π-axion and π-axiverse of dark QCD

被引:4
|
作者
Alexander, Stephon [1 ]
Gilmer, Humberto [1 ]
Manton, Tucker [1 ]
Mcdonough, Evan [2 ]
机构
[1] Brown Univ, Dept Phys, Providence, RI 02912 USA
[2] Univ Winnipeg, Dept Phys, Winnipeg, MB R3B 2E9, Canada
基金
美国国家科学基金会; 加拿大自然科学与工程研究理事会;
关键词
MATTER;
D O I
10.1103/PhysRevD.108.123014
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Axions and axionlike particles are a prominent dark matter candidate, drawing motivation in part from the axiverse of string theory. Axionlike particles can also arise as composite degrees of freedom of a dark sector, for example, as dark pions in dark quantum chromodynamics. In a dark Standard Model (SM) wherein all six quark flavors are light while the photon is massive, one finds a rich low-energy spectrum of stable and ultralight particles, in the form of neutral and charged dark scalars, and complex neutral scalars analogous to the SM kaon, with mass splittings determined by the mass and charge of the dark quarks. The model finds a natural portal to the visible sector via kinetic coupling of the dark and visible photons and consequent millicharges for dark matter. The dark matter can be a mixture of all these ultralight bosonic degrees of freedom and exhibits both parity-even and parity-odd interactions, making the theory testable at a wide variety of experiments. In context of dark QCD with Nf flavors of light quarks, this scenario predicts N2 f - 1 ultralight axionlike particles-effectively an axiverse from dark QCD. This "pi-axiverse" is consistent with but makes no recourse to string theory and is complementary to the conventional string theory axiverse.
引用
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页数:15
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