Search results for " Cosmology"

showing 10 items of 1486 documents

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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Born-Infeld f(R) gravity

2014

Motivated by the properties of matter quantum fields in curved space-times, we work out a gravity theory that combines the Born-Infeld gravity Lagrangian with an $f(R)$ piece. To avoid ghost-like instabilities, the theory is formulated within the Palatini approach. This construction provides more freedom to address a number of important questions such as the dynamics of the early universe and the cosmic accelerated expansion, among others. In particular, we consider the effect that adding an $f(R)=a R^2$ term has on the early-time cosmology. We find that bouncing solutions are robust against these modifications of the Lagrangian whereas the solutions with {\it loitering} behavior of the ori…

High Energy Physics - TheoryNuclear and High Energy PhysicsGravity (chemistry)Cosmology and Nongalactic Astrophysics (astro-ph.CO)Борна-Инфельда теория гравитации модифицированнаяmedia_common.quotation_subjectFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyCosmologyкосмологияGeneral Relativity and Quantum CosmologyTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)De Sitter universeBorn–Infeld modelmedia_commonPhysicsквантовая гравитацияFunction (mathematics)UniverseHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Quantum gravityf(R) gravityF(R)-гравитацияквантовые поляAstrophysics - Cosmology and Nongalactic Astrophysics
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Modular fluxes, elliptic genera, and weak gravity conjectures in four dimensions

2019

We analyse the Weak Gravity Conjecture for chiral four-dimensional F-theory compactifications with N=1 supersymmetry. Extending our previous work on nearly tensionless heterotic strings in six dimensions, we show that under certain assumptions a tower of asymptotically massless states arises in the limit of vanishing coupling of a U(1) gauge symmetry coupled to gravity. This tower contains super-extremal states whose charge-to-mass ratios are larger than those of certain extremal dilatonic Reissner-Nordstrom black holes, precisely as required by the Weak Gravity Conjecture. Unlike in six dimensions, the tower of super-extremal states does not always populate a charge sub-lattice. The main t…

High Energy Physics - TheoryNuclear and High Energy PhysicsGravity (chemistry)FOS: Physical sciencesF-TheoryTopological Strings01 natural sciencesTheoretical physicsGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheorySuperstrings and Heterotic Strings0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsGauge symmetryPhysicsHeterotic string theory010308 nuclear & particles physicshep-thCharge (physics)SupersymmetryF-theoryHigh Energy Physics - Theory (hep-th)lcsh:QC770-798String DualityMirror symmetryParticle Physics - TheoryString dualityJournal of High Energy Physics
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Stability analysis of black holes in massive gravity: a unified treatment

2014

We consider the analytic solutions of massive (bi)gravity which can be written in a simple form using advanced Eddington-Finkelstein coordinates. We analyse the stability of these solutions against radial perturbations. First we recover the previously obtained result on the instability of the bidiagonal bi-Schwarzschild solutions. In the non-bidiagonal case (which contains, in particular, the Schwarzschild solution with Minkowski fiducial metric) we show that generically there are physical spherically symmetric perturbations, but no unstable modes.

High Energy Physics - TheoryNuclear and High Energy PhysicsGravity (chemistry)Kerr metricFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesInstabilityGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmology0103 physical sciencesMinkowski spaceSchwarzschild metric010306 general physicsComputingMilieux_MISCELLANEOUSPhysics[PHYS.GRQC] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Massive gravityClassical mechanicsHigh Energy Physics - Theory (hep-th)Reissner–Nordström metric[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Deriving the Schwarzschild solution[PHYS.HTHE] Physics [physics]/High Energy Physics - Theory [hep-th]
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An alternative scenario for critical scalar field collapse in $AdS_3$

2016

In the context of gravitational collapse and black hole formation, we reconsider the problem to describe analytically the critical collapse of a massless and minimally coupled scalar field in $2+1$ gravity.

High Energy Physics - TheoryNuclear and High Energy PhysicsGravity (chemistry)Particle physicsBlack HolesCritical phenomenaAstrophysics::High Energy Astrophysical PhenomenaCollapse (topology)FOS: Physical sciencesContext (language use)Critical collapseGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyTheoretical physicsHigh Energy Physics::TheoryGeneral Relativity and Quantum Cosmology0103 physical sciencesGravitational collapse010306 general physicsComputingMilieux_MISCELLANEOUSPhysics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]010308 nuclear & particles physicsMassless particle2+1 gravityHigh Energy Physics - Theory (hep-th)Anti-de Sitter spaceScalar field
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Hawking radiation of massive modes and undulations

2012

We compute the analogue Hawking radiation for modes which posses a small wave vector perpendicular to the horizon. For low frequencies, the resulting mass term induces a total reflection. This generates an extra mode mixing that occurs in the supersonic region, which cancels out the infrared divergence of the near horizon spectrum. As a result, the amplitude of the undulation (0-frequency wave with macroscopic amplitude) emitted in white hole flows now saturates at the linear level, unlike what was recently found in the massless case. In addition, we point out that the mass introduces a new type of undulation which is produced in black hole flows, and which is well described in the hydrodyn…

High Energy Physics - TheoryNuclear and High Energy PhysicsHAWKING RADIATIONWhite holeFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyMicro black holeGeneral Relativity and Quantum CosmologyQuantum mechanics0103 physical sciencesExtremal black holeWave vectormassive modes010306 general physicsPhysics010308 nuclear & particles physicsBlack holeInfrared divergenceHigh Energy Physics - Theory (hep-th)Quantum Gases (cond-mat.quant-gas)Quantum electrodynamicsReflection (physics)[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Condensed Matter - Quantum GasesHawking radiation
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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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Limits on neutrino Lorentz violation from multimessenger observations of TXS 0506+056

2019

The observation by the IceCube Collaboration of a high-energy ($E \gtrsim 200$ TeV) neutrino from the direction of the blazar TXS 0506+056 and the coincident observations of enhanced $\gamma$-ray emissions from the same object by MAGIC and other experiments can be used to set stringent constraints on Lorentz violation in the propagation of neutrinos that is linear in the neutrino energy: $\Delta v = - E/M_1$, where $\Delta v$ is the deviation from the velocity of light, and $M_1$ is an unknown high energy scale to be constrained by experiment. Allowing for a difference in neutrino and photon propagation times of $\sim 10$ days, we find that $M_1 \gtrsim 3 \times 10^{16}$ GeV. This improves …

High Energy Physics - TheoryNuclear and High Energy PhysicsHigh energyParticle physicsAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)Lorentz transformationgr-qcAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesComputer Science::Digital LibrariesGeneral Relativity and Quantum CosmologyIceCubesymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Coincident0103 physical sciences010306 general physicsBlazarParticle Physics - PhenomenologyHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEMultimessenger010308 nuclear & particles physicsGeneral Relativity and Cosmologyhep-thHigh Energy Physics::PhenomenologyLorentz violationGamma rayhep-phlcsh:QC1-999High Energy Physics - PhenomenologyPhoton propagationHigh Energy Physics - Theory (hep-th)Astrophysical neutrinosVelocity of lightsymbolsastro-ph.COHigh Energy Physics::ExperimentNeutrinoTXS 0506+056Astrophysics - High Energy Astrophysical PhenomenaParticle Physics - Theorylcsh:PhysicsBlazarsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysics Letters
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The quantum clock: a critical discussion on space-time

2016

We critically discuss the measure of very short time intervals. By means of a Gedankenexperiment, we describe an ideal clock based on the occurrence of completely random events. Many previous thought experiments have suggested fundamental Planck-scale limits on measurements of distance and time. Here we present a new type of thought experiment, based on a different type of clock, that provide further support for the existence of such limits. We show that the minimum time interval $\Delta t$ that this clock can measure scales as the inverse of its size $\Delta r$. This implies an uncertainty relation between space and time: $\Delta r$ $\Delta t$ $> G \hbar / c^4$; where G, $\hbar$ and c are …

High Energy Physics - TheoryNuclear and High Energy PhysicsInverseFOS: Physical sciencesInterval (mathematics)General Relativity and Quantum Cosmology (gr-qc)Type (model theory)Planck constant01 natural sciencesMeasure (mathematics)General Relativity and Quantum Cosmologysymbols.namesakeTheoretical physicsSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesIdeal (ring theory)010306 general physicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsQuantum Physics010308 nuclear & particles physicsGravitational constantHigh Energy Physics - Theory (hep-th)symbolsAstrophysics - High Energy Astrophysical PhenomenaQuantum Physics (quant-ph)Quantum clock
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Gravitational footprints of massive neutrinos and lepton number breaking

2020

We investigate the production of primordial Gravitational Waves (GWs) arising from First Order Phase Transitions (FOPTs) associated to neutrino mass generation in the context of type-I and inverse seesaw schemes. We examine both "high-scale" as well as "low-scale" variants, with either explicit or spontaneously broken lepton number symmetry $U(1)_L$ in the neutrino sector. In the latter case, a pseudo-Goldstone majoron-like boson may provide a candidate for cosmological dark matter. We find that schemes with softly-broken $U(1)_L$ and with single Higgs-doublet scalar sector lead to either no FOPTs or too weak FOPTs, precluding the detectability of GWs in present or near future measurements.…

High Energy Physics - TheoryNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Spontaneous symmetry breakingDark matterFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Computer Science::Digital Libraries01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometry0103 physical sciences010306 general physicsPhysics010308 nuclear & particles physicsMass generationHigh Energy Physics::PhenomenologyLepton numberlcsh:QC1-999High Energy Physics - PhenomenologySeesaw mechanismHigh Energy Physics - Theory (hep-th)Higgs bosonNeutrinolcsh:PhysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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