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$ $In this paper we present a systematic treatment for fundamental renormalization of quantum electrodynamics in real space. Although the standard renormalization is an old school problem in this case, it has not yet been completely done in…

高能物理 - 理论 · 物理学 2021-02-18 Amirhosein Mojavezi , Reza Moazzemi , Mohammad Ebrahim Zomorrodian

We examine the renormalization of an effective theory description of a general initial state set in an isotropically expanding space-time, which is done to understand how to include the effects of new physics in the calculation of the…

高能物理 - 理论 · 物理学 2007-05-23 Hael Collins , R. Holman

The particle production process is reviewed, through which cosmic inflation can produce a scale invariant superhorizon spectrum of perturbations of suitable fields starting from their quantum fluctuations. Afterwards, in the context of the…

宇宙学与河外天体物理 · 物理学 2011-03-28 Konstantinos Dimopoulos

A quantum scalar field theory with spacetime-dependent coupling is studied. Surprisingly, while translation invariance is explicitly broken in the classical theory, momentum conservation is recovered at the quantum level for some specific…

高能物理 - 理论 · 物理学 2014-01-29 Gianluca Calcagni , Giuseppe Nardelli

We show that a pair of field theory monodromies in which the shift symmetry is broken by small, well motivated deformations, naturally incorporates a mechanism for cancelling off radiative corrections to the cosmological constant. The…

高能物理 - 理论 · 物理学 2019-02-20 Antonio Padilla

We consider general relativity with a cosmological constant as a perturbative expansion around a completely solvable diffeomorphism invariant field theory. This theory is the $\Lambda\to\infty$ limit of general relativity. This allows an…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Rodolfo Gambini , Jorge Pullin

Recently, we presented a unified way of analysing classical cosmological perturbation in generalized gravity theories. In this paper, we derive the perturbation spectrums generated from quantum fluctuations again in unified forms. We…

广义相对论与量子宇宙学 · 物理学 2014-11-17 J. Hwang

We consider a massive scalar field living on the recently found exact quantum space-time corresponding to vacuum spherically symmetric loop quantum gravity. The discreteness of the quantum space time naturally regularizes the scalar field,…

广义相对论与量子宇宙学 · 物理学 2015-12-16 Nahuel Barrios , Rodolfo Gambini , Jorge Pullin

A generalized scalar-tensor theory is investigated whose cosmological term depends on both a scalar field and its time derivative. A correspondence with solutions of five-dimensional Space-Time-Matter theory is noted. Analytic solutions are…

广义相对论与量子宇宙学 · 物理学 2009-11-07 T. Fukui , J. M. Overduin

We discuss the additional perturbation introduced during inflation by quantum stress tensor fluctuations of a conformally invariant field such as the photon. We consider both a kinematical model, which deals only with the expansion…

广义相对论与量子宇宙学 · 物理学 2011-08-15 L. H. Ford , S. P. Miao , Kin-Wang Ng , R. P. Woodard , Chun-Hsien Wu

After introducing gauge-invariant cosmological perturbation theory we give an improved set of governing equations for multiple fluids including energy transfer. Having defined adiabatic and entropic perturbations we derive the…

天体物理学 · 物理学 2007-05-23 Karim A. Malik

In the standard inflationary paradigm the inhomogeneities observed in the CMB arise from quantum fluctuations of an initially homogeneous and isotropic vacuum state. This picture suffers from two well-known weaknesses. First, it assumes…

广义相对论与量子宇宙学 · 物理学 2026-01-21 Gabriel R. Bengochea , Gabriel Leon , Alejandro Perez

I discuss the possibility of using classical field theory to approximate hot, real-time quantum field theory. I calculate, in a scalar theory, the classical two point and four point function in perturbation theory. The counterterms needed…

高能物理 - 唯象学 · 物理学 2007-05-23 Gert Aarts

Superstring theory, models with extra dimensions and other SUSY models generically predict that the coupling constants are in fact vacuum expectation values of fields like the dilaton, moduli etc. Assuming some of these fields are light…

天体物理学 · 物理学 2007-05-23 Lev Kofman

We compute the spectral distribution of the quantum fluctuations of the vacuum, amplified by inflation, after an arbitrary number of background transitions. Using a graphic representation of the process we find that the final spectrum can…

广义相对论与量子宇宙学 · 物理学 2009-11-07 G. De Risi , M. Gasperini

The predictive power of cosmic inflation hinges on the existence of a conserved quantity at very large scales, called the primordial curvature perturbation, which is therefore insensitive to the details of reheating and the physics of the…

宇宙学与河外天体物理 · 物理学 2026-03-11 Matteo Braglia , Lucas Pinol

We consider the linear perturbations for the single scalar field inflation model interacting with an additional triad of scalar fields. The background solutions of the three additional scalar fields depend on spatial coordinates with a…

广义相对论与量子宇宙学 · 物理学 2013-09-04 Seoktae Koh , Seyen Kouwn , O-Kab Kwon , Phillial Oh

A short pedagogical overview of cosmological perturbation theory, following the lectures given during the brazilian school of cosmology held in August 2012. Topics treated are: I. The background II. SVT decomposition and the gauge issue.…

宇宙学与河外天体物理 · 物理学 2013-03-15 Patrick Peter

I give a review of the conceptual issues that arise in theories of quantum cosmology. I start by emphasising some features of ordinary quantum theory that also play a crucial role in understanding quantum cosmology. I then give motivations…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Claus Kiefer

Quantum cosmology is traditionally formulated in a minisuperspace setting, implicitly averaging fields over space to obtain homogeneous models. For universal reasons related to the uncertainty principle, quantum corrections then depend on…

广义相对论与量子宇宙学 · 物理学 2019-06-05 Martin Bojowald