Direct couplings of mimetic dark matter and their cosmological effects

Liuyuan Shen; Yicen Mou; Yunlong Zheng; Mingzhe Li

doi:10.1088/1674-1137/42/1/015101

Chinese Physics C> 2018, Vol. 42> Issue(1) : 015101 DOI: 10.1088/1674-1137/42/1/015101

Direct couplings of mimetic dark matter and their cosmological effects

1.
Department of Physics, Nanjing University, Nanjing 210093, China
2.
Joint Center for Particle, Nuclear Physics and Cosmology, Nanjing 210093, China
3.
Interdisciplinary Center for Theoretical Study, University of Science and Technology of China, Hefei, Anhui 230026, China

Abstract
HTML
Reference
Related

PDF

Abstract：
The original mimetic model was proposed to take the role of dark matter. In this paper we consider possible direct interactions of mimetic dark matter with other matter in the universe, especially standard model particles such as baryons and photons. By imposing shift symmetry, the mimetic dark matter field can only have derivative couplings. We discuss the possibilities of generating baryon number asymmetry and cosmic birefringence in the universe based on the derivative couplings of mimetic dark matter to baryons and photons.
- cosmology ,
- dark matter ,
- baryogenesis ,
- cosmological CPT violation

References

[1]	A. H. Chamseddine and V. Mukhanov, JHEP, 1311:135 (2013) doi:10.1007/JHEP11(2013)135[arXiv:1308.5410[astro-ph.CO]]
[2]	A. Golovnev, Phys. Lett. B, 728:39 (2014) doi:10.1016/j.physletb.2013.11.026[arXiv:1310.2790[gr-qc]]
[3]	A. O. Barvinsky, JCAP, 1401:014 (2014) doi:10.1088/1475-7516/2014/01/014[arXiv:1311.3111[hep-th]]
[4]	K. Hammer and A. Vikman, arXiv:1512.09118[gr-qc]
[5]	A. H. Chamseddine, V. Mukhanov and A. Vikman, JCAP, 1406:017 (2014) doi:10.1088/1475-7516/2014/06/017[arXiv:1403.3961[astro-ph.CO]]
[6]	E. A. Lim, I. Sawicki, and A. Vikman, JCAP, 1005:012 (2010) doi:10.1088/1475-7516/2010/05/012[arXiv:1003.5751[astro-ph.CO]]
[7]	J. D. Bekenstein, Phys. Rev. D, 48:3641 (1993) doi:10.1103/PhysRevD.48.3641[gr-qc/9211017]
[8]	N. Deruelle and J. Rua, JCAP, 1409:002 (2014) doi:10.1088/1475-7516/2014/09/002[arXiv:1407.0825[gr-qc]]
[9]	F. Arroja, N. Bartolo, P. Karmakar, and S. Matarrese, JCAP, 1509:051 (2015) doi:10.1088/1475-7516/2015/09/051[arXiv:1506.08575[gr-qc]]
[10]	G. Domnech, S. Mukohyama, R. Namba, A. Naruko, R. Saitou, and Y. Watanabe, Phys. Rev. D, 92 (8):084027 (2015) doi:10.1103/PhysRevD.92.084027[arXiv:1507.05390[hep-th]]
[11]	O. Malaeb, Phys. Rev. D, 91 (10):103526 (2015) doi:10.1103/PhysRevD.91.103526[arXiv:1404.4195[gr-qc]]
[12]	M. Chaichian, J. Kluson, M. Oksanen, and A. Tureanu, JHEP, 1412:102 (2014) doi:10.1007/JHEP12(2014)102[arXiv:1404.4008[hep-th]]
[13]	S. Nojiri and S. D. Odintsov, Mod. Phys. Lett. A, 29 (40):1450211 (2014) doi:10.1142/S0217732314502113[arXiv:1408.3561[hep-th]]
[14]	G. Leon and E. N. Saridakis, JCAP, 1504 (04):031 (2015) doi:10.1088/1475-7516/2015/04/031[arXiv:1501.00488[gr-qc]]
[15]	A. V. Astashenok, S. D. Odintsov, and V. K. Oikonomou, Class. Quant. Grav., 32 (18):185007 (2015) doi:10.1088/0264-9381/32/18/185007[arXiv:1504.04861[gr-qc]]
[16]	R. Myrzakulov, L. Sebastiani, and S. Vagnozzi, Eur. Phys. J. C, 75:444 (2015) doi:10.1140/epjc/s10052-015-3672-6[arXiv:1504.07984[gr-qc]]
[17]	S. D. Odintsov and V. K. Oikonomou, Annals Phys., 363:503 (2015) doi:10.1016/j.aop.2015.10.013[arXiv:1508.07488[gr-qc]]
[18]	Y. Rabochaya and S. Zerbini, Eur. Phys. J. C, 76 (2):85 (2016) doi:10.1140/epjc/s10052-016-3926-y[arXiv:1509.03720[gr-qc]]
[19]	S. D. Odintsov and V. K. Oikonomou, Phys. Rev. D, 93 (2):023517 (2016) doi:10.1103/PhysRevD.93.023517[arXiv:1511.04559[gr-qc]]
[20]	F. Arroja, N. Bartolo, P. Karmakar and S. Matarrese, JCAP, 1604 (04):042 (2016) doi:10.1088/1475-7516/2016/04/042[arXiv:1512.09374[gr-qc]]
[21]	G. Cognola, R. Myrzakulov, L. Sebastiani, S. Vagnozzi, and S. Zerbini, Class. Quant. Grav., 33 (22):225014 (2016) doi:10.1088/0264-9381/33/22/225014[arXiv:1601.00102[gr-qc]]
[22]	S. Nojiri, S. D. Odintsov, and V. K. Oikonomou, Class. Quant. Grav., 33 (12):125017 (2016) doi:10.1088/0264-9381/33/12/125017[arXiv:1601.07057[gr-qc]]
[23]	S. D. Odintsov and V. K. Oikonomou, Phys. Rev. D, 94 (4):044012 (2016) doi:10.1103/PhysRevD.94.044012[arXiv:1608.00165[gr-qc]]
[24]	H. Saadi, Eur. Phys. J. C, 76 (1):14 (2016) doi:10.1140/epjc/s10052-015-3856-0[arXiv:1411.4531[gr-qc]]
[25]	L. Mirzagholi and A. Vikman, JCAP, 1506:028 (2015) doi:10.1088/1475-7516/2015/06/028[arXiv:1412.7136[gr-qc]]
[26]	J. Matsumoto, S. D. Odintsov, and S. V. Sushkov, Phys. Rev. D, 91 (6):064062 (2015) doi:10.1103/PhysRevD.91.064062[arXiv:1501.02149[gr-qc]]
[27]	D. Momeni, K. Myrzakulov, R. Myrzakulov, and M. Raza, Eur. Phys. J. C, 76 (6):301 (2016) doi:10.1140/epjc/s10052-016-4147-0[arXiv:1505.08034[gr-qc]]
[28]	S. Ramazanov, JCAP, 1512:007 (2015) doi:10.1088/1475-7516/2015/12/007[arXiv:1507.00291[gr-qc]]
[29]	R. Myrzakulov, L. Sebastiani, S. Vagnozzi, and S. Zerbini, Class. Quant. Grav., 33 (12):125005 (2016) doi:10.1088/0264-9381/33/12/125005[arXiv:1510.02284[gr-qc]]
[30]	A. V. Astashenok and S. D. Odintsov, Phys. Rev. D, 94 (6):063008 (2016) doi:10.1103/PhysRevD.94.063008[arXiv:1512.07279[gr-qc]]
[31]	A. H. Chamseddine and V. Mukhanov, JCAP, 1602 (02):040 (2016) doi:10.1088/1475-7516/2016/02/040[arXiv:1601.04941[astro-ph.CO]]
[32]	S. Nojiri, S. D. Odintsov, and V. K. Oikonomou, Phys. Rev. D, 94 (10):104050 (2016) doi:10.1103/PhysRevD.94.104050[arXiv:1608.07806[gr-qc]]
[33]	E. Babichev and S. Ramazanov, Phys. Rev. D, 95 (2):024025 (2017) doi:10.1103/PhysRevD.95.024025[arXiv:1609.08580[gr-qc]]
[34]	A. H. Chamseddine and V. Mukhanov, Eur. Phys. J. C, 77 (3):183 (2017) doi:10.1140/epjc/s10052-017-4759-z[arXiv:1612.05861[gr-qc]]
[35]	N. Sadeghnezhad and K. Nozari, arXiv:1703.06269[gr-qc]
[36]	A. Ijjas, J. Ripley, and P. J. Steinhardt, Phys. Lett. B, 760:132 (2016) doi:10.1016/j.physletb.2016.06.052[arXiv:1604.08586[gr-qc]]
[37]	H. Firouzjahi, M. A. Gorji, and A. Hosseini Mansoori, arXiv:1703.02923[hep-th]
[38]	S. Hirano, S. Nishi, and T. Kobayashi, JCAP, 1707 (07):009 (2017) doi:10.1088/1475-7516/2017/07/009[arXiv:1704.06031[gr-qc]]
[39]	Y. Zheng, L. Shen, Y. Mou, and M. Li, JCAP, 1708 (08):040 (2017) doi:10.1088/1475-7516/2017/08/040[arXiv:1704.06834[gr-qc]]
[40]	Y. Cai and Y. S. Piao, arXiv:1705.03401[gr-qc]
[41]	Y. Cai and Y. S. Piao, arXiv:1707.01017[gr-qc]
[42]	K. Takahashi and T. Kobayashi, arXiv:1708.02951[gr-qc]
[43]	L. Sebastiani, S. Vagnozzi, and R. Myrzakulov, Adv. High Energy Phys., 2017:3156915 (2017) doi:10.1155/2017/3156915[arXiv:1612.08661[gr-qc]]
[44]	S. Vagnozzi, Class. Quant. Grav., 34:18 (2017) doi:10.1088/1361-6382/aa838b[arXiv:1708.00603[gr-qc]]
[45]	M. A. Gorji, S. A. Hosseini Mansoori, and H. Firouzjahi, arXiv:1709.09988[astro-ph.CO]
[46]	S. Weinberg, Gravitation and Cosmology:Principles and Applications of the General Theory of Relativity (New York:Wiley, 1972)
[47]	A. G. Cohen and D. B. Kaplan, Phys. Lett. B, 199:251 (1987) doi:10.1016/0370-2693(87)91369-4
[48]	M. Li, X. Wang, B. Feng, and X. Zhang, Phys. Rev. D, 65:103511 (2002) doi:10.1103/PhysRevD.65.103511[hep-ph/0112069]
[49]	M. Li and X. Zhang, Phys. Lett. B, 573:20 (2003) doi:10.1016/j.physletb.2003.08.041[hep-ph/0209093]
[50]	E. W. Kolb and M. S. Turner, The Early Universe, Front. Phys., 69:1 (1990)
[51]	A. D. Sakharov, Pisma Zh. Eksp. Teor. Fiz., 5:32 (1967)[JETP Lett., 5:24 (1967) [Sov. Phys. Usp., 34:392 (1991) [Usp. Fiz. Nauk, 161:61 (1991) doi:10.1070/PU1991v034n05ABEH002497
[52]	H. Davoudiasl, R. Kitano, G. D. Kribs, H. Murayama, and P. J. Steinhardt, Phys. Rev. Lett., 93:201301 (2004) doi:10.1103/PhysRevLett.93.201301[hep-ph/0403019]
[53]	H. Li, M. Li, and X. Zhang, Phys. Rev. D, 70:047302 (2004) doi:10.1103/PhysRevD.70.047302[hep-ph/0403281]
[54]	P. A. R. Ade et al (Planck Collaboration), Astron. Astrophys., 594:A13 (2016) doi:10.1051/0004-6361/201525830[arXiv:1502.01589[astro-ph.CO]]
[55]	S. M. Carroll, G. B. Field, and R. Jackiw, Phys. Rev. D, 41:1231 (1990) doi:10.1103/PhysRevD.41.1231
[56]	S. M. Carroll, Phys. Rev. Lett., 81:3067 (1998) doi:10.1103/PhysRevLett.81.3067[astro-ph/9806099]
[57]	M. Li and X. Zhang, Phys. Rev. D, 78:103516 (2008) doi:10.1103/PhysRevD.78.103516[arXiv:0810.0403[astro-ph]]
[58]	M. Kamionkowski, Phys. Rev. Lett., 102:111302 (2009) doi:10.1103/PhysRevLett.102.111302[arXiv:0810.1286[astro-ph]]
[59]	M. Li and B. Yu, JCAP, 1306:016 (2013) doi:10.1088/1475-7516/2013/06/016[arXiv:1303.1881[astro-ph.CO]]
[60]	A. Lue, L. M. Wang, and M. Kamionkowski, Phys. Rev. Lett., 83:1506 (1999) doi:10.1103/PhysRevLett.83.1506[astro-ph/9812088]
[61]	B. Feng, H. Li, M. z. Li, and X. m. Zhang, Phys. Lett. B, 620:27 (2005) doi:10.1016/j.physletb.2005.06.009[hep-ph/0406269]
[62]	B. Feng, M. Li, J. Q. Xia, X. Chen, and X. Zhang, Phys. Rev. Lett., 96:221302 (2006) doi:10.1103/PhysRevLett.96.221302[astro-ph/0601095]
[63]	N. Aghanim et al (Planck Collaboration), Astron. Astrophys., 596:A110 (2016) doi:10.1051/0004-6361/201629018[arXiv:1605.08633[astro-ph.CO]]
[64]	Y. P. Li, Y. Liu, S. Y. Li, H. Li, and X. Zhang, arXiv:1709.09053[astro-ph.IM]
[65]	H. Li et al, arXiv:1710.03047[astro-ph.CO]

[1]	Ufuk Aydemir , Jing Ren . Dark sector production and baryogenesis from not quite black holes. Chinese Physics C, 2021, 45(7): 075103. doi: 10.1088/1674-1137/abf9ff
[2]	Constanza Callender , Alfonso R. Zerwekh . A dark vector resonance at CLIC. Chinese Physics C, 2019, 43(6): 063102. doi: 10.1088/1674-1137/43/6/063102
[3]	Ran Ding , Zhi-Long Han , Li Huang , Yi Liao . Phenomenology of colored radiative neutrino mass model and its implications on cosmic-ray observations. Chinese Physics C, 2018, 42(10): 103101. doi: 10.1088/1674-1137/42/10/103101
[4]	Li-Tao Yang , et al . Limits on light WIMPs with a 1 kg-scale germanium detector at 160 eVee physics threshold at the China Jinping Underground Laboratory. Chinese Physics C, 2018, 42(2): 023002. doi: 10.1088/1674-1137/42/2/023002
[5]	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
[6]	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
[7]	Andrea Addazi , Antonino Marcianò . Gravitational waves from dark first order phase transitions and dark photons. Chinese Physics C, 2018, 42(2): 023107. doi: 10.1088/1674-1137/42/2/023107
[8]	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
[9]	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
[10]	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
[11]	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
[12]	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
[13]	Qing-Hao Chen , Qian Yue , Jian-Ping Cheng , Ke-Jun Kang , Yuan-Jing Li , Shin-Ted Lin , Chang-Jian Tang , Hao-Yang Xing , Xun-Zhen Yu , Ming Zeng , Jing-Jun Zhu . Measurement of photoelectron yield of the CDEX-10 liquid argon detector prototype. Chinese Physics C, 2016, 40(11): 116002. doi: 10.1088/1674-1137/40/11/116002
[14]	Zhi-Ying Li , Zhi-Yong Zhang , Yi-Feng Wei , Chi Wang , Yun-Long Zhang , Si-Cheng Wen , Xiao-Lian Wang , Zi-Zong Xu , Guang-Shun Huang . Energy correction for the BGO calorimeter of DAMPE using an electron beam. Chinese Physics C, 2016, 40(8): 086202. doi: 10.1088/1674-1137/40/8/086202
[15]	Pei-Xian Li , Meng-Yun Guan , Chang-Gen Yang , Peng Zhang , Jin-Chang Liu , Yong-Peng Zhang , Cong Guo , Yi Wang . Preliminary test results of LAr prototype detector. Chinese Physics C, 2016, 40(11): 116005. doi: 10.1088/1674-1137/40/11/116005
[16]	Halife Caglar , Sezgin Aygün . String cloud and domain walls with quark matter for a higher dimensional FRW universe in self creation cosmology. Chinese Physics C, 2016, 40(4): 045103. doi: 10.1088/1674-1137/40/4/045103
[17]	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
[18]	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
[19]	CHEN Bin . On Hořava-Lifshitz cosmology. Chinese Physics C, 2011, 35(5): 429-435. doi: 10.1088/1674-1137/35/5/004
[20]	HE Xiao-Gang . Darkon dark matter, unparticle effects and collider physics. Chinese Physics C, 2009, 33(6): 451-455. doi: 10.1088/1674-1137/33/6/010

Access

Get Citation

Liuyuan Shen, Yicen Mou, Yunlong Zheng and Mingzhe Li. Direct couplings of mimetic dark matter and their cosmological effects[J]. Chinese Physics C, 2018, 42(1): 015101. doi: 10.1088/1674-1137/42/1/015101

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 2017-10-12

Fund

Supported by NSFC (11422543, 11653002)

Article Metric

Article Views(1597)
PDF Downloads(29)
Cited by(0)

Policy on re-use

To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.

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

Direct couplings of mimetic dark matter and their cosmological effects

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

Direct couplings of mimetic dark matter and their cosmological effects

HTML

目录