><scope>TSCCA</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>1XC</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0002-3091-8088</orcidid><orcidid>https://orcid.org/0000-0001-5810-4345</orcidid><orcidid>https://orcid.org/0000-0002-8434-5692</orcidid><orcidid>https://orcid.org/0000-0002-7592-7914</orcidid><orcidid>https://orcid.org/0000000158104345</orcidid><orcidid>https://orcid.org/0000000230918088</orcidid></search><sort><creationdate>20220908</creationdate><title>KATRIN: status and prospects for the neutrino mass and beyond</title><author>Aker, M ; Balzer, M ; Batzler, D ; Beglarian, A ; Berlev, A ; Besserer, U ; Bieringer, B ; Block, F ; Bobien, S ; Bombelli, L ; Bornschein, L ; Chilingaryan, S ; Choi, W ; Cremonesi, O ; Debowski, K ; Díaz Barrero, D ; Doe, P J ; Dragoun, O ; Drexlin, G ; Edzards, F ; Eitel, K ; Ellinger, E ; Enomoto, S ; Felden, A ; Fiorini, C ; Fränkle, F M ; Franklin, G B ; Friedel, F ; Fulst, A ; Gavin, A S ; Glück, F ; Grande, A ; Gugiatti, M ; Gumbsheimer, R ; Hannen, V ; Helbing, K ; Hillesheimer, D ; Höhn, T ; Houdy, T ; Jansen, A ; Kellerer, J ; King, P ; Kleifges, M ; Klein, M ; Köllenberger, L ; Kopmann, A ; Korzeczek, M ; Krasch, B ; Krause, H ; Lebeda, O ; Lechner, P ; Lokhov, A ; Malcherek, E ; Manfrin, D ; Mark, M ; Marsteller, A ; Martin, E L ; Mazzola, E ; Melzer, C ; Mertens, S ; Mostafa, J ; Müller, K ; Neumann, H ; Niemes, S ; Oelpmann, P ; Parno, D S ; Pavan, M ; Pigliafreddo, A ; Priester, F ; Radford, D C ; Robertson, R G H ; Rodejohann, W ; Rodenbeck, C ; Röllig, M ; Ryšavý, M ; Schäfer, P ; Schimpf, L ; Schneidewind, S ; Schrank, M ; Schwemmer, A ; Šefčík, M ; Sibille, V ; Spanier, F ; Spreng, D ; Thorne, L A ; Thümmler, T ; Titov, N ; Trigilio, P ; Urban, K ; Voigt, P ; Weinheimer, C ; Weiss, E ; Welte, S ; Wiesinger, C ; Wilkerson, J F ; Wolf, J ; Wunderl, L ; Wüstling, S ; Xu, W ; Zadoroghny, S</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c414t-3d6a7f645494ebdfe39f2b104c8763808d9cfe4a58d736a2e4d71990c8db71903</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Astrophysics</topic><topic>beyond standard model</topic><topic>High Energy Physics - Experiment</topic><topic>Instrumentation and Detectors</topic><topic>krypton</topic><topic>neutrino</topic><topic>neutrino mass</topic><topic>neutrino mass, tritium, sterile neutrinos</topic><topic>Nuclear Experiment</topic><topic>NUCLEAR PHYSICS AND RADIATION PHYSICS</topic><topic>Physics</topic><topic>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</topic><topic>sterile neutrino</topic><topic>tritium beta decay</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Aker, M</creatorcontrib><creatorcontrib>Balzer, M</creatorcontrib><creatorcontrib>Batzler, D</creatorcontrib><creatorcontrib>Beglarian, A</creatorcontrib><creatorcontrib>Berlev, A</creatorcontrib><creatorcontrib>Besserer, U</creatorcontrib><creatorcontrib>Bieringer, B</creatorcontrib><creatorcontrib>Block, F</creatorcontrib><creatorcontrib>Bobien, S</creatorcontrib><creatorcontrib>Bombelli, L</creatorcontrib><creatorcontrib>Bornschein, L</creatorcontrib><creatorcontrib>Chilingaryan, S</creatorcontrib><creatorcontrib>Choi, W</creatorcontrib><creatorcontrib>Cremonesi, O</creatorcontrib><creatorcontrib>Debowski, K</creatorcontrib><creatorcontrib>Díaz Barrero, D</creatorcontrib><creatorcontrib>Doe, P J</creatorcontrib><creatorcontrib>Dragoun, O</creatorcontrib><creatorcontrib>Drexlin, G</creatorcontrib><creatorcontrib>Edzards, F</creatorcontrib><creatorcontrib>Eitel, K</creatorcontrib><creatorcontrib>Ellinger, E</creatorcontrib><creatorcontrib>Enomoto, S</creatorcontrib><creatorcontrib>Felden, A</creatorcontrib><creatorcontrib>Fiorini, C</creatorcontrib><creatorcontrib>Fränkle, F M</creatorcontrib><creatorcontrib>Franklin, G B</creatorcontrib><creatorcontrib>Friedel, F</creatorcontrib><creatorcontrib>Fulst, A</creatorcontrib><creatorcontrib>Gavin, A S</creatorcontrib><creatorcontrib>Glück, F</creatorcontrib><creatorcontrib>Grande, A</creatorcontrib><creatorcontrib>Gugiatti, M</creatorcontrib><creatorcontrib>Gumbsheimer, R</creatorcontrib><creatorcontrib>Hannen, V</creatorcontrib><creatorcontrib>Helbing, K</creatorcontrib><creatorcontrib>Hillesheimer, D</creatorcontrib><creatorcontrib>Höhn, T</creatorcontrib><creatorcontrib>Houdy, T</creatorcontrib><creatorcontrib>Jansen, A</creatorcontrib><creatorcontrib>Kellerer, J</creatorcontrib><creatorcontrib>King, P</creatorcontrib><creatorcontrib>Kleifges, M</creatorcontrib><creatorcontrib>Klein, M</creatorcontrib><creatorcontrib>Köllenberger, L</creatorcontrib><creatorcontrib>Kopmann, A</creatorcontrib><creatorcontrib>Korzeczek, M</creatorcontrib><creatorcontrib>Krasch, B</creatorcontrib><creatorcontrib>Krause, H</creatorcontrib><creatorcontrib>Lebeda, O</creatorcontrib><creatorcontrib>Lechner, P</creatorcontrib><creatorcontrib>Lokhov, A</creatorcontrib><creatorcontrib>Malcherek, E</creatorcontrib><creatorcontrib>Manfrin, D</creatorcontrib><creatorcontrib>Mark, M</creatorcontrib><creatorcontrib>Marsteller, A</creatorcontrib><creatorcontrib>Martin, E L</creatorcontrib><creatorcontrib>Mazzola, E</creatorcontrib><creatorcontrib>Melzer, C</creatorcontrib><creatorcontrib>Mertens, S</creatorcontrib><creatorcontrib>Mostafa, J</creatorcontrib><creatorcontrib>Müller, K</creatorcontrib><creatorcontrib>Neumann, H</creatorcontrib><creatorcontrib>Niemes, S</creatorcontrib><creatorcontrib>Oelpmann, P</creatorcontrib><creatorcontrib>Parno, D S</creatorcontrib><creatorcontrib>Pavan, M</creatorcontrib><creatorcontrib>Pigliafreddo, A</creatorcontrib><creatorcontrib>Priester, F</creatorcontrib><creatorcontrib>Radford, D C</creatorcontrib><creatorcontrib>Robertson, R G H</creatorcontrib><creatorcontrib>Rodejohann, W</creatorcontrib><creatorcontrib>Rodenbeck, C</creatorcontrib><creatorcontrib>Röllig, M</creatorcontrib><creatorcontrib>Ryšavý, M</creatorcontrib><creatorcontrib>Schäfer, P</creatorcontrib><creatorcontrib>Schimpf, L</creatorcontrib><creatorcontrib>Schneidewind, S</creatorcontrib><creatorcontrib>Schrank, M</creatorcontrib><creatorcontrib>Schwemmer, A</creatorcontrib><creatorcontrib>Šefčík, M</creatorcontrib><creatorcontrib>Sibille, V</creatorcontrib><creatorcontrib>Spanier, F</creatorcontrib><creatorcontrib>Spreng, D</creatorcontrib><creatorcontrib>Thorne, L A</creatorcontrib><creatorcontrib>Thümmler, T</creatorcontrib><creatorcontrib>Titov, N</creatorcontrib><creatorcontrib>Trigilio, P</creatorcontrib><creatorcontrib>Urban, K</creatorcontrib><creatorcontrib>Voigt, P</creatorcontrib><creatorcontrib>Weinheimer, C</creatorcontrib><creatorcontrib>Weiss, E</creatorcontrib><creatorcontrib>Welte, S</creatorcontrib><creatorcontrib>Wiesinger, C</creatorcontrib><creatorcontrib>Wilkerson, J F</creatorcontrib><creatorcontrib>Wolf, J</creatorcontrib><creatorcontrib>Wunderl, L</creatorcontrib><creatorcontrib>Wüstling, S</creatorcontrib><creatorcontrib>Xu, W</creatorcontrib><creatorcontrib>Zadoroghny, S</creatorcontrib><creatorcontrib>Carnegie Mellon Univ., Pittsburgh, PA (United States)</creatorcontrib><creatorcontrib>Duke Univ., Durham, NC (United States). Triangle Universities Nuclear Laboratory</creatorcontrib><creatorcontrib>University of North Carolina, Chapel Hill, NC (United States)</creatorcontrib><creatorcontrib>Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)</creatorcontrib><collection>IOP Publishing Free Content</collection><collection>IOPscience (Open Access)</collection><collection>CrossRef</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>OSTI.GOV</collection><jtitle>J.Phys.G</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Aker, M</au><au>Balzer, M</au><au>Batzler, D</au><au>Beglarian, A</au><au>Berlev, A</au><au>Besserer, U</au><au>Bieringer, B</au><au>Block, F</au><au>Bobien, S</au><au>Bombelli, L</au><au>Bornschein, L</au><au>Chilingaryan, S</au><au>Choi, W</au><au>Cremonesi, O</au><au>Debowski, K</au><au>Díaz Barrero, D</au><au>Doe, P J</au><au>Dragoun, O</au><au>Drexlin, G</au><au>Edzards, F</au><au>Eitel, K</au><au>Ellinger, E</au><au>Enomoto, S</au><au>Felden, A</au><au>Fiorini, C</au><au>Fränkle, F M</au><au>Franklin, G B</au><au>Friedel, F</au><au>Fulst, A</au><au>Gavin, A S</au><au>Glück, F</au><au>Grande, A</au><au>Gugiatti, M</au><au>Gumbsheimer, R</au><au>Hannen, V</au><au>Helbing, K</au><au>Hillesheimer, D</au><au>Höhn, T</au><au>Houdy, T</au><au>Jansen, A</au><au>Kellerer, J</au><au>King, P</au><au>Kleifges, M</au><au>Klein, M</au><au>Köllenberger, L</au><au>Kopmann, A</au><au>Korzeczek, M</au><au>Krasch, B</au><au>Krause, H</au><au>Lebeda, O</au><au>Lechner, P</au><au>Lokhov, A</au><au>Malcherek, E</au><au>Manfrin, D</au><au>Mark, M</au><au>Marsteller, A</au><au>Martin, E L</au><au>Mazzola, E</au><au>Melzer, C</au><au>Mertens, S</au><au>Mostafa, J</au><au>Müller, K</au><au>Neumann, H</au><au>Niemes, S</au><au>Oelpmann, P</au><au>Parno, D S</au><au>Pavan, M</au><au>Pigliafreddo, A</au><au>Priester, F</au><au>Radford, D C</au><au>Robertson, R G H</au><au>Rodejohann, W</au><au>Rodenbeck, C</au><au>Röllig, M</au><au>Ryšavý, M</au><au>Schäfer, P</au><au>Schimpf, L</au><au>Schneidewind, S</au><au>Schrank, M</au><au>Schwemmer, A</au><au>Šefčík, M</au><au>Sibille, V</au><au>Spanier, F</au><au>Spreng, D</au><au>Thorne, L A</au><au>Thümmler, T</au><au>Titov, N</au><au>Trigilio, P</au><au>Urban, K</au><au>Voigt, P</au><au>Weinheimer, C</au><au>Weiss, E</au><au>Welte, S</au><au>Wiesinger, C</au><au>Wilkerson, J F</au><au>Wolf, J</au><au>Wunderl, L</au><au>Wüstling, S</au><au>Xu, W</au><au>Zadoroghny, S</au><aucorp>Carnegie Mellon Univ., Pittsburgh, PA (United States)</aucorp><aucorp>Duke Univ., Durham, NC (United States). Triangle Universities Nuclear Laboratory</aucorp><aucorp>University of North Carolina, Chapel Hill, NC (United States)</aucorp><aucorp>Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>KATRIN: status and prospects for the neutrino mass and beyond</atitle><jtitle>J.Phys.G</jtitle><stitle>JPG</stitle><addtitle>J. Phys. G: Nucl. Part. Phys</addtitle><date>2022-09-08</date><risdate>2022</risdate><volume>49</volume><issue>10</issue><spage>100501</spage><pages>100501-</pages><issn>0954-3899</issn><eissn>1361-6471</eissn><coden>JPGPED</coden><abstract>The Karlsruhe Tritium Neutrino (KATRIN) experiment is designed to measure a high-precision integral spectrum of the endpoint region of T 2 β decay, with the primary goal of probing the absolute mass scale of the neutrino. After a first tritium commissioning campaign in 2018, the experiment has been regularly running since 2019, and in its first two measurement campaigns has already achieved a sub-eV sensitivity. After 1000 days of data-taking, KATRIN’s design sensitivity is 0.2 eV at the 90% confidence level. In this white paper we describe the current status of KATRIN; explore prospects for measuring the neutrino mass and other physics observables, including sterile neutrinos and other beyond-Standard-Model hypotheses; and discuss research-and-development projects that may further improve the KATRIN sensitivity.</abstract><cop>United States</cop><pub>IOP Publishing</pub><doi>10.1088/1361-6471/ac834e</doi><tpages>62</tpages><orcidid>https://orcid.org/0000-0002-3091-8088</orcidid><orcidid>https://orcid.org/0000-0001-5810-4345</orcidid><orcidid>https://orcid.org/0000-0002-8434-5692</orcidid><orcidid>https://orcid.org/0000-0002-7592-7914</orcidid><orcidid>https://orcid.org/0000000158104345</orcidid><orcidid>https://orcid.org/0000000230918088</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0954-3899 |
| ispartof | J.Phys.G, 2022-09, Vol.49 (10), p.100501 |
| issn | 0954-3899 1361-6471 |
| language | eng |
| recordid | cdi_iop_journals_10_1088_1361_6471_ac834e |
| source | IOP Publishing Journals; Institute of Physics (IOP) Journals - HEAL-Link; Alma/SFX Local Collection |
| subjects | Astrophysics beyond standard model High Energy Physics - Experiment Instrumentation and Detectors krypton neutrino neutrino mass neutrino mass, tritium, sterile neutrinos Nuclear Experiment NUCLEAR PHYSICS AND RADIATION PHYSICS Physics PHYSICS OF ELEMENTARY PARTICLES AND FIELDS sterile neutrino tritium beta decay |
| title | KATRIN: status and prospects for the neutrino mass and beyond |
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