參考文獻 |
[1] R. D. Peccei and Helen R. Quinn. “CP Conservation in the Presence of Pseudoparticles”. In: Phys. Rev. Lett. 38 (25 1977), pp. 1440–1443. DOI: 10.1103/PhysRevLett.
38.1440. URL: https://link.aps.org/doi/10.1103/PhysRevLett.38.
1440.
[2] Steven Weinberg. “A New Light Boson?” In: Phys. Rev. Lett. 40 (4 1978), pp. 223–226.
DOI: 10.1103/PhysRevLett.40.223. URL: https://link.aps.org/doi/10.
1103/PhysRevLett.40.223.
[3] F. Wilczek. “Problem of Strong P and T Invariance in the Presence of Instantons”. In:
Phys. Rev. Lett. 40 (5 1978), pp. 279–282. DOI: 10.1103/PhysRevLett.40.279. URL:
https://link.aps.org/doi/10.1103/PhysRevLett.40.279.
[4] S. Borsanyi et al. “Calculation of the axion mass based on high-temperature lattice
quantum chromodynamics”. In: Nature 539.7627 (2016), pp. 69–71. DOI: 10.1038/
nature20115. arXiv: 1606.07494 [hep-lat].
[5] Michael Dine et al. “Axions, Instantons, and the Lattice”. In: Phys. Rev. D 96.9 (2017),
p. 095001. DOI: 10.1103/PhysRevD.96.095001. arXiv: 1705.00676 [hep-ph].
[6] Takashi Hiramatsu et al. “Improved estimation of radiated axions from cosmological
axionic strings”. In: Phys. Rev. D 83 (2011), p. 123531. DOI: 10.1103/PhysRevD.83.
123531. arXiv: 1012.5502 [hep-ph].
[7] Masahiro Kawasaki, Ken’ichi Saikawa, and Toyokazu Sekiguchi. “Axion dark matter
from topological defects”. In: Phys. Rev. D 91.6 (2015), p. 065014. DOI: 10 . 1103 /
PhysRevD.91.065014. arXiv: 1412.0789 [hep-ph].
73
[8] Evan Berkowitz, Michael I. Buchoff, and Enrico Rinaldi. “Lattice QCD input for axion
cosmology”. In: Phys. Rev. D 92.3 (2015), p. 034507. DOI: 10.1103/PhysRevD.92.
034507. arXiv: 1505.07455 [hep-ph].
[9] Leesa Fleury and Guy D. Moore. “Axion dark matter: strings and their cores”. In: J.
Cosmol. Astropart. Phys. 01.2016 (2016), pp. 004–004. DOI: 10 . 1088 / 1475 - 7516 /
2016/01/004. URL: https://doi.org/10.1088/1475-7516/2016/01/004.
[10] Claudio Bonati et al. “Axion phenomenology and θ-dependence from Nf = 2 + 1
lattice QCD”. In: JHEP 03.2016 (2016), p. 155. DOI: 10.1007/JHEP03(2016)155.
arXiv: 1512.06746 [hep-lat].
[11] Peter Petreczky, Hans-Peter Schadler, and Sayantan Sharma. “The topological susceptibility in finite temperature QCD and axion cosmology”. In: Phys. Lett. B 762 (2016),
pp. 498–505. DOI: 10 . 1016 / j . physletb . 2016 . 09 . 063. arXiv: 1606 . 03145
[hep-lat].
[12] Guillermo Ballesteros et al. “Unifying inflation with the axion, dark matter, baryogenesis and the seesaw mechanism”. In: Phys. Rev. Lett. 118.7 (2017), p. 071802. DOI:
10.1103/PhysRevLett.118.071802. arXiv: 1608.05414 [hep-ph].
[13] Vincent B. Klaer and Guy D. Moore. “The dark-matter axion mass”. In: J. Cosmol. Astropart. Phys. 11.2017 (2017), p. 049. DOI: 10 . 1088 / 1475 - 7516 / 2017 / 11 / 049.
arXiv: 1708.07521 [hep-ph].
[14] Malte Buschmann, Joshua W. Foster, and Benjamin R. Safdi. “Early-Universe Simulations of the Cosmological Axion”. In: Phys. Rev. Lett. 124.16 (2020), p. 161103. DOI:
10.1103/PhysRevLett.124.161103. arXiv: 1906.00967 [astro-ph.CO].
[15] Marco Gorghetto, Edward Hardy, and Giovanni Villadoro. “More axions from strings”.
In: SciPost Phys. 10.2 (2021), p. 050. DOI: 10.21468/SciPostPhys.10.2.050. arXiv:
2007.04990 [hep-ph].
74
[16] Malte Buschmann et al. “Dark matter from axion strings with adaptive mesh refinement”. In: Nature Commun. 13.1 (2022), p. 1049. DOI: 10.1038/s41467-022-28669-
y. arXiv: 2108.05368 [hep-ph].
[17] P. Sikivie. “Experimental Tests of the "Invisible" Axion”. In: Phys. Rev. Lett. 51 (16 1983),
pp. 1415–1417. DOI: 10.1103/PhysRevLett.51.1415. URL: https://link.
aps.org/doi/10.1103/PhysRevLett.51.1415.
[18] P. Sikivie. “Detection rates for “invisible”-axion searches”. In: Phys. Rev. D 32 (11 1985),
pp. 2988–2991. DOI: 10.1103/PhysRevD.32.2988. URL: https://link.aps.
org/doi/10.1103/PhysRevD.32.2988.
[19] Jihn E. Kim. “Weak Interaction Singlet and Strong CP Invariance”. In: Phys. Rev. Lett.
43 (1979), p. 103. DOI: 10.1103/PhysRevLett.43.103.
[20] Mikhail A. Shifman, A. I. Vainshtein, and Valentin I. Zakharov. “Can Confinement
Ensure Natural CP Invariance of Strong Interactions?” In: Nucl. Phys. B 166 (1980),
pp. 493–506. DOI: 10.1016/0550-3213(80)90209-6.
[21] Michael Dine, Willy Fischler, and Mark Srednicki. “A Simple Solution to the Strong
CP Problem with a Harmless Axion”. In: Phys. Lett. B 104 (1981), pp. 199–202. DOI:
10.1016/0370-2693(81)90590-6.
[22] A. R. Zhitnitsky. “On Possible Suppression of the Axion Hadron Interactions. (In Russian)”. In: Sov. J. Nucl. Phys. 31 (1980), p. 260.
[23] C. Hagmann et al. “Results from a High-Sensitivity Search for Cosmic Axions”. In:
Phys. Rev. Lett. 80 (10 1998), pp. 2043–2046. DOI: 10.1103/PhysRevLett.80.2043.
URL: https://link.aps.org/doi/10.1103/PhysRevLett.80.2043.
[24] S. J. Asztalos et al. “Experimental Constraints on the Axion Dark Matter Halo Density”. In: The Astrophysical Journal 571.1 (2002), pp. L27–L30. DOI: 10.1086/341130.
URL: https://doi.org/10.1086/341130.
75
[25] S. J. Asztalos et al. “Improved rf cavity search for halo axions”. In: Phys. Rev. D 69 (1
2004), 011101 (R). DOI: 10.1103/PhysRevD.69.011101. URL: https://link.
aps.org/doi/10.1103/PhysRevD.69.011101.
[26] S. J. Asztalos et al. “SQUID-Based Microwave Cavity Search for Dark-Matter Axions”.
In: Phys. Rev. Lett. 104 (4 2010), p. 041301. DOI: 10 . 1103 / PhysRevLett . 104 .
041301. URL: https://link.aps.org/doi/10.1103/PhysRevLett.104.
041301.
[27] N. Du et al. “Search for Invisible Axion Dark Matter with the Axion Dark Matter Experiment”. In: Phys. Rev. Lett. 120 (15 2018), p. 151301. DOI: 10.1103/PhysRevLett.
120.151301. URL: https://link.aps.org/doi/10.1103/PhysRevLett.
120.151301.
[28] T. Braine et al. “Extended Search for the Invisible Axion with the Axion Dark Matter
Experiment”. In: Phys. Rev. Lett. 124 (10 2020), p. 101303. DOI: 10.1103/PhysRevLett.
124.101303. URL: https://link.aps.org/doi/10.1103/PhysRevLett.
124.101303.
[29] C. Bartram et al. “Search for Invisible Axion Dark Matter in the 3.3–4.2 µeV Mass
Range”. In: Phys. Rev. Lett. 127.26 (2021), p. 261803. DOI: 10.1103/PhysRevLett.
127.261803.
[30] S. Lee et al. “Axion Dark Matter Search around 6.7 µeV”. In: Phys. Rev. Lett. 124.10
(2020), p. 101802. DOI: 10.1103/PhysRevLett.124.101802. arXiv: 2001.05102
[hep-ex].
[31] Junu Jeong et al. “Search for Invisible Axion Dark Matter with a Multiple-Cell Haloscope”. In: Phys. Rev. Lett. 125.22 (2020), p. 221302. DOI: 10.1103/PhysRevLett.
125.221302. arXiv: 2008.10141 [hep-ex].
[32] Ohjoon Kwon et al. “First Results from an Axion Haloscope at CAPP around 10.7 µeV”.
In: Phys. Rev. Lett. 126 (19 2021), p. 191802. DOI: 10 . 1103 / PhysRevLett . 126 .
191802. URL: https://link.aps.org/doi/10.1103/PhysRevLett.126.
191802.
76
[33] K. M. Backes et al. “A quantum enhanced search for dark matter axions”. In: Nature
590.7845 (2021), 238–242. ISSN: 1476-4687. DOI: 10.1038/s41586-021-03226-7.
URL: http://dx.doi.org/10.1038/s41586-021-03226-7.
[34] B. M. Brubaker et al. “First results from a microwave cavity axion search at 24 µeV”. In:
Phys. Rev. Lett. 118.6 (2017), p. 061302. DOI: 10.1103/PhysRevLett.118.061302.
arXiv: 1610.02580 [astro-ph.CO].
[35] L. Zhong et al. “Results from phase 1 of the HAYSTAC microwave cavity axion experiment”. In: Phys. Rev. D 97.9 (2018), p. 092001. DOI: 10.1103/PhysRevD.97.092001.
arXiv: 1803.03690 [hep-ex].
[36] “New CAST limit on the axion–photon interaction”. In: Nature Physics 13.6 (2017),
pp. 584–590. DOI: 10.1038/nphys4109. URL: https://arxiv.org/abs/1705.
02290.
[37] Peter W. Graham et al. “Experimental Searches for the Axion and Axion-Like Particles”. In: Annual Review of Nuclear and Particle Science 65.1 (2015), pp. 485–514. DOI:
10.1146/annurev-nucl-102014-022120. URL: https://arxiv.org/abs/
1602.00039.
[38] Hsin Chang et al. “TASEH: A haloscope axion search experiment”. In: (May 2022).
arXiv: 2205 . 01477 [physics.ins-det]. URL: https : / / arxiv . org / abs /
2205.01477.
[39] C. Bartram et al. “Axion dark matter experiment: Run 1B analysis details”. In: Phys.
Rev. D 103 (3 2021), p. 032002. DOI: 10.1103/PhysRevD.103.032002. URL: https:
//link.aps.org/doi/10.1103/PhysRevD.103.032002. |