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Gravity and general relativity are considered as an Effective Field Theory at low energies and macroscopic distances. The effective action of the conformal anomaly of light or massless quantum fields has significant effects on macroscopic…

高能物理 - 理论 · 物理学 2023-02-20 Emil Mottola

We discuss the evolution of linear perturbations about a Friedmann-Robertson-Walker background metric, using only the local conservation of energy-momentum. We show that on sufficiently large scales the curvature perturbation on spatial…

天体物理学 · 物理学 2009-10-31 David Wands , Karim A. Malik , David H. Lyth , Andrew R. Liddle

In [arXiv:1004.2488], Baumann et al. present a new formalism for studying cosmological systems where the characteristic scale of non-linearities is much smaller than the Hubble scale. By integrating out the short-wavelength modes, it is…

宇宙学与河外天体物理 · 物理学 2010-09-08 Hyeyoun Chung

We derive the general relativistic linear tidal response of a neutron star modeled as a barotropic perfect fluid. From the covariant fluid effective action, we linearize about equilibrium and obtain the action for fluid displacements…

广义相对论与量子宇宙学 · 物理学 2026-02-10 Irvin Martínez-Rodríguez

Recently we showed that in FLRW cosmology, the contribution from higher curvature terms in any generic metric gravity theory to the energy-momentum tensor is of the perfect fluid form. Such a geometric perfect fluid can be interpreted as a…

广义相对论与量子宇宙学 · 物理学 2024-08-07 Metin Gürses , Yaghoub Heydarzade , Çetin Şentürk

We construct the effective field theory of a perfect fluid in the early universe. Focusing on the case where the fluid has the equation of state of radiation, we show that it may lead to corrections to the background dynamics that can…

宇宙学与河外天体物理 · 物理学 2015-06-22 Bruno Balthazar , Pedro G. Ferreira

We study the cosmological perturbations of the recently proposed extension of non-linear massive gravity with a scalar field. The added scalar field ensures a new symmetry on the field space of the theory. The theory has the property of…

广义相对论与量子宇宙学 · 物理学 2013-07-12 Zahra Haghani , Hamid Reza Sepangi , Shahab Shahidi

A phenomenological model of an ideal fluid with a scalar charge is formulated, on the basis of which a model with a neutral fluid and a vacuum-field model with rules of transition between them are constructed. A qualitative analysis of the…

广义相对论与量子宇宙学 · 物理学 2025-04-21 Yu. G. Ignat'ev

We develop the effective field theory approach to torsional modified gravities, a formalism that allows for the systematic investigation of the background and perturbation levels separately. Starting from the usual effective field theory…

广义相对论与量子宇宙学 · 物理学 2018-10-03 Chunlong Li , Yong Cai , Yi-Fu Cai , Emmanuel N. Saridakis

We set the foundation and formulate the Perfect (Ideal) Hyperfluid. The latter represents the natural generalization of the usual perfect fluid structure where now the microscopic characteristics of matter (spin, shear, dilation) are also…

广义相对论与量子宇宙学 · 物理学 2021-05-05 Damianos Iosifidis

n scalar-tensor theories of gravity with torsion, the gravitational field is described in terms of a symmetric metric tensor $g$, a metric-compatible connection $\nabla$ with torsion, and a scalar field $\phi$. The main aim is to explore an…

广义相对论与量子宇宙学 · 物理学 2016-11-15 Chih-Hung Wang

We consider a free massless scalar field coupled to an infinite tower of background higher-spin gauge fields via minimal coupling to the traceless conserved currents. The set of Abelian gauge transformations is deformed to the non-Abelian…

高能物理 - 理论 · 物理学 2011-02-22 Xavier Bekaert , Euihun Joung , Jihad Mourad

We study the evolution of an anisotropic shear-free fluid with heat flux and kinematic self-similarity of the second kind. We found a class of solution to the Einstein field equations by assuming that the part of the tangential pressure…

广义相对论与量子宇宙学 · 物理学 2014-05-13 R. Chan , M. F. A. da Silva , C. F. C. Brandt

We compute the third order gauge invariant action for scalar-graviton interactions in the Jordan frame. We demonstrate that the gauge invariant action for scalar and tensor perturbations on one physical hypersurface only differs from that…

广义相对论与量子宇宙学 · 物理学 2015-06-15 Tomislav Prokopec , Jan Weenink

The late time evolution of Friedmann-Robertson-Walker (FRW) models with a perfect fluid matter source is studied in the conformal frame of $f(R) $ gravity. We assume that the corresponding scalar field, nonminimally coupled to matter, has…

广义相对论与量子宇宙学 · 物理学 2014-11-20 John Miritzis , Roberto Giambò

Mathematical modeling of gravitating configurations of physical fields is one of the priority directions of the modern theory of gravity. Most of the exact solutions constructed within the framework of the general relativity are static or…

广义相对论与量子宇宙学 · 物理学 2019-12-03 Ju V Tchemarina , E G Alekseeva , A N Tsirulev , N K Nuraliev

We investigate the relativistic effective field theory (EFT) describing a non-dissipative gravitating continuum. In addition to ordinary continua, namely solids and fluids, we find an extraordinary more symmetric continuum, aether. In…

高能物理 - 理论 · 物理学 2022-09-07 Katsuki Aoki , Mohammad Ali Gorji , Shinji Mukohyama , Kazufumi Takahashi

It has recently been shown that specific non-perturbative effects may lead to an explosive decay of flat direction condensates in supersymmetric theories. We confirm explicitly the efficiency of this process with lattice simulations: after…

宇宙学与河外天体物理 · 物理学 2009-09-02 Jean-Francois Dufaux

We propose a nonlocal scalar-tensor model of gravity with pseudodifferential operators inspired by the effective action of p-adic string and string field theory on flat spacetime. An infinite number of derivatives act both on the metric and…

高能物理 - 理论 · 物理学 2010-12-28 Gianluca Calcagni , Giuseppe Nardelli

In this letter we review the separate universe approach for cosmological perturbations and point out that it is essentially the lowest order approximation to a gradient expansion. Using this approach, one can study the nonlinear evolution…

天体物理学 · 物理学 2009-11-10 G. I. Rigopoulos , E. P. S. Shellard