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Electroweak-interacting spin-1 dark matter and its phenomenology / Motoko Fujiwara.

SpringerLink Books Physics and Astronomy eBooks 2023 Available online

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Format:
Book
Author/Creator:
Fujiwara, Motoko, author.
Series:
Springer Theses, Recognizing Outstanding Ph.D. Research, 2190-5061
Language:
English
Subjects (All):
Dark matter (Astronomy).
Nuclear spin.
Particles (Nuclear physics).
Physical Description:
1 online resource (104 pages)
Edition:
1st ed. 2023.
Place of Publication:
Singapore : Springer Nature Singapore Pte Ltd., [2023]
Summary:
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.
Contents:
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.
Notes:
Description based on print version record.
Includes bibliographical references.
Other Format:
Print version: Fujiwara, Motoko Electroweak-Interacting Spin-1 Dark Matter and Its Phenomenology
ISBN:
9789819910359
OCLC:
1378934893

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