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《中国物理C》(英文)编辑部
2024年10月30日

Gravitational waves from dark first order phase transitions and dark photons

  • Cold Dark Matter particles may interact with ordinary particles through a dark photon, which acquires a mass thanks to a spontaneous symmetry breaking mechanism. We discuss a dark photon model in which the scalar singlet associated to the spontaneous symmetry breaking has an effective potential that induces a first order phase transition in the early Universe. Such a scenario provides a rich phenomenology for electron-positron colliders and gravitational waves interferometers, and may be tested in several different channels. The hidden first order phase transition implies the emission of gravitational waves signals, which may constrain the dark photon's space of parameters. Compared limits from electron-positron colliders, astrophysics, cosmology and future gravitational waves interferometers such as eLISA, U-DECIGO and BBO are discussed. This highly motivates a cross-checking strategy of data arising from experiments dedicated to gravitational waves, meson factories, the International Linear Collider (ILC), the Circular Electron Positron Collider (CEPC) and other underground direct detection experiments of cold dark matter candidates.
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  • [1] C. Caprini et al, JCAP, 1604(4):001 (2016) doi:10.1088/1475-7516/2016/04/001[arXiv:1512.06239[astro-ph.CO]]
    [2] H. Kudoh, A. Taruya, T. Hiramatsu, and Y. Himemoto, Phys. Rev. D, 73:064006 (2006) doi:10.1103/PhysRevD.73.064006[gr-qc/0511145]
    [3] H. Audley et al, arXiv:1702.00786[astro-ph.IM]
    [4] E. Witten, Phys. Rev. D, 30:272 (1984) doi:10.1103/PhysRevD.30.272
    [5] M. S. Turner and F. Wilczek, Phys. Rev. Lett., 65; 3080 (1990) doi:10.1103/PhysRevLett.65.3080
    [6] C. J. Hogan, Mon. Not. Roy. Astron. Soc., 218:629 (1986)
    [7] A. Kosowsky, M. S. Turner, and R. Watkins, Phys. Rev. D, 45:4514 (1992) doi:10.1103/PhysRevD.45.4514
    [8] M. Kamionkowski, A. Kosowsky, and M. S. Turner, Phys. Rev. D, 49:2837 (1994) doi:10.1103/PhysRevD.49.2837[astroph/9310044]
    [9] M. Hindmarsh, S. J. Huber, K. Rummukainen, and D. J. Weir, Phys. Rev. Lett., 112:041301 (2014) doi:10.1103/PhysRevLett.112.041301[arXiv:1304.2433[hepph]]
    [10] M. Hindmarsh, S. J. Huber, K. Rummukainen, and D. J. Weir, Phys. Rev. D, 92(12):123009 (2015) doi:10.1103/PhysRevD.92.123009[arXiv:1504.03291[astroph.CO]]
    [11] P. Schwaller, Phys. Rev. Lett., 115(18):181101 (2015) doi:10.1103/PhysRevLett.115.181101[arXiv:1504.07263[hepph]]
    [12] M. Chala, G. Nardini, and I. Sobolev, Phys. Rev. D, 94(5):055006 (2016) doi:10.1103/PhysRevD.94.055006[arXiv:1605.08663[hep-ph]]
    [13] S. J. Huber, T. Konstandin, G. Nardini, and I. Rues, JCAP, 1603(3):036 (2016) doi:10.1088/1475-7516/2016/03/036[arXiv:1512.06357[hep-ph]]
    [14] F. P. Huang, Y. Wan, D. G. Wang, Y. F. Cai, and X. Zhang, Phys. Rev. D, 94(4):041702 (2016) doi:10.1103/PhysRevD.94.041702[arXiv:1601.01640[hep-ph]]
    [15] M. Artymowski, M. Lewicki, and J. D. Wells, arXiv:1609.07143[hep-ph]
    [16] P. S. B. Dev and A. Mazumdar, Phys. Rev. D, 93(10):104001 (2016) doi:10.1103/PhysRevD.93.104001[arXiv:1602.04203[hep-ph]]
    [17] A. Katz and A. Riotto, arXiv:1608.00583[hep-ph]
    [18] F. P. Huang and X. Zhang, arXiv:1701.04338[hep-ph]
    [19] I. Baldes, arXiv:1702.02117[hep-ph]
    [20] W. Chao, H. K. Guo, and J. Shu, arXiv:1702.02698[hep-ph]
    [21] A. Addazi, arXiv:1607.08057[hep-ph], to appear in Mod. Phys. Lett.A.
    [22] C. Delaunay, C. Grojean, and J. D. Wells, JHEP, 0804:029 (2008) doi:10.1088/1126-6708/2008/04/029[arXiv:0711.2511[hep-ph]]
    [23] B. Holdom, Phys. Lett., 166B:196 (1986) doi:10.1016/0370-2693(86)91377-8
    [24] S. L. Glashow, Phys. Lett. B, 167:36 (1986)
    [25] E. D. Carlson and S. L. Glashow, Phys. Lett. B, 193:168 (1987)
    [26] J. D. Bjorken, R. Essig, P. Schuster, and N. Toro, Phys. Rev. D, 80:075018 (2009)[arXiv:0906.0580[hep-ph]]
    [27] J. D. Bjorken et al, Phys. Rev. D, 38:3375 (1988)
    [28] E. M. Riordan et al, Phys. Rev. Lett., 59:755 (1987)
    [29] A. Bross, M. Crisler, S. H. Pordes, J. Volk, S. Errede, and J. Wrbanek, Phys. Rev. Lett., 67:2942 (1991)
    [30] M. Pospelov, Phys. Rev. D, 80:095002 (2009)[arXiv:0811.1030[hep-ph]]
    [31] H. Davoudiasl, H. -S. Lee, and W. J. Marciano, Phys. Rev. D, 86:095009 (2012)[arXiv:1208.2973[hep-ph]]
    [32] M. Endo, K. Hamaguchi, and G. Mishima, Phys. Rev. D, 86:095029 (2012)[arXiv:1209.2558[hep-ph]]
    [33] D. Babusci et al (KLOE-2 Collaboration), Phys. Lett. B, 720:111 (2013)[arXiv:1210.3927[hep-ex]]
    [34] F. Archilli, D. Babusci, D. Badoni, I. Balwierz, G. Bencivenni, C. Bini, C. Bloise, and V. Bocci et al, Phys. Lett. B, 706:251 (2012)[arXiv:1110.0411[hep-ex]]
    [35] P. Adlarson et al (WASA-at-COSY Collaboration), Phys. Lett. B, 726:187 (2013)[arXiv:1304.0671[hep-ex]]
    [36] Abrahamyan et al (APEX Collaboration), Phys. Rev. Lett., 107:191804 (2011)[arXiv:1108.2750[hep-ex]]
    [37] H. Merkel et al (A1 Collaboration), Phys. Rev. Lett., 106:251802 (2011)[arXiv:1101.4091[nucl-ex]]
    [38] M. Reece and L. T. Wang, JHEP, 0907:051 (2009)[arXiv:0904.1743[hep-ph]]
    [39] B. Aubert et al (BABAR Collaboration), Phys. Rev. Lett., 103:081803 (2009)[arXiv:0905.4539[hep-ex]]
    [40] J. B. Dent, F. Ferrer, and L. M. Krauss, arXiv:1201.2683[astroph.CO]
    [41] H. K. Dreiner, J.-F. Fortin, C. Hanhart, and L. Ubaldi, arXiv:1310.3826[hep-ph]
    [42] R. Essig, P. Schuster, N. Toro, and B. Wojtsekhowski, JHEP, 1102:009 (2011)[arXiv:1001.2557[hep-ph]]
    [43] The Heavy Photon Search Collaboration (HPS), https://confluence.slac.stanford.edu/display/hpsg/
    [44] M. Freytsis, G. Ovanesyan, and J. Thaler, JHEP, 1001 111 (2010)[arXiv:0909.2862[hep-ph]]
    [45] B. Wojtsekhowski, AIP Conf. Proc., 1160:149 (2009)[arXiv:0906.5265[hep-ex]]
    [46] B. Wojtsekhowski, D. Nikolenko, and I. Rachek, arXiv:1207.5089[hep-ex]
    [47] T. Beranek, H. Merkel, and M. Vanderhaeghen, Phys. Rev. D, 88:015032 arXiv:1303.2540[hep-ph]
    [48] R. Bernabei et al, Eur. Phys. J. C, 73:2648 (2013) doi:10.1140/epjc/s10052-013-2648-7[arXiv:1308.5109[astroph.GA]]
    [49] R. Bernabei et al, Phys. Rev. D, 77:023506 (2008) doi:10.1103/PhysRevD.77.023506[arXiv:0712.0562[astro-ph]]
    [50] R. Foot, arXiv:1508.07402[hep-ph]
    [51] S. K. Lee, M. Lisanti, S. Mishra-Sharma, and B. R. Safdi, Phys. Rev. D, 92(8):083517 (2015) doi:10.1103/PhysRevD.92.083517[arXiv:1508.07361[hep-ph]]
    [52] J. W. Chen, H. C. Chi, C. P. Liu, C. L. Wu, and C. P. Wu, Phys. Rev. D, 92(9):096013 (2015) doi:10.1103/PhysRevD.92.096013[arXiv:1508.03508[hep-ph]]
    [53] A. Addazi, Z. Berezhiani, R. Bernabei, P. Belli, F. Cappella, R. Cerulli, and A. Incicchitti, Eur. Phys. J. C, 75(8):400 (2015) doi:10.1140/epjc/s10052-015-3634-z[arXiv:1507.04317[hep-ex]]
    [54] R. Cerulli, P. Villar, F. Cappella, R. Bernabei, P. Belli, A. Incicchitti, A. Addazi, and Z. Berezhiani, Eur. Phys. J. C, 77(2):83 (2017) doi:10.1140/epjc/s10052-017-4658-3[arXiv:1701.08590[hep-ex]]
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Get Citation
Andrea Addazi and Antonino Marcianò. Gravitational waves from dark first order phase transitions and dark photons[J]. Chinese Physics C, 2018, 42(2): 023107. doi: 10.1088/1674-1137/42/2/023107
Andrea Addazi and Antonino Marcianò. Gravitational waves from dark first order phase transitions and dark photons[J]. Chinese Physics C, 2018, 42(2): 023107.  doi: 10.1088/1674-1137/42/2/023107 shu
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Received: 2017-10-09
Revised: 2017-12-18
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    Supported by the Shanghai Municipality (KBH1512299) and Fudan University (JJH1512105)}

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Gravitational waves from dark first order phase transitions and dark photons

    Corresponding author: Andrea Addazi,
Fund Project:  Supported by the Shanghai Municipality (KBH1512299) and Fudan University (JJH1512105)}

Abstract: Cold Dark Matter particles may interact with ordinary particles through a dark photon, which acquires a mass thanks to a spontaneous symmetry breaking mechanism. We discuss a dark photon model in which the scalar singlet associated to the spontaneous symmetry breaking has an effective potential that induces a first order phase transition in the early Universe. Such a scenario provides a rich phenomenology for electron-positron colliders and gravitational waves interferometers, and may be tested in several different channels. The hidden first order phase transition implies the emission of gravitational waves signals, which may constrain the dark photon's space of parameters. Compared limits from electron-positron colliders, astrophysics, cosmology and future gravitational waves interferometers such as eLISA, U-DECIGO and BBO are discussed. This highly motivates a cross-checking strategy of data arising from experiments dedicated to gravitational waves, meson factories, the International Linear Collider (ILC), the Circular Electron Positron Collider (CEPC) and other underground direct detection experiments of cold dark matter candidates.

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