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

Abstract
HTML
Reference
Related

PDF

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]]

[1]	Reggie C. Pantig , Ali Övgün . Imprints of a gravitational wave through the weak field deflection of photons. Chinese Physics C, 2024, 48(8): 085104. doi: 10.1088/1674-1137/ad4e25
[2]	Yu-Xin Wang , Shang-Jie Jin , Tian-Yang Sun , Jing-Fei Zhang , Xin Zhang . Rapid identification of time-frequency domain gravitational wave signals from binary black holes using deep learning. Chinese Physics C, 2024, 48(11): 1-14.
[3]	Zhe Chang , Yu-Ting Kuang , Xukun Zhang , Jing-Zhi Zhou . Primordial black holes and third order scalar induced gravitational waves. Chinese Physics C, 2023, 47(5): 055104. doi: 10.1088/1674-1137/acc649
[4]	Ze-Yu Qiu , Zhao-Huan Yu . Gravitational waves from cosmic strings associated with pseudo-Nambu-Goldstone dark matter. Chinese Physics C, 2023, 47(8): 085104. doi: 10.1088/1674-1137/acd9bf
[5]	Haipeng An , Kun-Feng Lyu , Lian-Tao Wang , Siyi Zhou . A unique gravitational wave signal from phase transition during inflation. Chinese Physics C, 2022, 46(10): 101001. doi: 10.1088/1674-1137/ac76a7
[6]	F. P. An , A. B. Balantekin , H. R. Band , M. Bishai , S. Blyth , G. F. Cao , J. Cao , J. F. Chang , Y. Chang , H. S. Chen , S. M. Chen , Y. Chen , Y. X. Chen , J. Cheng , Z. K. Cheng , J. J. Cherwinka , M. C. Chu , J. P. Cummings , O. Dalager , F. S. Deng , Y. Y. Ding , M. V. Diwan , T. Dohnal , J. Dove , M. Dvořák , D. A. Dwyer , J. P. Gallo , M. Gonchar , G. H. Gong , H. Gong , W. Q. Gu , J. Y. Guo , L. Guo , X. H. Guo , Y. H. Guo , Z. Guo , R. W. Hackenburg , S. Hans , M. He , K. M. Heeger , Y. K. Heng , A. Higuera , Y. K. Hor , Y. B. Hsiung , B. Z. Hu , J. R. Hu , T. Hu , Z. J. Hu , H. X. Huang , X. T. Huang , Y. B. Huang , P. Huber , D. E. Jaffe , K. L. Jen , X. L. Ji , X. P. Ji , R. A. Johnson , D. Jones , L. Kang , S. H. Kettell , S. Kohn , M. Kramer , T. J. Langford , J. Lee , J. H. C. Lee , R. T. Lei , R. Leitner , J. K. C. Leung , F. Li , J. J. Li , Q. J. Li , S. Li , S. C. Li , W. D. Li , X. N. Li , X. Q. Li , Y. F. Li , Z. B. Li , H. Liang , C. J. Lin , G. L. Lin , S. Lin , J. J. Ling , J. M. Link , L. Littenberg , B. R. Littlejohn , J. C. Liu , J. L. Liu , C. Lu , H. Q. Lu , J. S. Lu , K. B. Luk , X. B. Ma , X. Y. Ma , Y. Q. Ma , C. Marshall , D. A. Martinez Caicedo , K. T. McDonald , R. D. McKeown , Y. Meng , J. Napolitano , D. Naumov , E. Naumova , J. P. Ochoa-Ricoux , A. Olshevskiy , H. -R. Pan , J. Park , S. Patton , J. C. Peng , C. S. J. Pun , F. Z. Qi , M. Qi , X. Qian , N. Raper , J. Ren , C. Morales Reveco , R. Rosero , B. Roskovec , X. C. Ruan , H. Steiner , J. L. Sun , T. Tmej , K. Treskov , W. -H. Tse , C. E. Tull , B. Viren , V. Vorobel , C. H. Wang , J. Wang , M. Wang , N. Y. Wang , R. G. Wang , W. Wang , W. Wang , X. Wang , Y. Wang , Y. F. Wang , Z. Wang , Z. Wang , Z. M. Wang , H. Y. Wei , L. H. Wei , L. J. Wen , K. Whisnant , C. G. White , H. L. H. Wong , E. Worcester , D. R. Wu , F. L. Wu , Q. Wu , W. J. Wu , D. M. Xia , Z. Q. Xie , Z. Z. Xing , J. L. Xu , T. Xu , T. Xue , C. G. Yang , L. Yang , Y. Z. Yang , H. F. Yao , M. Ye , M. Yeh , B. L. Young , H. Z. Yu , Z. Y. Yu , B. B. Yue , S. Zeng , Y. Zeng , L. Zhan , C. Zhang , F. Y. Zhang , H. H. Zhang , J. W. Zhang , Q. M. Zhang , X. T. Zhang , Y. M. Zhang , Y. X. Zhang , Y. Y. Zhang , Z. J. Zhang , Z. P. Zhang , Z. Y. Zhang , J. Zhao , L. Zhou , H. L. Zhuang , J. H. Zou , (Daya Bay Collaboration) . Search for electron-antineutrinos associated with gravitational-wave events GW150914, GW151012, GW151226, GW170104, GW170608, GW170814, and GW170817 at Daya Bay. Chinese Physics C, 2021, 45(5): 055001. doi: 10.1088/1674-1137/abe84b
[7]	Hai-Nan Lin , Xin Li , Li Tang . Strongly lensed gravitational waves as probes to test the cosmic distance duality relation. Chinese Physics C, 2021, 45(1): 015109. doi: 10.1088/1674-1137/abc53a
[8]	Hai-Nan Lin , Xin Li . A new method to test the cosmic distance duality relation using the strongly lensed gravitational waves. Chinese Physics C, 2020, 44(7): 075101. doi: 10.1088/1674-1137/44/7/075101
[9]	Y. C. Acar , U. Kaya , B. B. Oner . Resonant production of color octet muons at Future Circular Collider-based muon-proton colliders. Chinese Physics C, 2018, 42(8): 083108. doi: 10.1088/1674-1137/42/8/083108
[10]	Yan-Bing Wei , Run-Hui Li , Dan Luo , Cai-Dian Lü , Yue-Long Shen . Exclusive production of B_c mesons in e⁺e^- colliders. Chinese Physics C, 2018, 42(8): 083107. doi: 10.1088/1674-1137/42/8/083107
[11]	Xin Li , Li Tang , Hai-Nan Lin , Li-Li Wang . Testing the variation of the fine structure constant with strongly lensed gravitational waves. Chinese Physics C, 2018, 42(9): 095104. doi: 10.1088/1674-1137/42/9/095104
[12]	Qing-Hong Cao , Fa-Peng Huang , Ke-Pan Xie , Xinmin Zhang . Testing the electroweak phase transition in scalar extension models at lepton colliders. Chinese Physics C, 2018, 42(2): 023103. doi: 10.1088/1674-1137/42/2/023103
[13]	Ligong Bian , Huai-Ke Guo , Jing Shu . Gravitational Waves, baryon asymmetry of the universe and electric dipole moment in the CP-violating NMSSM. Chinese Physics C, 2018, 42(9): 093106. doi: 10.1088/1674-1137/42/9/093106
[14]	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
[15]	Andrea Addazi , Xian-Wei Kang , Maxim Yu. Khlopov . Testing B-violating signatures from exotic instantons in future colliders. Chinese Physics C, 2017, 41(9): 093102. doi: 10.1088/1674-1137/41/9/093102
[16]	Yi Jin , Shi-Yuan Li , Yan-Rui Liu , Lu Meng , Zong-Guo Si , Xiao-Feng Zhang . Exotic hadron bound state production at hadron colliders. Chinese Physics C, 2017, 41(8): 083106. doi: 10.1088/1674-1137/41/8/083106
[17]	Hao Wen , Fang-Yu Li , Jin Li , Zhen-Yun Fang , Andrew Beckwith . Very high-frequency gravitational waves from magnetars and gamma-ray bursts. Chinese Physics C, 2017, 41(12): 125101. doi: 10.1088/1674-1137/41/12/125101
[18]	null . Signal photon flux generated by high-frequency relic gravitational waves. Chinese Physics C, 2016, 40(8): 085101. doi: 10.1088/1674-1137/40/8/085101
[19]	DONG Hai-Rong , FENG Feng , LI Hai-Bo . Lepton number violation in D meson decay. Chinese Physics C, 2015, 39(1): 013101. doi: 10.1088/1674-1137/39/1/013101
[20]	YANG Jin-Min , Young Bing-Lin . Searching for Top Squark at Hadron Colliders. Chinese Physics C, 2002, 26(S1): 25-33.

Access

Get Citation

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

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 2017-10-09

Fund

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

Article Metric

Article Views(1574)
PDF Downloads(25)
Cited by(0)

Policy on re-use

To reuse of Open Access content published by CPC, for content published under the terms of the Creative Commons Attribution 3.0 license (“CC CY”), the users don’t need to request permission to copy, distribute and display the final published version of the article and to create derivative works, subject to appropriate attribution.

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

Limiting majoron self-interactions from gravitational wave experiments

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

Limiting majoron self-interactions from gravitational wave experiments

Corresponding author: Andrea Addazi,

HTML

目录