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[null,"1.","Record Nr.",null,"UNINA9910720060403321"]
[null,null,"Autore",null,"Fujiwara Motoko"]
[null,null,"Titolo",null,"Electroweak-interacting spin-1 dark matter and its phenomenology / / Motoko Fujiwara"]
[null,null,"Pubbl/distr/stampa",null,"Singapore : , : Springer Nature Singapore Pte Ltd., , [2023]"]
[{"$nulls":4},"©2023"]
[null,null,"ISBN",null,"9789819910359"]
[{"$nulls":4},"9789819910342"]
[null,null,"Edizione",null,"[1st ed. 2023.]"]
[null,null,"Descrizione fisica",null,"1 online resource (104 pages)"]
[null,null,"Collana",null,"Springer Theses, Recognizing Outstanding Ph.D. Research, , 2190-5061"]
[null,null,"Disciplina",null,"523.1126"]
[null,null,"Soggetti",null,"Dark matter (Astronomy)"]
[{"$nulls":4},"Nuclear spin"]
[{"$nulls":4},"Particles (Nuclear physics)"]
[null,null,"Lingua di pubblicazione",null,"Inglese"]
[null,null,"Formato",null,"Materiale a stampa"]
[null,null,null,"Livello bibliografico","Monografia"]
[null,null,null,"Nota di bibliografia","Includes bibliographical references."]
[null,null,"Nota di contenuto",null,"Introduction -- WIMP Dark Matter and Its Thermal History -- Electroweakly Interacting Spin-1 Dark Matter -- Non-Relativistic Effective Field Theory For Spin-1 Dark Matter -- Thermal Relic Evaluation -- Gamma-ray Signatures and Dark Matter Spin Discrimination -- Conclusions -- Appendix."]
[null,null,null,"Sommario/riassunto","This book offers construction of a renormalizable effective theory of electroweak-interacting spin-1 dark matter (DM). The effective theory realizes minimal but essential features of DM predicted in extra-dimension models, and enables to systematically treat non-perturbative corrections such as the Sommerfeld effects. Deriving an annihilation cross section including the Sommerfeld effects based on the effective theory, the author discusses the future sensitivity of observations to gamma-ray from the Galactic Center. As a result, the author explains the monochromatic gamma-ray signatures originate from two photons (γγ) or photon and Z boson (γZ) produced in the process of DM annihilations, and concludes a possible scenario that unstable neutral spin-1 particles (Z’) appear and results in a spectral peak in addition to the one caused by γγ and γZ channels in gamma-ray observations. If those two spectral peaks are observed, the masses of spin-1 DM and Z’ would be reconstructed."]