Ultralight bosons for strong gravity applications from simple Standard Model extensions

被引：24

作者：

Freitas, Felipe F. ^{[1
,2
]}

Herdeiro, Carlos A. R. ^{[2
,3
]}

Morais, Antonio P. ^{[2
]}

Onofre, Antonio ^{[4
]}

Pasechnik, Roman ^{[5
]}

Radu, Eugen ^{[2
]}

Sanchis-Gual, Nicolas ^{[2
,3
]}

Santos, Rui ^{[6
,7
]}

机构：

[1] Univ Aveiro, Dept Fis, Campus Santiago, P-3810183 Aveiro, Portugal

[2] Ctr Res & Dev Math & Applicat CIDMA, Campus Santiago, P-3810183 Aveiro, Portugal

[3] Univ Aveiro, Dept Matemat, Campus Santiago, P-3810183 Aveiro, Portugal

[4] Univ Minho, Ctr Fis Univ Minho Porto CF UM UP, P-4710057 Braga, Portugal

[5] Lund Univ, Dept Astron & Theoret Phys, S-22100 Lund, Sweden

[6] Inst Politecn Lisboa, ISEL Inst Super Engenharia Lisboa, P-1959007 Lisbon, Portugal

[7] Univ Lisbon, Ctr Fis Teor Computac, Fac Ciencias, Edificio C8, P-1749016 Campo Grande, MS, Portugal

来源：

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2021年 / 12期

基金：

欧盟地平线“2020”; 欧洲研究理事会; 瑞典研究理事会;

关键词：

axions; gravity; massive stars; particle physics - cosmology connection; HAIRY BLACK-HOLES; DARK-MATTER; SYMMETRY-BREAKING; STARS; SCALAR; SEARCHES; SYSTEMS; AXION;

D O I：

10.1088/1475-7516/2021/12/047

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We construct families, and concrete examples, of simple extensions of the Standard Model that can yield ultralight real or complex vectors or scalars with potential astrophysical relevance. Specifically, the mass range for these putative fundamental bosons (similar to 10(-10) - 10(-20) eV) would lead dynamically to both new non-black hole compact objects (bosonic stars) and new non-Kerr black holes, with masses of similar to M-circle dot to similar to 10(10)M(circle dot), corresponding to the mass range of astrophysical black hole candidates (from stellar mass to supermassive). For each model, we study the properties of the mass spectrum and interactions after spontaneous symmetry breaking, discuss its theoretical viability and caveats, as well as some of its potential and most relevant phenomenological implications linking them to the physics of compact objects.

引用

页数：38

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