Limiting majoron self-interactions from gravitational wave experiments

Andrea Addazi; Antonino Marcian&ograve;

doi:10.1088/1674-1137/42/2/023105

Chinese Physics C> 2018, Vol. 42> Issue(2) : 023105 DOI: 10.1088/1674-1137/42/2/023105

Limiting majoron self-interactions from gravitational wave experiments

Andrea Addazi ^, ,
Antonino Marcianò

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Abstract：
We show how majoron models may be tested/limited in gravitational wave experiments. In particular, the majoron self-interaction potential may induce a first order phase transition, producing gravitational waves from bubble collisions. We dub such a new scenario the violent majoron model, because it would be associated with a violent phase transition in the early Universe. Sphaleron constraints can be avoided if the global U(1)_B-L is broken at scales lower than the electroweak scale, provided that the B-L spontaneously breaking scale is lower than 10 {TeV} in order to satisfy the cosmological mass density bound. The possibility of a sub-electroweak phase transition is practically unconstrained by cosmological bounds and it may be detected within the sensitivity of the next generation of gravitational wave experiments:eLISA, DECIGO and BBO. We also comment on its possible detection in the next generation of electron-positron colliders, where majoron production can be observed from the Higgs portals in missing transverse energy channels.
- lepton/baryon number violation ,
- majorons ,
- gravitational waves ,
- colliders

References

[1]	E. Majorana, Theory of the Symmetry of Electrons and Positrons, Nuovo Cimento, 14:171 (1937)
[2]	Y. Chikashige, R. N. Mohapatra, and R. D. Peccei, Phys. Lett. B, 98:265 (1981) doi:10.1016/0370-2693(81)90011-3
[3]	G. B. Gelmini and M. Roncadelli, Phys. Lett. B, 99:411 (1981) doi:10.1016/0370-2693(81)90559-1
[4]	J. Schechter and J. W. F. Valle, Phys. Rev. D, 25:774 (1982) doi:10.1103/PhysRevD.25.774
[5]	V. Berezinsky and J. W. F. Valle, Phys. Lett. B, 318:360 (1993) doi:10.1016/0370-2693(93)90140-D[hep-ph/9309214]
[6]	G. Steigman, K.A. Olive, and D.N. Schramm, Phys. Rev. Lett., 43:239 (1979)
[7]	K. A. Olive, D. N. Schramm, and G. Steigman, Nucl. Phys. B, 180:497 (1981)
[8]	K. A. Olive, D. N. Schramm, G. Steigman, and T.P. Walker, Phys. Lett. B, 236:454 (1990)
[9]	T. P. Walker, G. Steigman, D. N. Schramm, K. A. Olive, and H. S. Kang, Ap. J., 376:51 (1991)
[10]	J. M. Cline, K. Kainulainen, and K. A. Olive, Astropart. Phys., 1:387 (1993) doi:10.1016/0927-6505(93)90005-X[hep-ph/9304229]
[11]	E. K. Akhmedov, Z. G. Berezhiani, R. N. Mohapatra, and G. Senjanovic, Phys. Lett. B, 299:90 (1993) doi:10.1016/0370-2693(93)90887-N[hep-ph/9209285]
[12]	A. Addazi and M. Bianchi, JHEP, 1412:089 (2014) doi:10.1007/JHEP12(2014)089[arXiv:1407.2897[hep-ph]]
[13]	A. Addazi, Mod. Phys. Lett. A, 32(2):1750014 (2016) doi:10.1142/S0217732317500146[arXiv:1607.01203[hep-th]]
[14]	Z. Berezhiani, Eur. Phys. J. C, 76(12):705 (2016) doi:10.1140/epjc/s10052-016-4564-0[arXiv:1507.05478[hep-ph]]
[15]	A. Addazi, Nuovo Cim. C, 38(1):21 (2015) doi:10.1393/ncc/i2015-15021-6
[16]	A. Addazi, JHEP, 1504:153 (2015) doi:10.1007/JHEP04(2015)153[arXiv:1501.04660[hep-ph]]
[17]	A. Addazi, Z. Berezhiani, and Y. Kamyshkov, arXiv:1607.00348[hep-ph]
[18]	C. Caprini et al, JCAP, 1604(4):001 (2016) doi:10.1088/1475-7516/2016/04/001[arXiv:1512.06239[astro-ph.CO]]
[19]	H. Kudoh, A. Taruya, T. Hiramatsu, and Y. Himemoto, Phys. Rev. D, 73:064006 (2006) doi:10.1103/PhysRevD.73.064006[gr-qc/0511145]
[20]	H. Audley et al, arXiv:1702.00786[astro-ph.IM]
[21]	E. Witten, Phys. Rev. D, 30:272 (1984) doi:10.1103/PhysRevD.30.272
[22]	M. S. Turner and F. Wilczek, Phys. Rev. Lett., 65:3080 (1990) doi:10.1103/PhysRevLett.65.3080
[23]	C. J. Hogan, Mon. Not. Roy. Astron. Soc., 218:629 (1986)
[24]	A. Kosowsky, M. S. Turner, and R. Watkins, Phys. Rev. D, 45:4514 (1992) doi:10.1103/PhysRevD.45.4514
[25]	M. Kamionkowski, A. Kosowsky, and M. S. Turner, Phys. Rev. D, 49:2837 (1994) doi:10.1103/PhysRevD.49.2837[astro-ph/9310044]
[26]	R. Jinno and M. Takimoto, Phys. Rev. D, 95(2):024009 (2017) doi:10.1103/PhysRevD.95.024009[arXiv:1605.01403[astro-ph.CO]]
[27]	R. Jinno and M. Takimoto, arXiv:1707.03111[hep-ph]
[28]	R. Jinno, S. Lee, H. Seong, and M. Takimoto, arXiv:1708.01253[hep-ph]
[29]	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[hep-ph]]
[30]	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[astro-ph.CO]]
[31]	P. Schwaller, Phys. Rev. Lett., 115(18):181101 (2015) doi:10.1103/PhysRevLett.115.181101[arXiv:1504.07263[hep-ph]]
[32]	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]]
[33]	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]]
[34]	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]]
[35]	M. Artymowski, M. Lewicki, and J. D. Wells, arXiv:1609.07143[hep-ph]
[36]	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]]
[37]	A. Katz and A. Riotto, arXiv:1608.00583[hep-ph]
[38]	F. P. Huang and X. Zhang, arXiv:1701.04338[hep-ph]
[39]	I. Baldes, arXiv:1702.02117[hep-ph]
[40]	W. Chao, H. K. Guo, and J. Shu, arXiv:1702.02698[hep-ph]
[41]	A. Addazi, Mod. Phys. Lett. A, 32(8) 1750049 (2017)[arXiv:1607.08057[hep-ph]]
[42]	P. H. Ghorbani, arXiv:1703.06506[hep-ph]
[43]	K. Tsumura, M. Yamada, and Y. Yamaguchi, arXiv:1704.00219[hep-ph]
[44]	F. P. Huang and J. H. Yu, arXiv:1704.04201[hep-ph]
[45]	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]]
[46]	S. Chatrchyan et al (CMS Collaboration), Eur. Phys. J. C, 74:2980 (2014) doi:10.1140/epjc/s10052-014-2980-6[arXiv:1404.1344[hep-ex]]
[47]	C. Patrignani et al (Particle Data Group), Chin. Phys. C, 40:100001 (2016)
[48]	M. Bicer et al (TLEP Design Study Working Group Collaboration), JHEP, 1401:164 (2014)[arXiv:1308.6176[hep-ex]]
[49]	Technical Design Report, The ILC Baseline Design, https://forge.linearcollider.org/dist/20121210-CA-TDR2.pdf (2013)
[50]	A. Freitas, K. Hagiwara, S. Heinemeyer, P. Langacker, K. Moenig, M. Tanabashi, and G. W. Wilson, arXiv:1307.3962[hep-ph]
[51]	T. Golling et al, CERN Yellow Report no.3, 441 (2017) doi:10.23731/CYRM-2017-003.441[arXiv:1606.00947[hep-ph]]
[52]	J. Ellis and T. You, JHEP, 1603:089 (2016) doi:10.1007/JHEP03(2016)089[arXiv:1510.04561[hep-ph]].
[53]	M. J. Boland et al (CLIC and CLICdp Collaborations), doi:10.5170/CERN-2016-004 arXiv:1608.07537[physics.acc-ph]
[54]	N. Baouche and A. Ahriche, Phys. Rev. D, 96(5):055029 (2017) doi:10.1103/PhysRevD.96.055029[arXiv:1707.05263[hep-ph]]
[55]	J. L. Abelleira Fernandez et al (LHeC Study Group), J. Phys. G, 39:075001 (2012) doi:10.1088/0954-3899/39/7/075001[arXiv:1206.2913[physics.acc-ph]]

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Andrea Addazi and Antonino Marcianò. Limiting majoron self-interactions from gravitational wave experiments[J]. Chinese Physics C, 2018, 42(2): 023105. doi: 10.1088/1674-1137/42/2/023105

Andrea Addazi and Antonino Marcianò. Limiting majoron self-interactions from gravitational wave experiments[J]. Chinese Physics C, 2018, 42(2): 023105. doi: 10.1088/1674-1137/42/2/023105 shu

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Received: 2017-10-09

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Supported by the Shanghai Municipality, through the grant No. KBH1512299, and by Fudan University, through the grant No. JJH1512105

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Limiting majoron self-interactions from gravitational wave experiments

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