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Astrophysics > Cosmology and Nongalactic Astrophysics

arXiv:1608.00932v2 (astro-ph)
[Submitted on 2 Aug 2016 (v1) , last revised 15 Nov 2016 (this version, v2)]

Title: Smooth magnetogenesis

Title: 平滑磁生成

Authors:L. Campanelli, A. Marrone
Abstract: In the Ratra scenario of inflationary magnetogenesis, the kinematic coupling between the photon and the inflaton undergoes a nonanalytical jump at the end of inflation. Using smooth interpolating analytical forms of the coupling function, we show that such unphysical jump does not invalidate the main prediction of the model, which still represents a viable mechanism for explaining cosmic magnetization. Nevertheless, there is a spurious result associated with the nonanaliticity of the coupling, to wit, the prediction that the spectrum of created photons has a power-law decay in the ultraviolet regime. This issue is discussed using both semiclassical approximation and smooth coupling functions.
Abstract: 在Ratra暴胀磁化情景中,光子与暴胀子之间的运动学耦合在暴胀结束时会发生非解析跳跃。通过使用耦合函数的平滑插值解析形式,我们表明这种非物理跳跃并不会使模型的主要预测失效,该模型仍然代表了一种可行的宇宙磁化机制。然而,由于耦合的非解析性,确实存在一个虚假的结果,即所预测的产生的光子谱在紫外区域具有幂律衰减。这一问题使用半经典近似和光滑耦合函数进行了讨论。
Comments: 9 pages, 5 figures, typos corrected, references updated, version matching the published one
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO) ; General Relativity and Quantum Cosmology (gr-qc)
Cite as: arXiv:1608.00932 [astro-ph.CO]
  (or arXiv:1608.00932v2 [astro-ph.CO] for this version)
  https://doi.org/10.48550/arXiv.1608.00932
arXiv-issued DOI via DataCite
Journal reference: Phys. Rev. D 94, 103510 (2016)
Related DOI: https://doi.org/10.1103/PhysRevD.94.103510
DOI(s) linking to related resources

Submission history

From: Leonardo Campanelli [view email]
[v1] Tue, 2 Aug 2016 18:58:21 UTC (398 KB)
[v2] Tue, 15 Nov 2016 19:07:20 UTC (399 KB)
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