- [1]
R.D. Peccei and Helen R. Quinn, Phys. Rev. Lett.38, 1440 (1977)
- [2]
R.D. Peccei and Helen R. Quinn, Phys. Rev. D16, 1791 (1977)
- [3]
S. Weinberg, Phys. Rev. Lett.40, 223 (1978)
- [4]
F. Wilczek, Phys. Rev. Lett.40, 279 (1978)
- [5]
J. E. Kim, Phys. Rev. Lett.43, 103 (1979)
- [6]
M. A. Shifman, A. I. Vainshtein, and V. I. Zakharov, Nucl. Phys. B166, 493 (1980)
- [7]
M. Dine, W. Fischler, and M. Srednicki, Phys. Lett. B104, 199 (1981)
- [8]
A. R. Zhitnitsky, Sov. J. Nucl. Phys.31, 260 (1980)
- [9]
G. 't Hooft, Phys. Rev. Lett.37, 8 (1976)
- [10]
G. 't Hooft, Phys. Rev. D14, 3432 (1976)
- [11]
J. Preskill, M. B. Wise, and F. Wilczek, Phys. Lett. B120, 127 (1983)
- [12]
L.F. Abbott and P. Sikivie, Phys. Lett. B120, 133 (1983)
- [13]
M. Dine and W. Fischler, Phys. Lett. B120, 137 (1983)
- [14]
C. A. J. O'Hare, PoSCOSMICWISPers, 040 (2024), arXiv: 2403.17697[hep-ph]
- [15]
A. Hook, Phys. Rev. Lett.120, 261802 (2018), arXiv: 1802.10093[hep-ph]
- [16]
L. D. Luzio, B. Gavela, P. Quilezet al., JHEP05, 184 (2021), arXiv: 2102.00012[hep-ph]
- [17]
L. D. Luzio, B. Gavela, P. Quilezet al., JCAP10, 001 (2021), arXiv: 2102.01082[hep-ph]
- [18]
R. T. Co, L. J. Hall, and K. Harigaya, Phys. Rev. Lett.124, 251802 (2020), arXiv: 1910.14152[hep-ph]
- [19]
C. T. Hill and G. G. Ross, Nucl. Phys. B311, 253 (1988)
- [20]
R. Daido, N. Kitajima, and F. Takahashi, Phys. Rev. D93, 075027 (2016), arXiv: 1510.06675[hep-ph]
- [21]
D. Cyncynates and J. O. Thompson, Phys. Rev. D108, L091703 (2023), arXiv: 2306.04678[hep-ph]
- [22]
H. J. Li, Y. Q. Peng, W. Chaoet al., Phys. Lett. B849, 138444 (2024), arXiv: 2310.02126[hep-ph]
- [23]
L. Wolfenstein, Phys. Rev. D17, 2369 (1978)
- [24]
S. P. Mikheyev and A. Yu. Smirnov, Sov. J. Nucl. Phys.42, 913 (1985)
- [25]
S. P. Mikheev and A. Yu. Smirnov, Nuovo Cim. C9, 17 (1986)
- [26]
N. Kitajima and F. Takahashi, JCAP01, 032 (2015), arXiv: 1411.2011[hep-ph]
- [27]
S. Y. Ho, K. Saikawa, and F. Takahashi, JCAP10, 042 (2018), arXiv: 1806.09551[hep-ph]
- [28]
D. Cyncynates, T. Giurgica-Tiron, O. Simonet al., Phys. Rev. D105, 055005 (2022), arXiv: 2109.09755[hep-ph]
- [29]
H. J. Li, JCAP09, 025 (2024), arXiv: 2307.09245[hep-ph]
- [30]
R. Daido, N. Kitajima, and F. Takahashi, Phys. Rev. D92, 063512 (2015), arXiv: 1505.07670[hep-ph]
- [31]
D. Cyncynates, O. Simon, J. O. Thompsonet al., Phys. Rev. D106, 083503 (2022), arXiv: 2208.05501[hep-ph]
- [32]
Z. Chen, A. Kobakhidze, C. A. J. O'Hareet al.,Cosmology of the companion-axion model: dark matter, gravitational waves, and primordial black holes, (2021), arXiv: 2110.11014[hep-ph]
- [33]
H. J. Li and Y. F. Zhou, Chin. Phys. C49, 035101 (2025), arXiv: 2401.09138[hep-ph]
- [34]
K. Müürsepp, E. Nardi, and C. Smarra,Can the QCD axion feed a dark energy component? (2024), arXiv: 2405.00090[hep-ph]
- [35]
K. Müürsepp,On the viability of the QCD axion - dark energy transition”, (2024), arXiv: 2405.20478[hep-ph]
- [36]
E. Witten, Phys. Lett. B149, 351 (1984)
- [37]
M. B. Green and J. H. Schwarz, Phys. Lett. B149, 117 (1984)
- [38]
P. Svrcek and E. Witten, JHEP06, 051 (2006), arXiv: hep-th/0605206
- [39]
A. Arvanitaki, S. Dimopoulos, S. Dubovskyet al., Phys. Rev. D81, 123530 (2010), arXiv: 0905.4720[hep-th]
- [40]
M. Cicoli, M. Goodsell, and A. Ringwald, JHEP10, 146 (2012), arXiv: 1206.0819[hep-th]
- [41]
M. Demirtas, N. Gendler, C. Longet al., JHEP06, 092 (2023), arXiv: 2112.04503[hep-th]