Search results for "EINSTEIN"

showing 10 items of 246 documents

Einstein, Planck and Vera Rubin: Relevant Encounters Between the Cosmological and the Quantum Worlds

2021

In Cosmology and in Fundamental Physics there is a crucial question like: where the elusive substance that we call Dark Matter is hidden in the Universe and what is it made of? that, even after 40 years from the Vera Rubin seminal discovery [1] does not have a proper answer. Actually, the more we have investigated, the more this issue has become strongly entangled with aspects that go beyond the established Quantum Physics, the Standard Model of Elementary particles and the General Relativity and related to processes like the Inflation, the accelerated expansion of the Universe and High Energy Phenomena around compact objects. Even Quantum Gravity and very exotic Dark Matter particle candid…

High Energy Physics - TheoryGeneral Physics and AstronomyNature of dark matter01 natural sciencesGeneral Relativity and Quantum CosmologyCosmologyClassical vs quantum cosmologyHigh Energy Physics - Phenomenology (hep-ph)010303 astronomy & astrophysicsQuantumMathematical PhysicsQuantum gravity and cosmologyPhysicsModification of general relativityChaplygin Gaslcsh:QC1-999CosmologyHigh Energy Physics - PhenomenologyExpansion of the UniversesymbolsGeneral RelativityGeneral relativityMaterials Science (miscellaneous)BiophysicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Metric expansion of spacesymbols.namesakeTheory of relativitySettore FIS/05 - Astronomia e Astrofisica0103 physical sciencesDark matterddc:530Cosmological ModelsPhysical and Theoretical ChemistryPlanckEinsteindark matter; galaxies; nature of dark matter; beyond standard model; modification of general relativity; quantum gravity and cosmology; expansion of the Universe010308 nuclear & particles physicsFísicaGalaxiesAstrophysics - Astrophysics of GalaxiesCosmosEpistemologyHigh Energy Physics - Theory (hep-th)quantum gravityAstrophysics of Galaxies (astro-ph.GA)Quantum gravityBeyond standard modellcsh:Physics
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Do we Observe Quantum Gravity Effects at Galactic Scales?

2005

The nonperturbative renormalization group flow of Quantum Einstein Gravity (QEG) is reviewed. It is argued that there could be strong renormalization effects at large distances, in particular a scale dependent Newton constant, which mimic the presence of dark matter at galactic and cosmological scales.

High Energy Physics - TheoryGravity (chemistry)High Energy Physics::LatticeDark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsGeneral Relativity and Quantum CosmologyRenormalizationsymbols.namesakeGeneral Relativity and Quantum CosmologyEinsteinQuantumPhysicsAstrophysics (astro-ph)General EngineeringAstronomy and AstrophysicsHigh Energy Physics - Theory (hep-th)Space and Planetary ScienceQuantum electrodynamicsScale dependentsymbolsQuantum gravityConstant (mathematics)
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Lensing and dynamics of ultracompact bosonic stars

2017

Spherically symmetric bosonic stars are one of the few examples of gravitating solitons that are known to form dynamically, via a classical process of (incomplete) gravitational collapse. As stationary solutions of the Einstein--Klein-Gordon or the Einstein--Proca theory, bosonic stars may also become sufficiently compact to develop light rings and hence mimic, in principle, gravitational-wave observational signatures of black holes (BHs). In this paper, we discuss how these horizonless ultra-compact objects (UCOs) are actually distinct from BHs, both phenomenologically and dynamically. In the electromagnetic channel, the light ring associated phenomenology reveals remarkable lensing patter…

High Energy Physics - TheoryHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsEinstein ring010308 nuclear & particles physicsGravitational waveFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationGeneral Relativity and Quantum Cosmologysymbols.namesakeStarsHigh Energy Physics - Theory (hep-th)0103 physical sciencesGravitational collapsesymbolsSolitonAstrophysics - High Energy Astrophysical Phenomena010306 general physicsSchwarzschild radiusPhenomenology (particle physics)
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Infrared lessons for ultraviolet gravity: the case of massive gravity and Born-Infeld

2014

We generalize the ultraviolet sector of gravitation via a Born-Infeld action using lessons from massive gravity. The theory contains all of the elementary symmetric polynomials and is treated in the Palatini formalism. We show how the connection can be solved algebraically to be the Levi-Civita connection of an effective metric. The non-linearity of the algebraic equations yields several branches, one of which always reduces to General Relativity at low curvatures. We explore in detail a {\it minimal} version of the theory, for which we study solutions in the presence of a perfect fluid with special attention to the cosmological evolution. In vacuum we recover Ricci-flat solutions, but also…

High Energy Physics - TheoryModified gravityAlternatives to inflationCosmology and Nongalactic Astrophysics (astro-ph.CO)General relativityGravityFOS: Physical sciencesPerfect fluidddc:500.2General Relativity and Quantum Cosmology (gr-qc)Space (mathematics)01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationsymbols.namesakeTheoretical physicsGeneral Relativity and Quantum Cosmology0103 physical sciencesEinstein010306 general physicsPhysics010308 nuclear & particles physicsEquation of state (cosmology)Astronomy and AstrophysicsMassive gravityHigh Energy Physics - Theory (hep-th)symbolsGravitational singularityAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Cosmological Constant and Local Gravity

2010

We discuss the linearization of Einstein equations in the presence of a cosmological constant, by expanding the solution for the metric around a flat Minkowski space-time. We demonstrate that one can find consistent solutions to the linearized set of equations for the metric perturbations, in the Lorentz gauge, which are not spherically symmetric, but they rather exhibit a cylindrical symmetry. We find that the components of the gravitational field satisfying the appropriate Poisson equations have the property of ensuring that a scalar potential can be constructed, in which both contributions, from ordinary matter and Lambda > 0, are attractive. In addition, there is a novel tensor potentia…

High Energy Physics - TheoryNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)De Sitter spaceFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyDe Sitter universeLinearized gravity0103 physical sciencesMinkowski spaceSchwarzschild metric010303 astronomy & astrophysicsMathematical physicsPhysicsInhomogeneous cosmology010308 nuclear & particles physicsGeneral Relativity and CosmologyFísicaClassical mechanicsLorenz gauge conditionHigh Energy Physics - Theory (hep-th)Einstein field equationsAstrophysics - Cosmology and Nongalactic Astrophysics
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Transplanckian inflation as gravity echoes

2015

In this work, we show that, in the presence of non-minimal coupling to gravity, it is possible to generate sizeable tensor modes in single-field models without transplanckian field values. These transplanckian field values apparently needed in Einstein gravity to accommodate the experimental results may only be due to our insistence of imposing a minimal coupling of the inflaton field to gravity in a model with non-minimal couplings. We present three simple single-field models that prove that it is possible accommodate a large tensor-to-scalar ratio without requiring transplanckian field values within the slow-roll regime.

High Energy Physics - TheoryNuclear and High Energy PhysicsGravity (chemistry)Cosmology and Nongalactic Astrophysics (astro-ph.CO)Field (physics)FOS: Physical sciences01 natural sciencesGravitationTheoretical physicsGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesTensor010306 general physicsMinimal couplingPhysicsInflation (cosmology)010308 nuclear & particles physicsFísicaInflatonlcsh:QC1-999High Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Einstein field equationslcsh:PhysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Hawking radiation correlations in Bose-Einstein condensates using quantum field theory in curved space

2013

The density-density correlation function is computed for the Bogoliubov pseudoparticles created in a Bose-Einstein condensate undergoing a black hole flow. On the basis of the gravitational analogy, the method used relies only on quantum field theory in curved spacetime techniques. A comparison with the results obtained by ab initio full condensed matter calculations is given, confirming the validity of the approximation used, provided the profile of the flow varies smoothly on scales compared to the condensate healing length.

High Energy Physics - TheoryNuclear and High Energy PhysicsHAWKING RADIATION[PHYS.COND.GAS]Physics [physics]/Condensed Matter [cond-mat]/Quantum Gases [cond-mat.quant-gas]Black-hole evaporationFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesCONDENSATI DI BOSE EINSTEINGeneral Relativity and Quantum Cosmologylaw.inventionGravitationGeneral Relativity and Quantum CosmologyCorrelation functionlawQuantum mechanics0103 physical sciencesQuantum field theory010306 general physicsCurved spaceCondensed Matter::Quantum GasesPhysicsQuantum field theory in curved spacetime[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Condensed Matter::Other010308 nuclear & particles physicsBlack holeHigh Energy Physics - Theory (hep-th)Quantum Gases (cond-mat.quant-gas)[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Condensed Matter - Quantum GasesBose–Einstein condensateAnalog gravityHawking radiationPhysical Review D
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Relations for Einstein–Yang–Mills amplitudes from the CHY representation

2017

We show that a recently discovered relation, which expresses tree-level single trace Einstein-Yang-Mills amplitudes with one graviton and $(n-1)$ gauge bosons as a linear combination of pure Yang-Mills tree amplitudes with $n$ gauge bosons, can be derived from the CHY representation. In addition we show that there is a generalisation, which expresses tree-level single trace Einstein-Yang-Mills amplitudes with $r$ gravitons and $(n-r)$ gauge bosons as a linear combination of pure Yang-Mills tree amplitudes with $n$ gauge bosons. We present a general formula for this case.

High Energy Physics - TheoryNuclear and High Energy PhysicsTrace (linear algebra)High Energy Physics::LatticeFOS: Physical sciencesYang–Mills existence and mass gap01 natural sciencessymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryQuantum mechanics0103 physical sciencesEinstein010306 general physicsLinear combinationMathematical physicsPhysicsCondensed Matter::Quantum GasesIntroduction to gauge theoryGauge boson010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyGravitonlcsh:QC1-999High Energy Physics - Theory (hep-th)Supersymmetric gauge theorysymbolslcsh:PhysicsPhysics Letters B
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Palatini Approach to Modified Gravity: f(R) Theories and Beyond

2011

We review the recent literature on modified theories of gravity in the Palatini approach. After discussing the motivations that lead to consider alternatives to Einstein's theory and to treat the metric and the connection as independent objects, we review several topics that have been recently studied within this framework. In particular, we provide an in-depth analysis of the cosmic speedup problem, laboratory and solar systems tests, the structure of stellar objects, the Cauchy problem, and bouncing cosmologies. We also discuss the importance of going beyond the f(R) models to capture other phenomenological aspects related with dark matter/energy and quantum gravity.

High Energy Physics - TheoryPhysicsGravity (chemistry)Dark matterStructure (category theory)FOS: Physical sciencesAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyConnection (mathematics)High Energy Physics - Phenomenologysymbols.namesakeTheoretical physicsGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Space and Planetary ScienceMetric (mathematics)symbolsInitial value problemQuantum gravityEinsteinMathematical Physics
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On the Possibility of Quantum Gravity Effects at Astrophysical Scales

2007

The nonperturbative renormalization group flow of Quantum Einstein Gravity (QEG) is reviewed. It is argued that at large distances there could be strong renormalization effects, including a scale dependence of Newton's constant, which mimic the presence of dark matter at galactic and cosmological scales.

High Energy Physics - TheoryPhysicsGravity (chemistry)Scale (ratio)High Energy Physics::LatticeDark matterAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsGeneral Relativity and Quantum CosmologyRenormalizationTheoretical physicssymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Space and Planetary SciencesymbolsQuantum gravityEinsteinConstant (mathematics)QuantumMathematical Physics
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