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F(R) gravity in the early Universe: electroweak phase transition and chameleon mechanism

F(R) gravity in the early Universe: electroweak phase transition and chameleon mechanism
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摘要 It is widely believed that the screening mechanism is an essential feature for the modified gravity theory. Although this mechanism has been examined thoroughly in the past decade, their analyses are based on a conventional fluid prescription for the matter-sector configuration. In this paper, we demonstrate a new formulation of the chameleon mechanism in F(R) gravity theory, to shed light on quantum-field theoretical effects on the chameleon mechanism as well as the related scalaron physics, induced by the matter sector. We show a possibility that the chameleon mechanism is absent in the early Universe based on a scale-invariant-extended scenario beyond the standard model of particle physics, in which a realistic electroweak phase transition, yielding the right amount of baryon asymmetry of Universe today, simultaneously breaks the scale invariance in the early Universe. We also briefly discuss the oscillation of the scalaron field and indirect generation of non-tensorial gravitational waves induced by the electroweak phase transition. It is widely believed that the screening mechanism is an essential feature for the modified gravity theory.Although this mechanism has been examined thoroughly in the past decade, their analyses are based on a conventional fluid prescription for the matter-sector configuration. In this paper, we demonstrate a new formulation of the chameleon mechanism in F(R) gravity theory, to shed light on quantum-field theoretical effects on the chameleon mechanism as well as the related scalaron physics, induced by the matter sector. We show a possibility that the chameleon mechanism is absent in the early Universe based on a scale-invariant-extended scenario beyond the standard model of particle physics, in which a realistic electroweak phase transition, yielding the right amount of baryon asymmetry of Universe today, simultaneously breaks the scale invariance in the early Universe. We also briefly discuss the oscillation of the scalaron field and indirect generation of non-tensorial gravitational waves induced by the electroweak phase transition.
出处 《Chinese Physics C》 SCIE CAS CSCD 2019年第10期86-98,共13页 中国物理C(英文版)
基金 supported by International Postdoctoral Exchange Fellowship Program at Central China Normal University Project funded by China Postdoctoral Science Foundation(2018M632895) supported in part by the JSPS Grant-in-Aid for Young Scientists(B)(15K17645) National Science Foundation of China(NSFC)(11747308) the Seeds Funding of Jilin University.E.S.is supported by IBS under the project code,IBS-R018-D1
关键词 modified GRAVITY BEYOND standard model THERMAL FIELD THEORY modified gravity beyond standard model thermal field theory
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