Skip to main content
CenXiv.org
This website is in trial operation, support us!
We gratefully acknowledge support from all contributors.
Contribute
Donate
cenxiv logo > hep-ph > arXiv:1608.00583v3

Help | Advanced Search

High Energy Physics - Phenomenology

arXiv:1608.00583v3 (hep-ph)
[Submitted on 1 Aug 2016 (v1) , last revised 27 Oct 2016 (this version, v3)]

Title: Baryogenesis and Gravitational Waves from Runaway Bubble Collisions

Title: 重子生成与失控气泡碰撞产生的引力波

Authors:Andrey Katz, Antonio Riotto
Abstract: We propose a novel mechanism for production of baryonic asymmetry in the early Universe. The mechanism takes advantage of the strong first order phase transition that produces runaway bubbles in the hidden sector that propagate almost without friction with ultra-relativistic velocities. Collisions of such bubbles can non-thermally produce heavy particles that further decay out-of-equilibrium into the SM and produce the observed baryonic asymmetry. This process can proceed at the very low temperatures, providing a new mechanism of post-sphaleron baryogenesis. In this paper we present a fully calculable model which produces the baryonic asymmetry along these lines as well as evades all the existing cosmological constraints. We emphasize that the Gravitational Waves signal from the first order phase transition is completely generic and can potentially be detected by the future eLISA interferometer. We also discuss other potential signals, which are more model dependent, and point out the unresolved theoretical questions related to our proposal.
Abstract: 我们提出了一种在早期宇宙中产生重子不对称性的新机制。 该机制利用了产生逃逸气泡的强一阶相变,这些气泡在隐藏扇区中以几乎无摩擦的超相对论速度传播。 这种气泡的碰撞可以非热地产生重粒子,这些粒子随后在非平衡状态下衰变为标准模型,从而产生观测到的重子不对称性。 这一过程可以在非常低的温度下进行,提供了一种新的后 sphaleron 重子生成机制。 在本文中,我们提出了一种完全可计算的模型,沿着这些思路产生重子不对称性,并且避免了所有现有的宇宙学约束。 我们强调, 一阶相变产生的引力波信号是完全通用的,可能被未来的 eLISA 干涉仪检测到。 我们还讨论了其他潜在信号,这些信号更依赖于模型,并指出了与我们的提议相关的未解决理论问题。
Comments: 30 pages, 8 figures. v2: typos fixed and references added v3: discussion regarding the lifetime of the dark Z's fixed and the discussion on their relic abundance is removed, minor corrections, and references added. Conclusions are intact. Accepted to JCAP
Subjects: High Energy Physics - Phenomenology (hep-ph) ; Cosmology and Nongalactic Astrophysics (astro-ph.CO); General Relativity and Quantum Cosmology (gr-qc)
Cite as: arXiv:1608.00583 [hep-ph]
  (or arXiv:1608.00583v3 [hep-ph] for this version)
  https://doi.org/10.48550/arXiv.1608.00583
arXiv-issued DOI via DataCite
Journal reference: CERN-TH-2016-173
Related DOI: https://doi.org/10.1088/1475-7516/2016/11/011
DOI(s) linking to related resources

Submission history

From: Andrey Katz [view email]
[v1] Mon, 1 Aug 2016 20:00:06 UTC (2,816 KB)
[v2] Wed, 17 Aug 2016 21:15:09 UTC (2,817 KB)
[v3] Thu, 27 Oct 2016 10:32:32 UTC (2,480 KB)
Full-text links:

Access Paper:

    View a PDF of the paper titled
  • View Chinese PDF
  • View PDF
  • TeX Source
view license
Current browse context:
hep-ph
< prev   |   next >
new | recent | 2016-08
Change to browse by:
astro-ph
astro-ph.CO
gr-qc

References & Citations

  • NASA ADS
  • Google Scholar
  • Semantic Scholar
a export BibTeX citation Loading...

BibTeX formatted citation

×
Data provided by:

Bookmark

BibSonomy logo Reddit logo

Bibliographic and Citation Tools

Bibliographic Explorer (What is the Explorer?)
Connected Papers (What is Connected Papers?)
Litmaps (What is Litmaps?)
scite Smart Citations (What are Smart Citations?)

Code, Data and Media Associated with this Article

alphaXiv (What is alphaXiv?)
CatalyzeX Code Finder for Papers (What is CatalyzeX?)
DagsHub (What is DagsHub?)
Gotit.pub (What is GotitPub?)
Hugging Face (What is Huggingface?)
Papers with Code (What is Papers with Code?)
ScienceCast (What is ScienceCast?)

Demos

Replicate (What is Replicate?)
Hugging Face Spaces (What is Spaces?)
TXYZ.AI (What is TXYZ.AI?)

Recommenders and Search Tools

Influence Flower (What are Influence Flowers?)
CORE Recommender (What is CORE?)
IArxiv Recommender (What is IArxiv?)
  • Author
  • Venue
  • Institution
  • Topic

arXivLabs: experimental projects with community collaborators

arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website.

Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them.

Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs.

Which authors of this paper are endorsers? | Disable MathJax (What is MathJax?)
  • About
  • Help
  • contact arXivClick here to contact arXiv Contact
  • subscribe to arXiv mailingsClick here to subscribe Subscribe
  • Copyright
  • Privacy Policy
  • Web Accessibility Assistance
  • arXiv Operational Status
    Get status notifications via email or slack

京ICP备2025123034号