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相关论文: Photon mass from inflation

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We argue that the dynamics of photons canonically coupled to scalars in de Sitter inflation gets modified by a photon mass term. This might have lead to generation of potentially observable magnetic field correlated over cosmological scales…

天体物理学 · 物理学 2017-08-23 Tomislav Prokopec

We calculate the one-loop vacuum polarization tensor of scalar electrodynamics in a locally de Sitter space-time, endowed with a nearly minimally coupled, light scalar field. We show that the photon dynamics is well approximated by a…

天体物理学 · 物理学 2009-11-10 Tomislav Prokopec , Ewald Puchwein

We give a pedagogical review of a mechanism through which long wave length photons can become massive during inflation. Our account begins with a discussion of the period of exponentially rapid expansion known as inflation. We next describe…

天体物理学 · 物理学 2009-11-07 T. Prokopec , R. P. Woodard

We stochastically formulate the theory of scalar quantum electrodynamics on a de Sitter background. This reproduces the leading infrared logarithms at each loop order. It also allows one to sum the series of leading infrared logarithms to…

广义相对论与量子宇宙学 · 物理学 2008-11-26 T. Prokopec , N. C. Tsamis , R. P. Woodard

We propose a new mechanism for magnetic field generation from inflation, by which strong magnetic fields can be generated on cosmological scales. These fields may be observable by cosmic microwave background radition measurements, and may…

天体物理学 · 物理学 2009-11-10 Tomislav Prokopec , Ewald Puchwein

We use a recent result for the graviton contribution to the one loop vacuum polarization to solve the effective field equations for dynamical photons on de Sitter background. Our results show that the electric field experiences a secular…

广义相对论与量子宇宙学 · 物理学 2015-06-22 C. L. Wang , R. P. Woodard

We consider cosmological inflation generated by a scalar field slowly rolling off from a de Sitter maximum of its potential. The models belong to the class of hilltop models and represent the most general model of this kind in which the…

广义相对论与量子宇宙学 · 物理学 2016-09-05 Mariano Cadoni , Edgardo Franzin , Salvatore Mignemi

The representation theory of de Sitter space allows for a category of partially massless particles which have no flat space analog, but could have existed during inflation. We study the couplings of these exotic particles to inflationary…

高能物理 - 理论 · 物理学 2018-05-23 Daniel Baumann , Garrett Goon , Hayden Lee , Guilherme L. Pimentel

We study asymptotic dynamics of photons propagating in the polarized vacuum of a locally de Sitter Universe. The origin of the vacuum polarization is fluctuations of a massless, minimally coupled, scalar, which we model by the one-loop…

广义相对论与量子宇宙学 · 物理学 2015-06-25 Tomislav Prokopec , Richard P. Woodard

We show that an inflationary background might be realized by using any p-form non-minimally coupled to gravity. Standard scalar field inflation corresponds to the 0-form case and vector inflation to the 1-form. Moreover, we show that the 2-…

宇宙学与河外天体物理 · 物理学 2009-11-13 Cristiano Germani , Alex Kehagias

The large-scale magnetic fields we observe today in galaxies and galaxy clusters could be the result of a pure quantum effect taking place during inflation, to wit, the creation of particles (photons) out from the vacuum in a curved…

宇宙学与河外天体物理 · 物理学 2016-08-26 Leonardo Campanelli

We study constant classical electric fields and the Schwinger effect in de Sitter space, with potential implications for magnetogenesis and inflationary dark matter production. Treating the photon as a dynamical field, we show that…

高能物理 - 唯象学 · 物理学 2026-04-20 Mar Bastero-Gil , Paulo B. Ferraz , António Torres Manso , Lorenzo Ubaldi , Roberto Vega-Morales

We consider models in which the (transverse) photon mass is non-zero during inflation and drops to zero non-adiabatically at the end of inflation. Through this process, vacuum fluctuations of the photon field are converted into physical,…

天体物理学 · 物理学 2009-10-31 Ola Tornkvist , Anne-Christine Davis , Konstantinos Dimopoulos , Tomislav Prokopec

We revisit the efficiency of Schwinger mechanism in creating charged pairs during inflation. We consider a minimal setup of inflation in which the inflaton field is a complex scalar field charged under a $U(1)$ gauge field. There is a time…

高能物理 - 理论 · 物理学 2019-05-29 Soroush Shakeri , Mohammad Ali Gorji , Hassan Firouzjahi

We derive the semiclassical evolution of massless minimally coupled scalar matter in the de Sitter space-time from the Born-Oppenheimer reduction of the Wheeler-DeWitt equation. We show that the dynamics of trans-Planckian modes can be cast…

高能物理 - 理论 · 物理学 2009-11-11 Gian Luigi Alberghi , Roberto Casadio , Alessandro Tronconi

We consider a polymer quantization of a free massless scalar field in a homogeneous and isotropic cosmological spacetime. This quantization method assumes that field translations are fundamentally discrete, and is related to but distinct…

宇宙学与河外天体物理 · 物理学 2010-01-27 Golam Mortuza Hossain , Viqar Husain , Sanjeev S. Seahra

We propose a novel scenario in which scalar perturbations, that seed the large scale structure of the Universe, are generated without relying on a scalar field (the inflaton). In this framework, inflation is driven by a de Sitter space-time…

宇宙学与河外天体物理 · 物理学 2024-12-20 Daniele Bertacca , Raul Jimenez , Sabino Matarrese , Angelo Ricciardone

We study classical background electric fields and the Schwinger effect in de Sitter space. We show that having a constant electric field in de Sitter requires the photon to have a tachyonic mass proportional to the Hubble scale. This has…

高能物理 - 唯象学 · 物理学 2025-03-05 Mar Bastero-Gil , Paulo B. Ferraz , António Torres Manso , Lorenzo Ubaldi , Roberto Vega-Morales

Some form of approximately exponential inflation is generally assumed to be the origin of our present universe. The inflation is thought to be driven by a scalar field potential where the field first slowly slides along the potential and…

广义相对论与量子宇宙学 · 物理学 2023-04-27 Gustaf Rydbeck

We describe a simple and efficient mechanism by which very heavy particles are copiously created from a primordial inflationary epoch. It works for scalar fields which are massless or very light during inflation and acquire a large mass…

高能物理 - 唯象学 · 物理学 2010-04-05 G. F. Giudice , A. Riotto , A. Zaffaroni
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