Axion misalignment driven to the hilltop

被引:54
作者
Co, Raymond T. [1 ]
Gonzalez, Eric [1 ]
Harigaya, Keisuke [2 ]
机构
[1] Univ Michigan, Leinweber Ctr Theoret Phys, Dept Phys, 450 Church St, Ann Arbor, MI 48104 USA
[2] Inst Adv Study, Sch Nat Sci, 1 Einstein Dr, Princeton, NJ 08540 USA
关键词
Cosmology of Theories beyond the SM; Confinement; Supersymmetric Gauge Theory; Supersymmetric Standard Model; ELECTRIC-DIPOLE MOMENT; STRONG CP PROBLEM; QCD AXION; STRONGER QCD; CONSTRAINTS; INFLATION; COSMOLOGY; CONSERVATION; INVARIANCE; BREAKING;
D O I
10.1007/JHEP05(2019)163
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
The QCD axion serves as a well-motivated dark matter candidate and the misalignment mechanism is known to reproduce the observed abundance with a decay constant f(a) similar or equal to O(10(12)) GeV for a misalignment angle theta(mis) similar or equal to O(1). While f(a) << 10(12) GeV is of great experimental interest, the misalignment mechanism requires the axion to be very close to the hilltop, i.e. theta(mis) similar or equal to pi. This particular choice of theta(mis) has been understood as fine-tuning the initial condition. We offer a dynamical explanation for theta(mis) similar or equal to pi in a class of models. The axion dynamically relaxes to the minimum of the potential by virtue of an enhanced mass in the early universe. This minimum is subsequently converted to a hilltop because the CP phase of the theory shifts by when one contribution becomes subdominant to another with an opposite sign. We demonstrate explicit and viable examples in supersymmetric models where the higher dimensional Higgs coupling with the inflaton naturally achieves both criteria. Associated phenomenology includes a strikingly sharp prediction of 3 x 10(9) GeV less than or similar to f(a) less than or similar to 10(10) GeV and the absence of isocurvature perturbation.
引用
收藏
页数:22
相关论文
共 87 条
[1]   A COSMOLOGICAL BOUND ON THE INVISIBLE AXION [J].
ABBOTT, LF ;
SIKIVIE, P .
PHYSICS LETTERS B, 1983, 120 (1-3) :133-136
[2]   DYNAMICAL SUPERSYMMETRY BREAKING IN SUPERSYMMETRIC QCD [J].
AFFLECK, I ;
DINE, M ;
SEIBERG, N .
NUCLEAR PHYSICS B, 1984, 241 (02) :493-534
[3]   Improved limit on the electric dipole moment of the electron [J].
Andreev, V. ;
Ang, D. G. ;
DeMille, D. ;
Doyle, J. M. ;
Gabrielse, G. ;
Haefner, J. ;
Hutzler, N. R. ;
Lasner, Z. ;
Meisenhelder, C. ;
O'Leary, B. R. ;
Panda, C. D. ;
West, A. D. ;
West, E. P. ;
Wu, X. .
NATURE, 2018, 562 (7727) :355-+
[4]  
[Anonymous], hep-ph/9505253
[5]  
[Anonymous], ARXIV181007736
[6]  
[Anonymous], 2017, JINST
[7]   Conceptual design of the International Axion Observatory (IAXO) [J].
Armengaud, E. ;
Avignone, F. T. ;
Betz, M. ;
Brax, P. ;
Brun, P. ;
Cantatore, G. ;
Carmona, J. M. ;
Carosi, G. P. ;
Caspers, F. ;
Caspi, S. ;
Cetin, S. A. ;
Chelouche, D. ;
Christensen, F. E. ;
Dael, A. ;
Dafni, T. ;
Davenport, M. ;
Derbin, A. V. ;
Desch, K. ;
Diago, A. ;
Doebrich, B. ;
Dratchnev, I. ;
Dudarev, A. ;
Eleftheriadis, C. ;
Fanourakis, G. ;
Ferrer-Ribas, E. ;
Galan, J. ;
Garcia, J. A. ;
Garza, J. G. ;
Geralis, T. ;
Gimeno, B. ;
Giomataris, I. ;
Gninenko, S. ;
Gomez, H. ;
Gonzalez-Diaz, D. ;
Guendelman, E. ;
Hailey, C. J. ;
Hiramatsu, T. ;
Hoffmann, D. H. H. ;
Horns, D. ;
Iguaz, F. J. ;
Irastorza, I. G. ;
Isern, J. ;
Imai, K. ;
Jakobsen, A. C. ;
Jaeckel, J. ;
Jakovcic, K. ;
Kaminski, J. ;
Kawasaki, M. ;
Karuza, M. ;
Krcmar, M. .
JOURNAL OF INSTRUMENTATION, 2014, 9
[8]   Resonant Absorption of Bosonic Dark Matter in Molecules [J].
Arvanitaki, Asimina ;
Dimopoulos, Savas ;
Van Tilburg, Ken .
PHYSICAL REVIEW X, 2018, 8 (04)
[9]   Resonantly Detecting Axion-Mediated Forces with Nuclear Magnetic Resonance [J].
Arvanitaki, Asimina ;
Geraci, Andrew A. .
PHYSICAL REVIEW LETTERS, 2014, 113 (16)
[10]   Updating the axion cold dark matter energy density [J].
Bae, Kyu Jung ;
Huh, Ji-Haeng ;
Kim, Jihn E. .
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2008, (09)