A sterile neutrino is a well-motivated and widely studied dark matter (DM) candidate. The most straightforward realization of sterile neutrino DM, through the Dodelson-Widrow (DW) mechanism, is now ruled out by a combination of X-ray and Lymana measurements. An alternative production mechanism that is becoming increasingly popular in the literature is the freeze-in mechanism, involving frameworks where a feeble coupling to a particle - usually a scalar beyond the Standard Model - in the thermal bath results in a gradual accumulation of the sterile neutrino DM abundance. This paper reviews the various motivations for realizing such frameworks in the literature, their common characteristic features and phenomenological signatures.
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Chinese Acad Sci, CAS Key Lab Theoret Phys, Inst Theoret Phys, Beijing 100190, Peoples R China
Univ Massachusetts Amherst, Amherst Ctr Fundamental Interact, Dept Phys, Amherst, MA 01003 USAChinese Acad Sci, CAS Key Lab Theoret Phys, Inst Theoret Phys, Beijing 100190, Peoples R China
Du, Yong
Huang, Fei
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Chinese Acad Sci, CAS Key Lab Theoret Phys, Inst Theoret Phys, Beijing 100190, Peoples R China
Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USAChinese Acad Sci, CAS Key Lab Theoret Phys, Inst Theoret Phys, Beijing 100190, Peoples R China
Huang, Fei
Li, Hao-Lin
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Chinese Acad Sci, CAS Key Lab Theoret Phys, Inst Theoret Phys, Beijing 100190, Peoples R ChinaChinese Acad Sci, CAS Key Lab Theoret Phys, Inst Theoret Phys, Beijing 100190, Peoples R China
Li, Hao-Lin
Yu, Jiang-Hao
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Chinese Acad Sci, CAS Key Lab Theoret Phys, Inst Theoret Phys, Beijing 100190, Peoples R China
Univ Chinese Acad Sci, Sch Phys Sci, Beijing 100049, Peoples R China
Univ Chinese Acad Sci, Hangzhou Inst Adv Study, Sch Fundamental Phys & Math Sci, Hangzhou 310024, Peoples R China
Int Ctr Theoret Phys Asia Pacific, Beijing, Peoples R ChinaChinese Acad Sci, CAS Key Lab Theoret Phys, Inst Theoret Phys, Beijing 100190, Peoples R China
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CNRS, Pole Theorie, Lab Phys Infinis Irene Joliot Curie 2, UMR 9012,IN2P3, 15 Rue Georges Clemenceau, F-91400 Orsay, FranceCNRS, Pole Theorie, Lab Phys Infinis Irene Joliot Curie 2, UMR 9012,IN2P3, 15 Rue Georges Clemenceau, F-91400 Orsay, France
Abada, A.
Arcadi, G.
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Univ Messina, Dipartimento Sci Matemat & Informat Sci Fis & Sci, Via Ferdinando Stagno dAlcontres 31, I-98166 Messina, Italy
INFN, Sez Catania, Via Santa Sofia 64, I-95123 Catania, ItalyCNRS, Pole Theorie, Lab Phys Infinis Irene Joliot Curie 2, UMR 9012,IN2P3, 15 Rue Georges Clemenceau, F-91400 Orsay, France
Arcadi, G.
Lucente, M.
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Univ Bologna, Dipartimento Fis & Astron, Via Irnerio 46, I-40126 Bologna, Italy
INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, ItalyCNRS, Pole Theorie, Lab Phys Infinis Irene Joliot Curie 2, UMR 9012,IN2P3, 15 Rue Georges Clemenceau, F-91400 Orsay, France
Lucente, M.
Piazza, G.
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CNRS, Pole Theorie, Lab Phys Infinis Irene Joliot Curie 2, UMR 9012,IN2P3, 15 Rue Georges Clemenceau, F-91400 Orsay, FranceCNRS, Pole Theorie, Lab Phys Infinis Irene Joliot Curie 2, UMR 9012,IN2P3, 15 Rue Georges Clemenceau, F-91400 Orsay, France
Piazza, G.
Rosauro-Alcaraz, S.
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CNRS, Pole Theorie, Lab Phys Infinis Irene Joliot Curie 2, UMR 9012,IN2P3, 15 Rue Georges Clemenceau, F-91400 Orsay, FranceCNRS, Pole Theorie, Lab Phys Infinis Irene Joliot Curie 2, UMR 9012,IN2P3, 15 Rue Georges Clemenceau, F-91400 Orsay, France
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Univ Antonio Narino, Ctr Invest, Carrera 3 Este 47A-15, Bogota, Colombia
Univ Warsaw, Inst Theoret Phys, Fac Phys, Ul Pasteura 5, PL-02093 Warsaw, PolandUniv Antonio Narino, Ctr Invest, Carrera 3 Este 47A-15, Bogota, Colombia
Barman, Basabendu
Dev, P. S. Bhupal
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Washington Univ, Dept Phys, St Louis, MO 63130 USA
Washington Univ, McDonnell Ctr Space Sci, St Louis, MO 63130 USA
Fermilab Natl Accelerator Lab, Theoret Phys Dept, POB 500, Batavia, IL 60510 USAUniv Antonio Narino, Ctr Invest, Carrera 3 Este 47A-15, Bogota, Colombia
Dev, P. S. Bhupal
Ghoshal, Anish
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Univ Warsaw, Inst Theoret Phys, Fac Phys, Ul Pasteura 5, PL-02093 Warsaw, PolandUniv Antonio Narino, Ctr Invest, Carrera 3 Este 47A-15, Bogota, Colombia