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

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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]]

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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

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Received: 2018-03-16

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

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