Gravitational waves from dark first order phase transitions and dark photons

Andrea Addazi; Antonino Marcian&ograve;

doi:10.1088/1674-1137/42/2/023107

Chinese Physics C> 2018, Vol. 42> Issue(2) : 023107 DOI: 10.1088/1674-1137/42/2/023107

Gravitational waves from dark first order phase transitions and dark photons

Andrea Addazi ^, ,
Antonino Marcianò

Abstract
HTML
Reference
Related

PDF

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.
- dark matter ,
- gravitational waves ,
- colliders

References

[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]]

[1]	Jie Wang , Jinghong Ma , Jing Gao , Xiao-Fang Han , Lei Wang . U(1)_{L_μ-L_τ} breaking phase transition, muon g–2, dark matter, collider, and gravitational wave. Chinese Physics C, 2024, 48(2): 023101. doi: 10.1088/1674-1137/ad0f89
[2]	Yu Zhang , Yi-Wei Huang , Wei-Tao Zhang , Mao Song , Ran Ding . Exploring dark matter-gauge boson effective interactions at current and future colliders. Chinese Physics C, 2024, 48(6): 063106. doi: 10.1088/1674-1137/ad2362
[3]	Ze-Yu Qiu , Zhao-Huan Yu . Gravitational waves from cosmic strings associated with pseudo-Nambu-Goldstone dark matter. Chinese Physics C, 2023, 47(8): 085104. doi: 10.1088/1674-1137/acd9bf
[4]	Kai Ma . Mono-γ production of a dark vector at future e⁺e⁻ colliders. Chinese Physics C, 2022, 46(11): 113104. doi: 10.1088/1674-1137/ac827b
[5]	Qing-Hong Cao , An-Kang Wei , Qian-Fei Xiang . Dark matter search at colliders and neutrino floor. Chinese Physics C, 2020, 44(11): 113105. doi: 10.1088/1674-1137/abae53
[6]	Hai-Nan Lin , Xin Li . A new method to test the cosmic distance duality relation using the strongly lensed gravitational waves. Chinese Physics C, 2020, 44(7): 075101. doi: 10.1088/1674-1137/44/7/075101
[7]	Wen Yin . Fixed point and anomaly mediation in partial N=2 supersymmetric standard models. Chinese Physics C, 2018, 42(1): 013104. doi: 10.1088/1674-1137/42/1/013104
[8]	Kun Wang , Fei Wang , Jingya Zhu , Quanlin Jie . The semi-constrained NMSSM in light of muon g-2, LHC, anddark matter constraints. Chinese Physics C, 2018, 42(10): 103109. doi: 10.1088/1674-1137/42/10/103109
[9]	Guoli Liu , Fei Wang , Wenyu Wang , Jin-Min Yang . Explaining DAMPE results by dark matter with hierarchical lepton-specific Yukawa interactions. Chinese Physics C, 2018, 42(3): 035101. doi: 10.1088/1674-1137/42/3/035101
[10]	Andrea Addazi , Stephon Alexander , Yi-Fu Cai , Antonino Marcianó . Dark matter and baryogenesis in the Fermi-bounce curvaton mechanism. Chinese Physics C, 2018, 42(6): 065101. doi: 10.1088/1674-1137/42/6/065101
[11]	Peyman Zakeri , Mohammad Moosavi , Mohammadreza Zakeri , Yaser Ayazi . A minimal model for two-component FIMP dark matter: A basic search. Chinese Physics C, 2018, 42(7): 073101. doi: 10.1088/1674-1137/42/7/073101
[12]	Andrea Addazi , Pietro Donà , Antonino Marcianò . Dynamical interactions of dark energy and dark matter: Yang-Mills condensate and QCD axions. Chinese Physics C, 2018, 42(7): 075102. doi: 10.1088/1674-1137/42/7/075102
[13]	Liuyuan Shen , Yicen Mou , Yunlong Zheng , Mingzhe Li . Direct couplings of mimetic dark matter and their cosmological effects. Chinese Physics C, 2018, 42(1): 015101. doi: 10.1088/1674-1137/42/1/015101
[14]	Andrea Addazi , Antonino Marcianò . Limiting majoron self-interactions from gravitational wave experiments. Chinese Physics C, 2018, 42(2): 023105. doi: 10.1088/1674-1137/42/2/023105
[15]	Hao Wen , Fang-Yu Li , Jin Li , Zhen-Yun Fang , Andrew Beckwith . Very high-frequency gravitational waves from magnetars and gamma-ray bursts. Chinese Physics C, 2017, 41(12): 125101. doi: 10.1088/1674-1137/41/12/125101
[16]	Shivaramakrishna Singirala . Implications of fermionic dark matter on recent neutrino oscillation data. Chinese Physics C, 2017, 41(4): 043102. doi: 10.1088/1674-1137/41/4/043102
[17]	null . Signal photon flux generated by high-frequency relic gravitational waves. Chinese Physics C, 2016, 40(8): 085101. doi: 10.1088/1674-1137/40/8/085101
[18]	Yi-Ming Hu , Jin Chang , Deng-Yi Chen , Jian-Hua Guo , Yun-Long Zhang , Chang-Qing Feng . Environmental test of the BGO calorimeterfor DArk Matter Particle Explorer. Chinese Physics C, 2016, 40(11): 116003. doi: 10.1088/1674-1137/40/11/116003
[19]	S. A. Alavi , F. S. Kazemian . Photonic dark matter portal and quantum physics. Chinese Physics C, 2016, 40(2): 025101. doi: 10.1088/1674-1137/40/2/025101
[20]	HUANG Chao-Guang , ZHANG Hai-Qing , GUO Han-Ying . A new gravitational model for dark energy. Chinese Physics C, 2008, 32(9): 687-691. doi: 10.1088/1674-1137/32/9/002

Access

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

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 2017-10-09
Revised: 2017-12-18

Fund

Supported by the Shanghai Municipality (KBH1512299) and Fudan University (JJH1512105)}

Article Metric

Article Views(1603)
PDF Downloads(20)
Cited by(0)

Policy on re-use

To reuse of Open Access content published by CPC, for content published under the terms of the Creative Commons Attribution 3.0 license (“CC CY”), the users don’t need to request permission to copy, distribute and display the final published version of the article and to create derivative works, subject to appropriate attribution.

通讯作者: 陈斌, bchen63@163.com

1.
沈阳化工大学材料科学与工程学院沈阳 110142

Gravitational waves from dark first order phase transitions and dark photons

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

Gravitational waves from dark first order phase transitions and dark photons

Corresponding author: Andrea Addazi,

HTML

目录