Dynamical interactions of dark energy and dark matter: Yang-Mills condensate and QCD axions

Andrea Addazi; Pietro Don&agrave;; Antonino Marcian&ograve;

doi:10.1088/1674-1137/42/7/075102

Chinese Physics C> 2018, Vol. 42> Issue(7) : 075102 DOI: 10.1088/1674-1137/42/7/075102

Dynamical interactions of dark energy and dark matter: Yang-Mills condensate and QCD axions

1.
Department of Physics &

Abstract
HTML
Reference
Related

PDF

Abstract：
We analyze a model of cold axion dark matter weakly coupled with a dark gluon condensate, reproducing dark energy. We first review how to recover the dark energy behavior using the functional renormalization group approach, and ground our study in the properties of the effective Lagrangian, to be determined non-perturbatively. Then, within the context of G_SM×SU(2)_D×U(1)_PQ, we consider Yang-Mills condensate (YMC) interactions with QCD axions. We predict a transfer of dark energy density into dark matter density, that can be tested in the next generation of experiments dedicated to dark energy measurements. We obtain new bounds on the interactions between the Yang-Mills condensate and axion dark matter from Planck data:the new physics interaction scale related to the axion/gluon condensate mixing is constrained to be higher than the 10⁶ GeV energy scale.
- dark matter ,
- dark energy ,
- axion ,
- peccei-quinn

References

[1]	P. Don, A. Marcian, Y. Zhang, and C. Antolini, Phys. Rev. D, 93(4): 043012 (2016) [arXiv:1509.05824 [gr-qc]]
[2]	A. G. Riess et al, Astron. J., 116: 1009 (1998) [astroph/9805201]
[3]	S. Perlmutter et al, Astrophys. J., 517: 565 (1999) [astroph/9812133]
[4]	M. Kowalski et al, Astrophys. J., 686: 749 (2008) [arXiv:0804.4142 [astro-ph]]
[5]	D. N. Spergel et al (WMAP Collaboration), Astrophys. J. Suppl., 148: 175 (2003) [astro-ph/0302209]
[6]	A. W. Graham, D. Merritt, B. Moore, J. Diemand, and B. Terzic, Astron. J., 132: 2685 (2006) [astro-ph/0509417]
[7]	D. N. Spergel et al (WMAP Collaboration), Astrophys. J. Suppl., 170: 377 (2007) [astro-ph/0603449]
[8]	E. Komatsu et al (WMAP Collaboration), Astrophys. J. Suppl., 180: 330 (2009) [arXiv:0803.0547 [astro-ph]]
[9]	S. Cole et al (2dFGRS Collaboration), Mon. Not. Roy. Astron. Soc., 362: 505 (2005) [astro-ph/0501174]
[10]	M. Tegmark et al (SDSS Collaboration), Phys. Rev. D, 74:123507 (2006) [astro-ph/0608632]
[11]	S. Capozziello, S. Carloni, and A. Troisi, Recent Res. Dev. Astron. Astrophys., 1: 625 (2003) [astro-ph/0303041]
[12]	S. M. Carroll, V. Duvvuri, M. Trodden, and M. S. Turner, Phys. Rev. D, 70: 043528 (2004) [astro-ph/0306438]
[13]	L. Amendola and S. Tsujikawa, Dark Energy: Theory and Observations (Cambridge University Press, Cambridge, UK, 2010)
[14]	Y. Zhang, Phys. Lett. B, 340: 18-22 (1994)
[15]	T. Y. Xia and Y. Zhang, Phys. Lett. B, 656: 19-24 (2007)
[16]	S. Wang, Y. Zhang, and T. Y. Xia, The three-loop Yang Mills condensate dark energy model and its cosmological constraints, JCAP, 10: 037 (2008)
[17]	H. Pagels and E. Tomboulis, Nucl. Phys. B, 143: 485 (1978)
[18]	S. Adler, Phys. Rev. D, 23: 2905 (1981); S. Adler, Nucl. Phys. B, 217: 3881 (1983); S. Adler and T. Piran, Rev. Mod. Phys., 56: 1 (1984); S. Adler and T. Piran, Phys. Lett. B, 113: 405 (1982)
[19]	S. G. Matinyan and G. K. Savvidy, Nucl. Phys. B, 134: 539 (1978)
[20]	C. N. Yang, Phys Rev. Lett., 33: 445 (1974)
[21]	W. Zhao and Y. Zhang, Phys. Lett. B, 640: 69 (2006)
[22]	S. W. Hawking and G. F. R. Ellis, The Large Scale Structure of Spacetime (Cambridge Univ. Press, 1973)
[23]	L. Parker and Y. Zhang, Phys. Rev. D, 44: 2421 (1991)
[24]	G. K. Savvidy, Phys. Lett. B, 71: 133 (1977)
[25]	S. Weinberg, In Hawking, S .W. Israel, W. General Relativity, (Cambridge: Cambridge University Press, 1980) p.790-831
[26]	C. Wetterich, Phys. Lett. B, 301: 90 (1993)
[27]	T. R. Morris, Int. J. Mod. Phys. A, 9: 2411 (1994) [hepph/9308265]
[28]	T. Papenbrock and C. Wetterich, Z. Phys. C, 65: 519 (1995) [hep-th/9403164]
[29]	C. S. Fischer and R. Alkofer, Phys. Lett. B, 536: 177 (2002) [hep-ph/0202202]
[30]	C. S. Fischer and J. M. Pawlowski, Phys. Rev. D, 75: 025012 (2007) [arXiv:hep-th/0609009]; Phys. Rev. D, 80: 025023 (2009) [arXiv:0903.2193 [hep-th]]
[31]	C. S. Fischer, A. Maas, and J. M. Pawlowski, Annals Phys., 324: 2408 (2009) [arXiv:0810.1987 [hep-ph]]
[32]	U. Ellwanger, M. Hirsch, and A. Weber, Z. Phys. C, 69: 687 (1996); U. Ellwanger, M. Hirsch, and A. Weber, Eur. Phys. J. C, 1: 563 (1998); B. Bergerhoff and C. Wetterich, Phys. Rev. D, 57: 1591 (1998); [hep-ph/9708425] J. Kato, hep-th/0401068
[33]	J. M. Pawlowski, D. F. Litim, S. Nedelko, and L. von Smekal, Phys. Rev. Lett., 93: 152002 (2004) [hep-th/0312324]; J. M. Pawlowski, D. F. Litim, S. Nedelko, and L. von Smekal, AIP Conf. Proc., 756: 278 (2005) [arXiv:hep-th/0412326]
[34]	M. Reuter and C. Wetterich, hep-th/9411227
[35]	M. Reuter and C. Wetterich, Phys. Rev. D, 56: 7893 (1997) [hep-th/9708051]
[36]	H. Gies, Phys. Rev. D, 66: 025006 (2002) [hep-th/0202207]
[37]	A. Eichhorn, H. Gies, and J. M. Pawlowski, Phys. Rev. D, 83: 045014 (2011); Phys. Rev. D, 83: 069903 (2011) [arXiv:1010.2153 [hep-ph]]
[38]	A. Codello, R. Percacci, L. Rachwa, and A. Tonero, Eur. Phys. J. C, 76(4): 226 (2016) doi:10.1140/epjc/s10052-016-4063-3 [arXiv:1505.03119 [hep-th]]
[39]	Y. A. Simonov, JETP Lett., 55: 627 (1992)
[40]	A. Peshier, B. Kampfer, O. P. Pavlenko, and G. Soff, Phys. Lett. B, 337: 235 (1994)
[41]	M. I. Gorenstein and S.-N. Yang, Phys. Rev. D, 52: 5206 (1995)
[42]	Z. G. Berezhiani, A. D. Dolgov, and R. N. Mohapatra, Phys. Lett. B, 375: 26 (1996) doi:10.1016/0370-2693(96)00219-5 [hep-ph/9511221]
[43]	A. Drago, M. Gibilisco and C. Ratti, Nucl. Phys. A, 742: 165 (2004) doi:10.1016/j.nuclphysa.2004.06.017 [hep-ph/0112282]
[44]	E. W. Kolb and M. S. Turner, Front. Phys., 69: 1 (1990)
[45]	J. Preskill, M. B. Wise and F. Wilczek, Phys. Lett. B, 120:127 (1983); L. F. Abbott and P. Sikivie, Phys. Lett. B, 120:133 (1983); M. Dine and W. Fischler, Phys. Lett. B, 120: 137 (1983); P. Sikivie, Lect. Notes Phys., 741: 19 (2008)
[46]	P. W. Graham, D. E. Kaplan, and S. Rajendran, Phys. Rev. Lett., 115: 22, 221801 (2015) doi:10.1103/PhysRevLett.115.221801 [arXiv:1504.07551 [hepph]]
[47]	D. Ejlli and A. D. Dolgov, Phys. Rev. D, 90: 063514 (2014) doi:10.1103/PhysRevD.90.063514 [arXiv:1312.3558 [hep-ph]]
[48]	M. Le Bellac, Thermal Field Theory, Cambridge University Press (2000), ISBN 0521654777
[49]	A.Salvio, A.Strumia, and W.Xue, JCAP, 1401: 011 (2014) doi:10.1088/1475-7516/2014/01/011 [arXiv:1310.6982 [hep-ph]]
[50]	D. Blas, J. Lesgourgues, and T. Tram, JCAP, 07: 034 (2011) [arXiv:1104.2933]
[51]	B. Audren, J. Lesgourgues, K. Benabed, and S. Prunet, JCAP, 02: 001 (2013) [arXiv:1210.7183]
[52]	https://github.com/cmbant/getdist
[53]	A.Addazi and M.Bianchi, JHEP, 1412: 089 (2014) doi:10.1007/JHEP12(2014)089 [arXiv:1407.2897 [hep-ph]]
[54]	A.Addazi and M.Bianchi, JHEP, 1507: 144 (2015) doi:10.1007/JHEP07(2015)144 [arXiv:1502.01531 [hep-ph]]
[55]	A.Addazi and M.Bianchi, JHEP, 1506: 012 (2015) doi:10.1007/JHEP06(2015)012 [arXiv:1502.08041 [hep-ph]]
[56]	A. Addazi, M. Bianchi, and G. Ricciardi, JHEP, 1602: 035 (2016) doi:10.1007/JHEP02(2016)035 [arXiv:1510.00243 [hepph]]
[57]	E. Elizalde, J. E. Lidsey, S. Nojiri, and S. D. Odintsov, Phys. Lett. B, 574: 1 (2003) doi:10.1016/j.physletb.2003.08.074 [hepth/0307177]
[58]	A. Addazi, S. Capozziello, and S. Odintsov, Phys. Lett. B, 760: 611 (2016) doi:10.1016/j.physletb.2016.07.047 [arXiv:1607.05706 [gr-qc]]
[59]	M. Carrillo Gonzalez and M. Trodden, arXiv:1705.04737 [astroph.CO]
[60]	T. Abbott et al (DES Collaboration), astro-ph/0510346
[61]	R. Laureijs et al (EUCLID Collaboration), arXiv:1110.3193 [astro-ph.CO]
[62]	S. Dodelson, K. Heitmann, C. Hirata, K. Honscheid, A. Roodman, U. Seljak, A. Slosar, and M. Trodden, arXiv:1604.07626 [astro-ph.CO]
[63]	S. Dodelson, K. Heitmann, C. Hirata, K. Honscheid, A. Roodman, U. Seljak, A. Slosar, and M. Trodden, arXiv:1604.07821 [astro-ph.IM]
[64]	C. P. Ma and E. Bertschinger, Astrophys. J., 455: 7 (1995) doi:10.1086/176550 [astro-ph/9506072]
[65]	W. Yang, N. Banerjee, and S. Pan, Phys. Rev. D, 95(12):123527 (2017) Addendum: [Phys. Rev. D, 96(8): 089903 (2017)] doi:10.1103/PhysRevD.95.123527, 10.1103/PhysRevD.96.089903 [arXiv:1705.09278 [astro-ph.CO]]
[66]	S. Kumar and R. C. Nunes, Eur. Phys. J. C, 77(11): 734 (2017) doi:10.1140/epjc/s10052-017-5334-3 [arXiv:1709.02384 [astroph.CO]]
[67]	J. E. Mandula and M. Ogilvie, Phys. Lett. B, 185: 127 (1987) doi:10.1016/0370-2693(87)91541-3
[68]	S. Gongyo, H. Suganuma, and T. Iritani, PoS ConfinementX, : 050 (2012) [arXiv:1301.2646 [hep-lat]]
[69]	A. C. Aguilar, D. Binosi, and J. Papavassiliou, Front. Phys. (Beijing), 11(2): 111203 (2016) doi:10.1007/s11467-015-0517-6 [arXiv:1511.08361 [hep-ph]]

[1]	Shang Wang , Changbo Fu , De-Chang Dai , Hongwei Wang , Gongtao Fan , Xiguang Cao , Yugang Ma . Searching for dark matter particles using Compton scattering. Chinese Physics C, 2021, 45(9): 093001. doi: 10.1088/1674-1137/ac0c0f
[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]	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
[4]	Rui-Yun Guo , Jing-Fei Zhang , Xin Zhang . Exploring neutrino mass and mass hierarchy in the scenario of vacuum energy interacting with cold dark matter. Chinese Physics C, 2018, 42(9): 095103. doi: 10.1088/1674-1137/42/9/095103
[5]	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
[6]	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
[7]	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
[8]	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
[9]	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
[10]	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
[11]	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
[12]	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
[13]	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
[14]	HU Jie , GONG Hao-Wei , LIN Qing , NI Kai-Xuan , TAN An-Di , WEI Yue-Huan , XIAO Meng-Jiao , XIAO Xiang , ZHAO Li . Development of the liquid level meters for the PandaX dark matter detector. Chinese Physics C, 2014, 38(5): 056002. doi: 10.1088/1674-1137/38/5/056002
[15]	KANG Ke-Jun , YUE Qian , WU Yu-Cheng et al. (CDEX collaboration) and (TEXONO collaboration) . CDEX-1 1 kg point-contact germanium detector for low mass dark matter searches. Chinese Physics C, 2013, 37(12): 126002. doi: 10.1088/1674-1137/37/12/126002
[16]	CHANG Xue , LIU Chun , MA Feng-Cai , YANG Shuo . Supersymmetric extension of the minimal dark matter model. Chinese Physics C, 2012, 36(9): 810-817. doi: 10.1088/1674-1137/36/9/003
[17]	Jeong Ryeol . An approach to dark energy problem through linear invariants. Chinese Physics C, 2011, 35(3): 233-242. doi: 10.1088/1674-1137/35/3/005
[18]	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
[19]	GU Pei-Hong , BI Xiao-Jun , FENG Bo , YOUNG Bing-Lin , ZHANG Xin-Min . Detecting dark energy in long baseline neutrino oscillations. Chinese Physics C, 2008, 32(7): 530-535. doi: 10.1088/1674-1137/32/7/004
[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, Pietro Donà and Antonino Marcianò. Dynamical interactions of dark energy and dark matter: Yang-Mills condensate and QCD axions[J]. Chinese Physics C, 2018, 42(7): 075102. doi: 10.1088/1674-1137/42/7/075102

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 2018-03-16

Fund

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

Article Metric

Article Views(1730)
PDF Downloads(14)
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

Dynamical interactions of dark energy and dark matter: Yang-Mills condensate and QCD axions

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

Dynamical interactions of dark energy and dark matter: Yang-Mills condensate and QCD axions

HTML

目录