Dark matter and baryogenesis in the Fermi-bounce curvaton mechanism

Andrea Addazi; Stephon Alexander; Yi-Fu Cai; Antonino Marcian&oacute;

doi:10.1088/1674-1137/42/6/065101

Chinese Physics C> 2018, Vol. 42> Issue(6) : 065101 DOI: 10.1088/1674-1137/42/6/065101

Dark matter and baryogenesis in the Fermi-bounce curvaton mechanism

1.
Department of Physics &
2.
Department of Physics, Brown University, Providence, RI, 02912, USA
3.
CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Chinese Academy of Sciences, Hefei 230026, China

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Abstract：
We elaborate on a toy model of matter bounce, in which the matter content is constituted by two fermion species endowed with four fermion interaction terms. We describe the curvaton mechanism that is thus generated, and then argue that one of the two fermionic species may realize baryogenesis, while the other (lighter) one is compatible with constraints on extra hot dark matter particles.
- dark matter ,
- matter bounce ,
- fermi bounce ,
- baryogenesis

References

[1]	R. H. Brandenberger, arXiv: 1206.4196
[2]	R. Brandenberger and P. Peter, arXiv: 1603.05834 [hep-th]
[3]	Y.-F. Cai, E. McDonough, F. Duplessis, and R. H. Brandenberger, JCAP, 1310: 024 (2013) [arXiv: 1305.5259 [hep-th]]
[4]	J. Quintin, Z. Sherkatghanad, Y.-F. Cai, and R. H. Brandenberger, Phys. Rev. D, 92: 063532 (2015), arXiv: 1508.04141
[5]	Planck, P. Ade et al, arXiv: 1502.01589
[6]	BICEP2, Planck, P. Ade et al, Phys. Rev. Lett., 114: 101301 (2015), arXiv: 1502.00612
[7]	E. Wilson-Ewing, JCAP, 1303: 026 (2013), arXiv: 1211.6269
[8]	Y.-F. Cai and E. Wilson-Ewing, JCAP, 1503: 006 (2015), arXiv: 1412.2914
[9]	Y. F. Cai, F. Duplessis, D. A. Easson, and D. G. Wang, Phys. Rev. D, 93(4): 043546 (2016) [arXiv: 1512.08979 [astro-ph.CO]]
[10]	Y. F. Cai, R. Brandenberger, and X. Zhang, JCAP, 1103: 003 (2011) doi: 10.1088/1475-7516/2011/03/003 [arXiv: 1101.0822 [hep-th]]
[11]	E. Wilson-Ewing, Separate universes in loop quantum cosmology: framework and applications, to appear in Int. J. Mod. Phys. D, arXiv: 1512.05743
[12]	J. de Haro and Y. F. Cai, Gen. Rel. Grav., 47(8): 95 (2015) [arXiv: 1502.03230 [gr-qc]]
[13]	S. D. Odintsov and V. K. Oikonomou, Phys. Rev. D, 91(6): 064036 (2015) [arXiv: 1502.06125 [gr-qc]]
[14]	J. L. Lehners and E. Wilson-Ewing, JCAP, 1510(10): 038 (2015) [arXiv: 1507.08112 [astro-ph.CO]]
[15]	P. C. Ferreira and D. Pavon, Eur. Phys. J. C, 76(1): 37 (2016) [arXiv: 1509.03725 [gr-qc]]
[16]	R. H. Brandenberger, Y. F. Cai, S. R. Das, E. G. M. Ferreira, I. A. Morrison, and Y. Wang, arXiv: 1601.00231 [hep-th]
[17]	S. Nojiri, S. D. Odintsov, and V. K. Oikonomou, Phys. Rev. D, 93(8): 084050 (2016) [arXiv: 1601.04112 [gr-qc]]
[18]	S. D. Odintsov and V. K. Oikonomou, Phys. Rev. D, 94(6): 064022 (2016) [arXiv: 1606.03689 [gr-qc]]
[19]	Y. F. Cai, A. Marciano, D. G. Wang, and E. Wilson-Ewing, Universe, 3(1): 1 (2016) arXiv: 1610.00938 [astro-ph.CO]
[20]	S. W. Hawking and G. F. R. Ellis, The Large scale structure of space-time, (Cambridge: Cambridge University Press, 1973)
[21]	Y.-F. Cai and E. Wilson-Ewing, JCAP, 1403: 026 (2014) [arXiv: 1402.3009 [gr-qc]]
[22]	R. Durrer, M. Gasperini, M. Sakellariadou and G. Veneziano, Phys. Rev. D, 59: 043511 (1999) doi: 10.1103/PhysRevD.59. 043511 [gr-qc/9804076]
[23]	T. Biswas, A. Mazumdar and W. Siegel, JCAP, 0603: 009 (2006) [hep-th/0508194]
[24]	R. H. Brandenberger, C. Kounnas, H. Partouche, S. P. Patil, and N. Toumbas, JCAP, 1403: 015 (2014) [arXiv: 1312.2524 [hep-th]]
[25]	R. Brandenberger, Phys. Rev. D, 80: 043516 (2009) [arXiv: 0904.2835 [hep-th]]
[26]	S. D. Odintsov and V. K. Oikonomou, Phys. Rev. D, 90(12): 124083 (2014) [arXiv: 1410.8183 [gr-qc]]
[27]	K. Bamba, A. N. Makarenko, A. N. Myagky, and S. D. Odintsov, Phys. Lett. B, 732: 349 (2014) [arXiv: 1403.3242 [hep-th]]
[28]	C. Lin, R. H. Brandenberger, and L. Perreault Levasseur, JCAP, 1104: 019 (2011) [arXiv: 1007.2654 [hep-th]]
[29]	S. Alexander, C. Bambi, A. Marciano, and L. Modesto, Phys. Rev. D, 90(12): 123510 (2014) doi: 10.1103/PhysRevD.90.123510 [arXiv: 1402.5880 [gr-qc]]
[30]	S. Alexander, Y. F. Cai, and A. Marciano, Phys. Lett. B, 745: 97 (2015) doi: 10.1016/j.physletb.2015.04.026 [arXiv: 1406.1456 [gr-qc]]
[31]	S. Alexander, C. Bambi, A. Marciano, and L. Modesto, Phys. Rev. D, 90(12): 123510 (2014) doi: 10.1103/PhysRevD.90.123510 [arXiv: 1402.5880 [gr-qc]]
[32]	Y.-F. Cai, T. -t. Qiu, R. Brandenberger, and X.-m. Zhang, Phys. Rev. D, 80: 023511 (2009) [arXiv: 0810.4677 [hep-th]]
[33]	F. W. Hehl, Phys. Lett. A, 36: 225 (1971); F. W. Hehl, Gen. Relativ. Gravit., 4: 333 (1973); F. W. Hehl, Gen. Relativ. Gravit., 5: 491 (1974); P. von der Heyde, G. D. Kerlick, and J. M. Nester, Rev. Mod. Phys., 48: 393 (1976); E. A. Lord, Tensors, Relativity and Cosmology (New Delhi: McGraw-Hill, 1976); V. de Sabbata and M. Gasperini, Introduction to Gravitation (Singapore: World Scientific, 1985); V. de Sabbata and C. Sivaram, Spin and Torsion in Gravitation (Singapore: World Scientific, 1994); I. L. Shapiro, Phys. Rep., 357: 113 (2002); R. T. Hammond, Rep. Prog. Phys., 65: 599 (2002)
[34]	A. Trautman, Bull. Acad. Pol. Sci. Ser. Math. Astron. Phys., 20: 185, 503, 895 (1972)
[35]	P. van Nieuweinhuizen, Physics Reports, 68: 189 (1981)
[36]	L. Freidel, D. Minic, and T. Takeuchi, Phys. Rev. D, 72: 104002 (2005), arXiv: hep-th/0507253
[37]	A. Perez and C. Rovelli, Phys. Rev. D, 73: 044013 (2006), arXiv: gr-qc/0505081
[38]	C. Bambi, D. Malafarina, A. Marciano, and L. Modesto, Phys. Lett. B, 734: 27 (2014), arXiv: 1402.5719 [gr-qc]
[39]	S. Alexander, T. Biswas, and G. Calcagni, Phys. Rev. D, 81: 043511 (2010); Phys. Rev. D, 81: 069902 (2010) arXiv: 0906.5161 [astro-ph.CO]
[40]	S. Dubovsky, T. Gregoire, A. Nicolis, and R. Rattazzi, JHEP, 0603: 025 (2006) [hep-th/0512260]
[41]	V. A. Rubakov, Phys. Rev. D, 88 (2013) 044015 doi: 10.1103/PhysRevD.88.044015 [arXiv: 1305.2614 [hep-th]]
[42]	B. Elder, A. Joyce, and J. Khoury, Phys. Rev. D, 89(4): 044027 (2014) doi: 10.1103/PhysRevD.89.044027 [arXiv: 1311.5889 [hep-th]]
[43]	V. A. Rubakov, Phys. Usp., 57: 128 (2014); Usp. Fiz. Nauk, 184(2): 137 (2014) doi: 10.3367/UFNe.0184.201402b.0137 [arXiv: 1401.4024 [hep-th]]
[44]	A. Addazi and A. Marciano, in preparation
[45]	J. Khoury, B. A. Ovrut, P. J. Steinhardt, and N. Turok, Phys. Rev. D, 64: 123522 (2001), arXiv: hep-th/0103239
[46]	R. H. Brandenberger and C. Vafa, Nucl. Phys. B, 316: 391 (1989); S. Alexander, R. H. Brandenberger and D. A. Easson, Phys. Rev. D, 62: 103509 (2000), arXiv: hep-th/0005212; A. Nayeri, R. H. Brandenberger and C. Vafa, Phys. Rev. Lett., 97: 021302 (2006) arXiv: hep-th/0511140.
[47]	F. Finelli and R. Brandenberger, Phys. Rev. D, 65: 103522 (2002), arXiv: hep-th/0112249
[48]	D. Wands, Phys. Rev. D, 60: 023507 (1999), arXiv: gr-qc/9809062
[49]	C. Armendariz-Picon and P. B. Greene, Gen. Rel. Grav., 35: 1637 (2003), hep-th/0301129, hep-th/0301129
[50]	N. J. Poplawski, Phys. Rev. D, 85: 107502 (2012), arXiv: 1111.4595 [gr-qc]
[51]	S. Alexander and T. Biswas, Phys. Rev. D, 80: 023501 (2009), arXiv: 0807.4468 [hep-th]
[52]	J. Magueijo, T. G. Zlosnik, and T. W. B. Kibble, Phys. Rev. D, 87(6): 063504 (2013), arXiv: 1212.0585 [astro-ph.CO]
[53]	M. Bojowald and R. Das, Phys. Rev. D, 78: 064009 (2008), arXiv: 0710.5722 [gr-qc]
[54]	M. Bojowald and R. Das, Class. Quant. Grav., 25: 195006 (2008), arXiv: 0806.2821 [gr-qc]
[55]	S. Mercuri, Phys. Rev. D, 73: 084016 (2006), arXiv: gr-qc/0601013
[56]	P. Dona, A. Marciano and X. Gan, in preparation
[57]	P. Dona and A. Marciano, Phys. Rev. D, 94(2): 123517 (2016) doi: 10.1103/PhysRevD.94.123517 arXiv: 1605.09337 [gr-qc]
[58]	Y.-F. Cai, D. A. Easson, and R. Brandenberger, JCAP, 1208: 020 (2012) [arXiv: 1206.2382 [hep-th]]
[59]	P. A. R. Ade et al (Planck Collaboration), arXiv: 1303.5076 [astro-ph.CO]
[60]	R. A. Battye and A. Moss, Phys. Rev. Lett., 112: 051303 (2014) [arXiv: 1308.5870 [astro-ph.CO]]
[61]	V. A. Kuzmin, V. A. Rubakov, N. E. Shaposhnikov, Phys. Lett. B, 155: 36 (1985)
[62]	H. Georgi, Phys. Lett. B, 108: 283 (1982)
[63]	M. Fukugita, T. Yanagida, Phys.Lett. B, 174: 45 (1986)
[64]	W. Buchmuller, R. D. Peccei, and T. Yanagida, Ann. Rev. Nucl. Part. Sci., 55: 311 (2005) doi: 10.1146/annurev.nucl.55.090704.151558 [hep-ph/0502169]
[65]	A. D. Sakharov, JETP Lett., 5: 24 (1967)
[66]	L. P. Kadanoff, G. Baym, Quantum Statistical Mechanics, (New York: Benjamin, 1962)

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Andrea Addazi, Stephon Alexander, Yi-Fu Cai and Antonino Marcianó. Dark matter and baryogenesis in the Fermi-bounce curvaton mechanism[J]. Chinese Physics C, 2018, 42(6): 065101. doi: 10.1088/1674-1137/42/6/065101

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Received: 2018-01-15
Revised: 2018-04-11

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The work of AA was partially supported during this collaboration by the MIUR research grant Theoretical Astroparticle Physics PRIN 2012CPPYP7 and by SdC Progetto speciale Multiasse La Societ della Conoscenza in Abruzzo PO FSE Abruzzo 2007-2013. The work of YFC is supported in part by the Chinese National Youth Thousand Talents Program (KJ2030220006), by the USTC start-up funding (KY2030000049), by the NSFC (11421303, 11653002), and by the Fund for Fostering Talents in Basic Science of the NSFC (J1310021). AM wishes to acknowledge support by the Shanghai Municipality, through the grant No. KBH1512299, and by Fudan University, through the grant No. JJH1512105

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