文献类型：期刊文献

英文题名：A White Paper on keV sterile neutrino Dark Matter

作者：Adhikari, R.[62];Agostini, M.[85];Ky, N. Anh[39,74];Araki, T.[58];Archidiacono, M.[34];Bahr, M.[71];Baur, J.[2];Behrens, J.[70];Bezrukov, F.[65];Dev, P. S. Bhupal[31];Borah, D.[35];Boyarsky, A.[45];de Gouvea, A.[63];Pires, C. A. de S.[37];de Vega, H. J.[9];Dias, A. G.[36];Di Bari, P.[32];Djurcic, Z.[21];Dolde, K.[7];Dorrer, H.[82];Durero, M.[2];Dragoun, O.[72];Drewes, M.[1];Drexlin, G.[30];Duellmann, Ch. E.[82,84];Eberhardt, K.[82];Eliseev, S.[87];Enss, C.[50];Evans, N. W.[54];Faessler, A.[86];Filianin, P.[87];Fischer, V.[2];Fleischmann, A.[50];Formaggio, J. A.[20];Franse, J.[16];Fraenkle, F. M.[7];Frenk, C. S.[64];Fuller, G.[76];Gastaldo, L.[50];Garzilli, A.[16];Giunti, C.[22];Glueck, F.[7,67];Goodman, M. C.[21];Gonzalez-Garcia, M. C.[19];Gorbunov, D.[66,73];Hamann, J.[40];Hannen, V.[70];Hannestad, S.[34];Hansen, S. H.[33];Hassel, C.[50];Heeck, J.[11];Hofmann, F.[81];Houdy, T.[2,4];Huber, A.[7];Lakubovskyi, D.[43,90];Lanni, A.[28];Ibarra, A.[1];Jacobsson, R.[88];Jeltema, T.[77];Jochum, J.[12,13];Kempf, S.[50];Kieck, T.[82,83];Korzeczek, M.[2,7];Kornoukhov, V.[42];Lachenmaier, T.[13];Laine, M.[75];Langacker, P.[67,68];Lasserre, T.[1,2,3,4];Lesgourgues, J.[15];Lhuillier, D.[2];Li, Y. F.[78];Liao, W.[80];Long, A. W.[91];Maltoni, M.[26,27];Mangano, G.[24];Mavromatos, N. E.[44];Menci, N.[59];Merle, A.[5];Mertens, S.[6,7];Mirizzi, A.[25,46];Monrea, B.[71];Nozik, A.[66,73];Neronov, A.[49];Niro, V.[26,27];Novikov, Y.[52,53];Oberauer, L.[1];Otten, E.[83];Palanque-Delabrouille, N.[2];Pallavicini, M.[23];Pantuev, V. S.[66];Papastergis, E.[51];Parke, S.[79];Pascoli, S.[56];Pastor, S.[29];Patwardhan, A.[76];Pilaftsis, A.[55];Radford, D. C.[92];Ranitzsch, P. C. -O.[70];Rest, O.[70];Robinson, D. J.[17];Rodrigues da Silva, P. S.[37];Ruchayskiy, O.[10,90];Sanchez, N. G.[8];Sasaki, M.[12];Saviano, N.[14,56];Schneider, A.[61];Schneider, F.[82,83];Schwetz, T.[30];Schoenert, S.[1];Scholl, S.[12];Shankar, F.[32];Shrock, R.[19];Steinbrink, N.[70];Strigari, L.[57];Suekane, F.[41];Suerfu, B.[69];Takahashi, R.[38];Thi Hong Van, N.[39];Tkachev, I.[66];Totzauer, M.[5];Tsai, Y.[18];Tully, C. G.[69];Valerius, K.[7];Valle, J. W. F.[29];Venos, D.[72];Viel, M.[47,48];Vivier, M.[2];Wang, M. Y.[60];Weinheimer, C.[70];Wendt, K.[83];Winslow, L.[20];Wolf, J.[7];Wurm, M.[14];Xing, Z.[78];Zhou, S.[78];Zuber, K.[89]

机构：[1]Tech Univ Munich, Phys Dept & Excellence Cluster Univ, James Franck Str 1, D-85748 Garching, Germany;[2]Commissariat Energie Atom & Energ Alternat, Ctr Saclay, DSM, IRFU, F-91191 Gif Sur Yvette, France;[3]Tech Univ Munich, Inst Adv Study, James Franck Str 1, D-85748 Garching, Germany;[4]Univ Paris Diderot, Astroparticule & Cosmol, CNRS, IN2P3,CEA,IRFU,Observ Paris,Sorbonne Paris Cite, F-75205 Paris 13, France;[5]Max Planck Inst Phys & Astrophys, Werner Heisenberg Inst, Foehringer Ring 6, D-80805 Munich, Germany;[6]Inst Nucl & Particle Astrophys, Lawrence Berkeley Lab, Berkeley, CA 94720 USA;[7]KCETA, Karlsruhe Inst Technol, D-76021 Karlsruhe, Germany;[8]Sorbonne Univ, UPMC, CNRS, LERMA,Observ Paris,PSL, Paris, France;[9]UPMC Univ P&M Curie Paris VI, CNRS, LPTHE, Paris, France;[10]Ecole Polytech Fed Lausanne, FSB, ITP, LPPC,BSP, CH-1015 Lausanne, Switzerland;[11]Univ Libre Bruxelles, Serv Phys Theor, Blvd Triomphe,CP225, B-1050 Brussels, Belgium;[12]Univ Tubingen, Inst Astron & Astrophys, Kepler Ctr Astro & Particle Phys, Tubingen, Germany;[13]Eberhard Karls Univ Tubingen, Phys Inst, D-72076 Tubingen, Germany;[14]Johannes Gutenberg Univ Mainz, Inst Phys & EC PRISMA, Mainz, Germany;[15]Rhein Westfal TH Aachen, Inst Theoret Particle Phys & Cosmol TTK, D-52056 Aachen, Germany;[16]Leiden Univ, Lorentz Inst, Niels Bohrweg 2, NL-2333 CA Leiden, Netherlands;[17]Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA;[18]Univ Maryland, Maryland Ctr Fundamental Phys, College Pk, MD 20742 USA;[19]SUNY Stony Brook, CN Yang Inst Theoret Phys, Stony Brook, NY 11794 USA;[20]MIT, Cambridge, MA 02139 USA;[21]Argonne Natl Lab, Argonne, IL 60439 USA;[22]INFN, Sez Torino, Via P Giuria 1, I-10125 Turin, Italy;[23]Univ Genoa, Dipartimento Fis, Via Dodecaneso 33, I-16146 Genoa, Italy;[24]INFN, Sez Napoli, Via Cintia, I-80126 Naples, Italy;[25]Dipartimento Interateneo Fis Michelangelo Merlin, Via Amendola 173, I-70126 Bari, Italy;[26]Univ Autonoma Madrid, Dept Fis Teor, Calle Nicolas Cabrera 13-15, E-28049 Madrid, Spain;[27]UMA, Inst Fis Teor, CSIC, Calle Nicolas Cabrera 13-15, E-28049 Madrid, Spain;[28]Lab Subterraneo Canfranc Paseo Ayerbe, S-N 22880, Canfranc Estacion, Huesca, Spain;[29]Univ Valencia, CSIC, Inst Fis Corpuscular, Valencia, Spain; Univ Autonoma Madrid, Inst Fis Teor, UAM, CSIC, Calle Nicolas Cabrera 13-15, E-28049 Madrid, Spain;[30]Karlsruhe Inst Technol, Inst Kernphys, D-76021 Karlsruhe, Germany;[31]Univ Manchester, Sch Phys & Astron, Consortium Fundamental Phys, Manchester M13 9PL, Lancs, England;[32]Univ Southampton, Sch Phys & Astron, Southampton SO17 1BJ, Hants, England;[33]Univ Copenhagen, Niels Bohr Inst, Dark Cosmol Ctr, Juliane Maries Vej 30, DK-2100 Copenhagen, Denmark;[34]Univ Aarhus, Dept Phys & Astron, DK-8000 Aarhus C, Denmark;[35]Indian Inst Technol Guwahati, Dept Phys, Gauhati 781039, Assam, India;[36]Univ Fed Abc, Ctr Ciencias Nat & Humanas, Av Estados 5001, BR-09210580 Santo Andre, SP, Brazil;[37]Univ Fed Paraiba, Dept Fis, Caixa Postal 5008, BR-58051970 Joao Pessoa, Paraiba, Brazil;[38]Shimane Univ, Grad Sch Sci & Engn, Matsue, Shimane, Japan;[39]Vietnam Acad Sci & Technol, Inst Phys, 10 Dao Tan, Hanoi, Vietnam;[40]Univ Sydney, Sydney Inst Astron, Sch Phys, Sydney, NSW 2006, Australia;[41]Tohoku Univ, RCNS, Sendai, Miyagi, Japan;[42]ITEP, Ul Bol Cheremushkinskaya 25, Moscow 117218, Russia;[43]Bogolyubov Inst Theoret Phys, 14-b Metrologichna Str, UA-03680 Kiev, Ukraine;[44]Kings Coll London, Phys Dept, Strand, London WC2R 2LS, England;[45]Leiden Univ, Inst Lorentz Theoret Phys, POB 9506, NL-2300 RA Leiden, Netherlands;[46]Ist Nazl Fis Nucl, Sez Bari, Via Amendola 173, I-70126 Bari, Italy;[47]Osserv Astron Trieste, OATs, INAF, Via Tiepolo 11, I-34143 Trieste, Italy;[48]Natl Inst Nucl Phys, INFN, Via Valerio 2, I-34127 Trieste, Italy;[49]Univ Geneva, Astron Dept, ISDC, Ch Ecogia 16, CH-1211 Geneva, Switzerland;[50]Heidelberg Univ, Kirchhoff Inst Phys, Neuenheimer Feld 227, D-69120 Heidelberg, Germany;[51]Univ Groningen, Kapteyn Astron Inst, Landleven 12, NL-9747 AD Groningen, Netherlands;[52]Petersburg Nucl Phys Inst, Gatchina 188300, Russia;[53]St Petersburg State Univ, St Petersburg 199034, Russia;[54]Inst Astron, Madingley Rd, Cambridge CB3 OHA, England;[55]Univ Manchester, Sch Phys & Astron, Manchester M13 9PL, Lancs, England;[56]Univ Durham, Inst Particle Phys Phenomenol, Dept Phys, Durham DH1 3LE, England;[57]Texas A&M Univ, Mitchell Inst Fundamental Phys & Astron, College Stn, TX 77843 USA;[58]Saitama Univ, Dept Phys, Sakura Ku, Shimo Okubo 255, Saitama, Japan;[59]INAF, Osservatorio Astron Roma, Via Frascati 33, I-00040 Monte Porzio Catone, Italy;[60]Texas A&M Univ, Mitchell Inst Fundamental Phys & Astron, Dept Phys & Astron, College Stn, TX 77843 USA;[61]Univ Zurich, Inst Computat Sci, CH-8057 Zurich, Switzerland;[62]Jamia Millia Islamia, Cent Univ, Ctr Theoret Phys, New Delhi 110025, India;[63]Northwestern Univ, Evanston, IL 60208 USA;[64]Univ Durham, Inst Computat Cosmol, Durham, England;[65]Univ Connecticut, Storrs, CT USA;[66]Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia;[67]Wigner Res Ctr Phys, Budapest, Hungary;[68]Inst Adv Study, Princeton, NJ 08540 USA;[69]Princeton Univ, Princeton, NJ 08542 USA;[70]Westfal Wilhelms Univ Munster, Inst Kernphys, Wilhelm Klemm Str 9, D-48149 Munster, Germany;[71]Univ Calif Santa Barbara, Santa Barbara, CA USA;[72]Nucl Phys Inst, ASCR, CZ-25068 Rez, Czech Republic;[73]MIPT, Inst Skiy Per 9, Dolgoprudnyi 141700, Moscow Region, Russia;[74]VNU Univ Sci, Fac Phys, Lab High Energy Phys & Cosmol, 334 Nguyen Trai, Hanoi, Vietnam;[75]Univ Bern, ITP, AEC, Sidlerstr 5, CH-3012 Bern, Switzerland;[76]Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA;[77]Univ Calif Santa Cruz, Santa Cruz, CA 95064 USA;[78]Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China;[79]Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA;[80]East China Univ Sci & Technol, Inst Modern Phys, Sch Sci, 130 Meilong Rd, Shanghai, Peoples R China;[81]Max Planck Inst Extraterr Phys, Giessenbachstr, D-85748 Garching, Germany;[82]Johannes Gutenberg Univ Mainz, Inst Kernchem, D-55099 Mainz, Germany;[83]Johannes Gutenberg Univ Mainz, Inst Phys, D-55099 Mainz, Germany;[84]GSI Helmholtzzentrum Schwerionenforsch, D-64291 Darmstadt, Germany;[85]Gran Sasso Sci Inst INFN, Laquila, Italy;[86]Univ Tubingen, Inst Theoret Phys, D-72076 Tubingen, Germany;[87]Max Planck Inst Kernphys, D-69117 Heidelberg, Germany;[88]European Org Nucl Res, CERN, Geneva, Switzerland;[89]Tech Univ Dresden, Inst Kern & Teilchenphys, Dresden, Germany;[90]Niels Bohr Inst, Discovery Ctr, Blegdamsvej 17, DK-2100 Copenhagen, Denmark;[91]Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA;[92]Oak Ridge Natl Lab, Oak Ridge, TN 37831 USA

年份：2017

期号：1

外文期刊名：JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS

收录：;WOS:【SCI-EXPANDED(收录号:WOS:000399409800025)】；

基金：The work of C. Giunti was partially supported by the research grant Theoretical Astroparticle Physics number 2012CPPYP7 under the program PRIN 2012 funded by the Ministero dellIstruzione, Universita e della Ricerca (MIUR). The authors of Section 2 would like to thank A. Vincent for discussion and comments. The work of A. Mirizzi is supported by the Italian Ministero dellIstruzione, Universita e Ricerca (MIUR) and Istituto Nazionale di Fisica Nucleare (INFN) through the Theoretical Astroparticle Physics projects. The work of A. Ibarra was supported in part by the DFG cluster of excellence Origin and Structure of the Universe and by the ERC Advanced Grant project FLAVOUR (267104). M. Viel is supported by the ERC StG cosmoIGM. The work of O. Dragoun was supported by the GACR (contract P203/12/1896) and the ASCR (contract IRP AV02 10480585). This work was supported in part by the Gottfried Wilhelm Leibniz Programme of the Deutsche Forschungsgemeinschaft (DFG) and the NSF grant PHY-1307372 at UCSD. M. Laine was supported in part by the Swiss National Science Foundation (SNF) under grant 200020-155935. A. Merle acknowledges partial support by the Micron Technology Foundation, Inc. V. Niro acknowledges support by Spanish MINECO through project FPA2012-31880, by Spanish MINECO (Centro de excelencia Severo Ochoa Program) under grant SEV-2012-0249 as well as the Spanish grants FPA2014-58183-P, Multidark CSD2009-00064 and SEV-2014-0398 (MINECO) and by the PROMETEOII/2014/084 grant from Generalitat Valenciana; the work of V. Niro was also supported by the Deutsche Forschungsgemeinschaft (DFG) through the Collaborative Research Centre SFB 676 Particles, Strings and the Early Universe (through an SFB fellowship). M. Drewes acknowledges support by the Gottfried Wilhelm Leibniz program of the Deutsche Forschungsgemeinschaft (DFG) and the DFG cluster of excellence Origin and Structure of the Universe. D. Robinson is supported by the NSF under grant No. PHY-1002399. Y. Tsai acknowledges support by the NSF under grant No. PHY-1315155 and the Maryland Center for Fundamental Physics. This research was partially supported by Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq), (A. Gomes Dias, C.A. de S. Pires, and P.S. Rodrigues da Silva,), by Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP), (A. Gomes Dias), and by the National Foundation for Science and Technology Development (NAFOSTED) of Vietnam under grant 103.03-2012.49 (N. Anh Ky and N. T. Hong Van). The work of J. Heeck is funded in part by IISN and by Belgian Science Policy (IAP VII/37). The work of N.E. Mavromatos is supported in part by the London Centre for Terauniverse Studies (LCTS), using funding from the European Research Council via the Advanced Investigator Grant 267352, and by the U.K. Science and Technology Facilities Council (STFC) under the research grants ST/J002798/1 and ST/L000326/1. The work of A. Pilaftsis is supported in part by the Lancaster-Manchester-Sheffield Consortium for Fundamental Physics, under STFC (UK) research grant: ST/J000418/1. L. Gastaldo would like to acknowledge the support by the DFG Research Unit FOR 2202 Neutrino Mass Determination by Electron Capture in 163Ho, ECH (funding under GA 2219/2-1). T. Lasserre would like to acknowledge the support of the Technische Universitat Munchen Institute for Advanced Study, funded by the German Excellence Initiative and the European Union Seventh Framework Programme under grant agreement No. 291763, as well as the European Union Marie Curie COFUND program. S. r r Mertens gratefully acknowledges support of a Feodor Lynen fellowship by the Alexander von Humboldt Foundation and support by the Helmholtz Association. R. Shrock acknowledges support from the U.S. NSF grants NSF-PHY-13-16617 and NSF-PHY-16-1620628. The work of Y. F. Li, W. Liao, and Z. Xing is supported in part by the National Natural Science Foundation of China under Grant No. 11135009. Several authors acknowledge (partial) support by the European Union through the FP7 Marie Curie Actions ITN INVISIBLES (PITN-GA-2011-289442). Furthermore, his project has received funding from the European Unions Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant agreements No. 690575 (InvisiblesPlus RISE) and No. 674896 (Elusives ITN).

语种：英文

外文关键词：cosmological neutrinos; dark matter experiments; dark matter theory; particle physics;cosmology connection

摘要：We present a comprehensive review of keV-scale sterile neutrino Dark Matter, collecting views and insights from all disciplines involved - cosmology, astrophysics, nuclear, and particle physics - in each case viewed from both theoretical and experimental/observational perspectives. After reviewing the role of active neutrinos in particle physics, astrophysics, and cosmology, we focus on sterile neutrinos in the context of the Dark Matter puzzle. Here, we first review the physics motivation for sterile neutrino Dark Matter, based on challenges and tensions in purely cold Dark Matter scenarios. We then round out the discussion by critically summarizing all known constraints on sterile neutrino Dark Matter arising from astrophysical observations, laboratory experiments, and theoretical considerations. In this context, we provide a balanced discourse on the possibly positive signal from X-ray observations. Another focus of the paper concerns the construction of particle physics models, aiming to explain how sterile neutrinos of keV-scale masses could arise in concrete settings beyond the Standard Model of elementary particle physics. The paper ends with an extensive review of current and future astrophysical and laboratory searches, highlighting new ideas and their experimental challenges, as well as future perspectives for the discovery of sterile neutrinos.