Gravitational waves at aLIGO and vacuum stability with a scalar singlet extension of the standard model

被引:50
作者
Balazs, Csaba [1 ,2 ]
Fowlie, Andrew [1 ]
Mazumdar, Anupam [3 ,4 ]
White, Graham A. [1 ]
机构
[1] Monash Univ, Sch Phys & Astron, ARC Ctr Excellence Particle Phys Tera Scale, Melbourne, Vic 3800, Australia
[2] Monash Univ, Sch Phys & Astron, Monash Ctr Astrophys, Melbourne, Vic 3800, Australia
[3] Univ Lancaster, Dept Phys, Consortium Fundamental Phys, Lancaster LA1 4YB, England
[4] Univ Groningen, Kapteyn Astron Inst, NL-9700 AV Groningen, Netherlands
基金
英国科学技术设施理事会; 澳大利亚研究理事会;
关键词
RADIATION; NUCLEATION; INFLATION;
D O I
10.1103/PhysRevD.95.043505
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A new gauge singlet scalar field can undergo a strongly first-order phase transition (PT) leading to gravitational waves (GW) potentially observable at aLIGO and stabilizes the electroweak vacuum at the same time by ensuring that the Higgs quartic coupling remains positive up to at least the grand unification (GUT) scale. aLIGO (O5) is potentially sensitive to cosmological PTs at 10(7)-10(8) GeV, which coincides with the requirement that the singlet scale is less than the standard model (SM) vacuum instability scale, which is between 10(8) GeV and 10(14) GeV. After sampling its parameter space, we identify three benchmark points with a PT at about T approximate to 10(7) GeV in a gauge singlet extension of the SM. We calculate the nucleation temperature, order parameter, characteristic time scale, and peak amplitude and frequency of GW from bubble collisions during the PT for the benchmarks and find that, in an optimistic scenario, GW from such a PT may be in reach of aLIGO (O5). We confirm that the singlet stabilizes the electroweak vacuum while remaining consistent with zero-temperature phenomenology as well. Thus, this scenario presents an intriguing possibility that aLIGO may detect traces of fundamental physics motivated by vacuum stability at an energy scale that is well above the reach of any other experiment.
引用
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页数:10
相关论文
共 90 条
[1]   Observation of Gravitational Waves from a Binary Black Hole Merger [J].
Abbott, B. P. ;
Abbott, R. ;
Abbott, T. D. ;
Abernathy, M. R. ;
Acernese, F. ;
Ackley, K. ;
Adams, C. ;
Adams, T. ;
Addesso, P. ;
Adhikari, R. X. ;
Adya, V. B. ;
Affeldt, C. ;
Agathos, M. ;
Agatsuma, K. ;
Aggarwal, N. ;
Aguiar, O. D. ;
Aiello, L. ;
Ain, A. ;
Ajith, P. ;
Allen, B. ;
Allocca, A. ;
Altin, P. A. ;
Anderson, S. B. ;
Anderson, W. G. ;
Arai, K. ;
Arain, M. A. ;
Araya, M. C. ;
Arceneaux, C. C. ;
Areeda, J. S. ;
Arnaud, N. ;
Arun, K. G. ;
Ascenzi, S. ;
Ashton, G. ;
Ast, M. ;
Aston, S. M. ;
Astone, P. ;
Aufmuth, P. ;
Aulbert, C. ;
Babak, S. ;
Bacon, P. ;
Bader, M. K. M. ;
Baker, P. T. ;
Baldaccini, F. ;
Ballardin, G. ;
Ballmer, S. W. ;
Barayoga, J. C. ;
Barclay, S. E. ;
Barish, B. C. ;
Barker, D. ;
Barone, F. .
PHYSICAL REVIEW LETTERS, 2016, 116 (06)
[2]   GW150914: Implications for the Stochastic Gravitational-Wave Background from Binary Black Holes [J].
Abbott, B. P. ;
Abbott, R. ;
Abbott, T. D. ;
Abernathy, M. R. ;
Acernese, F. ;
Ackley, K. ;
Adams, C. ;
Adams, T. ;
Addesso, P. ;
Adhikari, R. X. ;
Adya, V. B. ;
Affeldt, C. ;
Agathos, M. ;
Agatsuma, K. ;
Aggarwal, N. ;
Aguiar, O. D. ;
Aiello, L. ;
Ain, A. ;
Ajith, P. ;
Allen, B. ;
Allocca, A. ;
Altin, P. A. ;
Anderson, S. B. ;
Anderson, W. G. ;
Arai, K. ;
Araya, M. C. ;
Arceneaux, C. C. ;
Areeda, J. S. ;
Arnaud, N. ;
Arun, K. G. ;
Ascenzi, S. ;
Ashton, G. ;
Ast, M. ;
Aston, S. M. ;
Astone, P. ;
Aufmuth, P. ;
Aulbert, C. ;
Babak, S. ;
Bacon, P. ;
Bader, M. K. M. ;
Baker, P. T. ;
Baldaccini, F. ;
Ballardin, G. ;
Ballmer, S. W. ;
Barayoga, J. C. ;
Barclay, S. E. ;
Barish, B. C. ;
Barker, D. ;
Barone, F. ;
Barr, B. .
PHYSICAL REVIEW LETTERS, 2016, 116 (13)
[3]   Semi-analytic techniques for calculating bubble wall profiles [J].
Akula, Sujeet ;
Balazs, Csaba ;
White, Graham A. .
EUROPEAN PHYSICAL JOURNAL C, 2016, 76 (12)
[4]   The top quark and Higgs boson masses and the stability of the electroweak vacuum [J].
Alekhin, S. ;
Djouadi, A. ;
Moch, S. .
PHYSICS LETTERS B, 2012, 716 (01) :214-219
[5]  
[Anonymous], P 16 INT C GEN REL G
[6]  
[Anonymous], THESIS
[7]  
[Anonymous], 2016, arXiv:1608.06619
[8]  
[Anonymous], ARXIV10115881
[9]  
[Anonymous], ARXIV10101546
[10]  
[Anonymous], ARXIV160907143