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相关论文: On Constraining Electroweak-Baryogenesis with Inho…

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We study electroweak baryogenesis driven by the top quark in two Higgs doublet model that allows flavor-changing neutral Higgs couplings. Taking Higgs sector couplings and the additional top Yukawa coupling $\rho_{tt}$ to be…

高能物理 - 唯象学 · 物理学 2017-09-06 George W. -S. Hou

To elucidate the significance of the effect of systematic uncertainties in light element abundance estimates on cosmological bounds derivable from Big Bang Nucleosynthesis (BBN) we present tables giving bounds on $\Omega_{baryon}$ and…

天体物理学 · 物理学 2009-10-22 Lawrence M. Krauss , Peter J. Kernan

We propose a new electroweak baryogenesis scenario in high-scale supersymmetric (SUSY) models. We consider a singlet extension of the minimal SUSY standard model introducing additional vector-like multiplets. We show that the strongly…

高能物理 - 唯象学 · 物理学 2015-03-05 Kazuya Ishikawa , Teppei Kitahara , Masahiro Takimoto

The origin of the matter-antimatter asymmetry of the universe remains one of the outstanding questions yet to be answered by modern cosmology and also one of only a handful of problems where the need of a larger number of degrees of freedom…

高能物理 - 唯象学 · 物理学 2017-08-23 Gabriella Piccinelli , Alejandro Ayala

We review the current status of baryogenesis with emphasis on electroweak baryogenesis and leptogenesis. The first detailed studies were carried out for SU(5) GUT models where CP-violating decays of leptoquarks generate a baryon asymmetry.…

高能物理 - 唯象学 · 物理学 2021-11-09 Dietrich Bodeker , Wilfried Buchmuller

We discuss the constraints on the Higgs sector coming from the requirement of the generation of the matter-antimatter asymmetry at the electroweak phase transition. These relate to both a strongly first order first transition, necessary for…

高能物理 - 唯象学 · 物理学 2023-11-14 Carlos E. M. Wagner

We re-examine the generation of the baryon asymmetry in the minimal supersymmetric standard model (MSSM) during the electroweak phase transition. We find that the dominant source for baryogenesis arises from the chargino sector. The…

高能物理 - 唯象学 · 物理学 2009-10-31 James M. Cline , Michael Joyce , Kimmo Kainulainen

For a brief time in its early evolution the Universe was a cosmic nuclear reactor. The expansion and cooling of the Universe limited this epoch to the first few minutes, allowing time for the synthesis in astrophysically interesting…

宇宙学与河外天体物理 · 物理学 2010-09-27 Gary Steigman

It has recently been suggested that the baryon washout problem of standard electroweak baryogenesis could be avoided if inflation ends at a low enough energy density and a parametric resonance transfers its energy repidly into the standard…

高能物理 - 唯象学 · 物理学 2007-05-23 A. Rajantie , P. M. Saffin , E. J. Copeland

Using the semi-analytic method proposed by \citet{Esma91} we calculate the abundances of the light elements produced during primordial nucleosynthesis assuming that the gauge coupling constants of the fundamental interactions may vary. We…

天体物理学 · 物理学 2008-11-26 Susana J. Landau , Mercedes E. Mosquera , Hector Vucetich

I describe work done in collaboration with M. Joyce and K. Kainulainen on (1) the strength of the electroweak phase transition in the MSSM and (2) the mechanism for producing the baryon asymmetry during the phase transition. In the former…

高能物理 - 唯象学 · 物理学 2016-10-26 J. M. Cline

Cosmic microwave background (CMB) determinations of the baryon-to-photon ratio $\eta \propto \Omega_{\rm baryon} h^2$ will remove the last free parameter from (standard) big bang nucleosynthesis (BBN) calculations. This will make BBN a much…

天体物理学 · 物理学 2008-11-26 Richard H. Cyburt , Brian D. Fields , Keith A. Olive

In the standard model and most of its extensions the electroweak transition is too weak to affect the cosmological baryon asymmetry. Due to sphaleron processes baryogenesis in the high-temperature, symmetric phase of the standard model is…

高能物理 - 唯象学 · 物理学 2007-05-23 W. Buchmüller

We propose a novel cosmological scenario in which baryonic neutron stars could plausibly form in the early universe. If baryogenesis initially produces an excessively-large baryon asymmetry, $Y_B \gg 10^{-10},$ the baryonic mass inside the…

宇宙学与河外天体物理 · 物理学 2026-04-13 Gordan Krnjaic , Duncan Rocha , Huangyu Xiao

We have modified the standard code for primordial nucleosynthesis to include the effect of the slight heating of neutrinos by $e^\pm$ annihilations. There is a small, systematic change in the $^4$He yield, $\Delta Y \simeq +1.5\times…

天体物理学 · 物理学 2009-10-22 B. Fields , S. Dodelson , M. S. Turner

We propose a novel mechanism for electroweak baryogenesis in which collapsing domain walls formed by an axion-like field replace the bubble walls in a strong first-order electroweak phase transition. The axion-like particle coupling to the…

高能物理 - 唯象学 · 物理学 2026-05-01 Yang Bai , Kun-Feng Lyu , Yue Zhao

In this study we examine post-inflationary cosmologies dominated by a scalar field with the equation of state: p_phi=w_phi rho_phi (0 leq w_phi leq 1) in order to facilitate baryogenesis at the electroweak scale. We take a more conventional…

高能物理 - 唯象学 · 物理学 2009-10-31 Tomislav Prokopec

We construct two anomaly-free supersymmetric $U(1)'$ models with a secluded $U(1)'$-breaking sector. For the one with $E_6$ embedding we show that there exists a strong enough first order electroweak phase transition for electroweak…

高能物理 - 唯象学 · 物理学 2011-04-28 Junhai Kang , Paul Langacker , Tianjun Li , Tao Liu

The mechanism of "cold electroweak baryogenesis" has been so far unpopular because its proposal has relied on the ad-hoc assumption of a period of hybrid inflation at the electroweak scale with the Higgs acting as the waterfall field. We…

高能物理 - 唯象学 · 物理学 2015-05-28 Thomas Konstandin , Geraldine Servant

We include correlations between elemental abundances in a Monte Carlo statistical analysis of BBN predictions, which, along with updated reaction rates and an improved BBN code, lead to tightened constraints on $\Omega_{B}$ and $N_{\nu}$.…

天体物理学 · 物理学 2009-10-22 Peter J. Kernan , Lawrence M. Krauss