4.6 Article

Thermalization process after inflation and effective potential of scalar field

出版社

IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2016/02/003

关键词

inflation; particle physics - cosmology connection; physics of the early universe; cosmological phase transitions

资金

  1. World Premier International Research Center (WPI), MEXT, Japan
  2. JSPS Research Fellowships [25.8715]
  3. Program for Leading Graduate Schools, MEXT, Japan
  4. Grants-in-Aid for Scientific Research [13J08715, 15J07034] Funding Source: KAKEN

向作者/读者索取更多资源

We investigate the thermalization process of the Universe after inflation to determine the evolution of the effective temperature. The time scale of thermalization is found to be so long that it delays the evolution of the effective temperature, and the resulting maximal temperature of the Universe can be significantly lower than the one obtained in the literature. Our results clarify the finite density corrections to the effective potential of a scalar field and also processes of heavy particle production. In particular, we find that the maximum temperature of the Universe may be at most electroweak scale if the reheating temperature is as low as O(1) MeV, which implies that the electroweak symmetry may be marginally restored. In addition, it is noticeable that the dark matter may not be produced from thermal plasma in such a low reheating scenario, since the maximum temperature can be smaller than the conventional estimation by five orders of magnitude. We also give implications to the Peccei-Quinn mechanism and the Affleck-Dine baryogenesis.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.6
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

Article Physics, Particles & Fields

Non-Abelian electric field correlator at NLO for dark matter relic abundance and quarkonium transport

Tobias Binder, Kyohei Mukaida, Bruno Scheihing-Hitschfeld, Xiaojun Yao

Summary: This article presents a complete next-to-leading order calculation of the non-Abelian electric field correlator in a SU(N-c) plasma, providing insights into the properties of the plasma that are relevant for heavy particle bound state formation and dissociation.

JOURNAL OF HIGH ENERGY PHYSICS (2022)

Article Physics, Particles & Fields

Scalar field couplings to quadratic curvature and decay into gravitons

Yohei Ema, Kyohei Mukaida, Kazunori Nakayama

Summary: The hidden sector scalar field generically couples to quadratic curvature through dimension five operators, potentially inducing decays into graviton pairs. Decay of the scalar field can produce a significant amount of stochastic cosmic graviton background at high frequencies due to the suppression scale being determined by the mass of heavy particles rather than the Planck scale. The resulting graviton spectrum is computed in specific models, highlighting the phenomenological interest of these scalar couplings.

JOURNAL OF HIGH ENERGY PHYSICS (2022)

Article Physics, Multidisciplinary

Baryon Asymmetry of the Universe from Lepton Flavor Violation

Kyohei Mukaida, Kai Schmitz, Masaki Yamada

Summary: Charged-lepton flavor violation (CLFV) is a distinct feature of physics beyond the standard model, which plays an important role in the early universe. This Letter points out that efficient CLFV interactions create new pathways for generating the baryon asymmetry of the universe, and the conversion factor from lepton flavor asymmetry to baryon asymmetry is naturally explained by the suppression of charged-lepton Yukawa couplings squared.

PHYSICAL REVIEW LETTERS (2022)

Article Physics, Particles & Fields

Cascades of high-energy SM particles in the primordial thermal plasma

Kyohei Mukaida, Masaki Yamada

Summary: This paper investigates the thermalization of high-energy standard model particles in thermal plasma, considering the Landau-Pomeranchuk-Migdal effect. The distribution function of each particle species is calculated numerically and analytically. The results demonstrate that, after multiple splittings, the particle distributions converge to certain values at low momentum, independent of the high-energy particles injected by inflaton decay. This is helpful for calculating the dark matter abundance produced during the pre-thermal phase.

JOURNAL OF HIGH ENERGY PHYSICS (2022)

Article Physics, Particles & Fields

Charge transfer between rotating complex scalar fields

Valerie Domcke, Keisuke Harigaya, Kyohei Mukaida

Summary: We study the transfer of charge between complex scalar fields and find that under certain conditions, this transfer can be very efficient. This has important implications for cosmological studies involving complex scalar fields.

JOURNAL OF HIGH ENERGY PHYSICS (2022)

Article Astronomy & Astrophysics

Formation of hot spots around small primordial black holes

Minxi He, Kazunori Kohri, Kyohei Mukaida, Masaki Yamada

Summary: This paper investigates the thermalization of Hawking radiation from primordial black holes in the early Universe, taking into account the interference effect on thermalization of high energy particles. The findings show that small primordial black holes completely evaporate before the big bang nucleosynthesis, and the radiation emitted from these black holes results in a hot spot with a non-trivial temperature profile around them.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2023)

Article Astronomy & Astrophysics

Stochastic formalism for U(1) gauge fields in axion inflation

Tomohiro Fujita, Kyohei Mukaida, Yuichiro Tada

Summary: In this study, we develop a stochastic formalism for U(1) gauge fields coupled with a rolling pseudo-scalar field during inflation. We derive the Langevin equations for the physical electromagnetic fields and study their analytic solutions. Through numerical simulation, we demonstrate that the averaged electromagnetic fields over the Hubble scale continuously change their direction and fluctuate around the analytically obtained expectation values. While the isotropy is spontaneously broken in each local Hubble patch, it is globally preserved by averaging all the Hubble patches.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2022)

Article Physics, Particles & Fields

Transient phenomena in the axion assisted Schwinger effect

Valerie Domcke, Yohei Ema, Kyohei Mukaida

Summary: This paper investigates the problem of particle production in a time-dependent background, focusing on the transient effects of fermions in a homogeneous axion background. The definition of particles and antiparticles at intermediate times in the presence of external fields is more ambiguous compared to the asymptotic states in conventional cases, and these external fields also lead to divergences that require regularization.

JOURNAL OF HIGH ENERGY PHYSICS (2022)

Article Physics, Particles & Fields

Wash-in leptogenesis after axion inflation

Valerie Domcke, Kohei Kamada, Kyohei Mukaida, Kai Schmitz, Masaki Yamada

Summary: CP violations and B-L violations are not required to occur simultaneously for successful leptogenesis. New CP-violating interactions at high energies can result in primordial charge asymmetries, which can then be transformed into a nonvanishing B-L asymmetry by right-handed neutrinos at lower energies. In this paper, we study a novel mechanism known as wash-in leptogenesis, using axion inflation as the source of high-scale CP violation. We find a large range of viable scenarios and provide insights into intergalactic magnetic fields, primordial black holes, and gravitational waves.

JOURNAL OF HIGH ENERGY PHYSICS (2023)

Article Astronomy & Astrophysics

Cosmic F- and D-strings from pure Yang-Mills theory

Masaki Yamada, Kazuya Yonekura

Summary: We discuss the formation of cosmic strings or macroscopic color flux tubes after the deconfinement/con-finement phase transition in the pure Yang-Mills theory. These cosmic strings, based on holographic dual descriptions, can be interpreted as F-strings or D-strings in the gravity side, depending on the structure of the gauge group. The reconnection probabilities of F- and D-strings are suppressed by factors of 1/N^2 and e^-cN, respectively, in the large-N limit. The formation of color flux tubes after the phase transition is similar to the formation of local cosmic strings after spontaneous symmetry breaking in the weak-U(1) gauge theory. We use a velocity-dependent one-scale model to describe the dynamics of the string network and calculate the gravitational wave signals from string loops, considering the dependence on the size of produced string loops.

PHYSICS LETTERS B (2023)

Article Astronomy & Astrophysics

Axion dark matter from first-order phase transition, and very high energy photons from GRB 221009A

Shota Nakagawa, Fuminobu Takahashi, Masaki Yamada, Wen Yin

Summary: This study investigates the behavior of an axion-like particle (ALP) that goes through a first-order phase transition in terms of its mass or potential minimum. It is observed that if the ALP obtains a potential from non-perturbative effects of SU(N) gauge theory confined via the first-order phase transition, similar dynamics can be achieved as in the trapped misalignment mechanism. The enhanced ALP abundance in this mechanism provides an explanation for dark matter and is accessible to experiments such as IAXO, ALPS-II, and DM-radio.

PHYSICS LETTERS B (2023)

Article Physics, Multidisciplinary

New Constraint on Primordial Lepton Flavor Asymmetries

Valerie Domcke, Kohei Kamada, Kyohei Mukaida, Kai Schmitz, Masaki Yamada

Summary: This letter investigates the relationship between helical hypermagnetic fields and fermion asymmetry in the early Universe caused by chiral chemical potential. The study demonstrates that even with zero total lepton number, a mechanism can be triggered through lepton flavor asymmetry. This sets a constraint on lepton flavor asymmetry at temperatures above 106 GeV, which is about two orders of magnitude stronger than current limits from cosmic microwave background and primordial nucleosynthesis.

PHYSICAL REVIEW LETTERS (2023)

Article Physics, Particles & Fields

Dark baryon from pure Yang-Mills theory and its GW signature from cosmic strings

Masaki Yamada, Kazuya Yonekura

Summary: We propose a candidate for dark matter (DM) in the form of a baryonic glueball, which is a stable and naturally produced type of glueball in the SO(2N) pure Yang-Mills theory. This model offers characteristic gravitational wave signals for testing and can explain both the abundance of DM and the recently detected gravitational wave signals.

JOURNAL OF HIGH ENERGY PHYSICS (2023)

Article Astronomy & Astrophysics

Cosmic strings from pure Yang-Mills theory

Masaki Yamada, Kazuya Yonekura

Summary: This study discusses the formation of cosmic strings or macroscopic color flux tubes in the phase transition from the deconfinement to confinement phase in pure Yang-Mills theory. The holographic dual descriptions suggest that the cosmic strings are related to fundamental strings or wrapped D-branes in gravity side, with reconnection probability being suppressed. The study shows that the pure YM theory provides a simple realization of cosmic F-and D-strings.

PHYSICAL REVIEW D (2022)

暂无数据