Search results for " Cosmology"

showing 10 items of 1486 documents

Infrasonic, Acoustic and Seismic Waves Produced by the Axion Quark Nuggets

2022

We advocate an idea that the Axion Quark Nuggets (AQN) hitting the Earth can be detected by analysing the infrasound, acoustic and seismic waves which always accompany the AQN's passage in the atmosphere and underground. Our estimates for the infrasonic frequency $\nu\simeq 5$ ~Hz and overpressure $\delta p\sim 0.3 ~$Pa for relatively large size dark matter (DM) nuggets suggest that sensitivity of presently available instruments is already sufficient to detect very intense (but very rare) events today with existing technology. A study of much more frequent but less intense events requires a new type of instruments. We propose a detection strategy for a systematic study to search for such re…

Earth and Planetary Astrophysics (astro-ph.EP)570Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)General MathematicsFOS: Physical sciencesGeophysics (physics.geo-ph)Physics - GeophysicsHigh Energy Physics - PhenomenologyPhysics - Atmospheric and Oceanic PhysicsHigh Energy Physics - Phenomenology (hep-ph)Chemistry (miscellaneous)ddc:570Atmospheric and Oceanic Physics (physics.ao-ph)Computer Science (miscellaneous)dark matter; axion; quark nuggetsAstrophysics - Cosmology and Nongalactic AstrophysicsAstrophysics - Earth and Planetary AstrophysicsSymmetry
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Photon frequency shift in curvature based Extended Theories of Gravity

2021

We study the frequency shift of photons generated by rotating gravitational sources in the framework of curvature based Extended Theories of Gravity. The discussion is developed considering the weak-field approximation. Following a perturbative approach, we analyze the process of exchanging photons between Earth and a given satellite, and we find a general relation to constrain the free parameters of gravitational theories. Finally, we suggest the Moon as a possible laboratory to test theories of gravity by future experiments which can be, in principle, based also on other Solar System bodies.

Earth and Planetary Astrophysics (astro-ph.EP)High Energy Physics - TheoryHigh Energy Physics - Theory (hep-th)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyAstrophysics - Earth and Planetary Astrophysics
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Conformal transformations and weak field limit of scalar-tensor gravity

2013

The weak field limit of scalar tensor theories of gravity is discussed in view of conformal transformations. Specifically, we consider how physical quantities, like gravitational potentials derived in the Newtonian approximation for the same scalar-tensor theory, behave in the Jordan and in the Einstein frame. The approach allows to discriminate features that are invariant under conformal transformations and gives contributions in the debate of selecting the true physical frame. As a particular example, the case of $f(R)$ gravity is considered.

Earth and Planetary Astrophysics (astro-ph.EP)PhysicsNuclear and High Energy PhysicsConformal field theoryScalar (physics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Invariant (physics)Astrophysics - Astrophysics of GalaxiesGeneral Relativity and Quantum CosmologyGravitationConformal gravityGeneral Relativity and Quantum CosmologyParameterized post-Newtonian formalismConformal symmetryAstrophysics of Galaxies (astro-ph.GA)f(R) gravityAstrophysics - Earth and Planetary AstrophysicsMathematical physicsPhysical Review D
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On the annual modulation signal in dark matter direct detection

2012

We derive constraints on the annual modulation signal in Dark Matter (DM) direct detection experiments in terms of the unmodulated event rate. A general bound independent of the details of DM distribution follows from the assumption that the motion of the earth around the sun is the only source of time variation. The bound is valid for a very general class of particle physics models and also holds in the presence of an unknown unmodulated background. More stringent bounds are obtained, if modest assumptions on symmetry properties of the DM halo are adopted. We illustrate the bounds by applying them to the annual modulation signals reported by the DAMA and CoGeNT experiments in the framework…

Elastic scatteringPhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencesAstronomy and AstrophysicsCosmologySymmetry (physics)Particle identificationHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)ModulationStatistical physicsHaloEvent (particle physics)Astrophysics - Cosmology and Nongalactic Astrophysics
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Semiclassical geons as solitonic black hole remnants

2013

We find that the end state of black hole evaporation could be represented by non-singular and without event horizon stable solitonic remnants with masses of the order the Planck scale and up to similar to 16 units of charge. Though these objects are locally indistinguishable from spherically symmetric, massive electric (or magnetic) charges, they turn out to be sourceless geons containing a wormhole generated by the electromagnetic field. Our results are obtained by interpreting semiclassical corrections to Einstein's theory in the first-order (Palatini) formalism, which yields second-order equations and avoids the instabilities of the usual (metric) formulation of quadratic gravity. We als…

Electromagnetic fieldHigh Energy Physics - TheoryCosmology and Nongalactic Astrophysics (astro-ph.CO)Event horizonDark matterSemiclassical physicsFOS: Physical sciencesPrimordial black holeGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationGeneral Relativity and Quantum Cosmology0103 physical sciencesWormhole010306 general physicsmodified gravityMathematical physicsPhysics010308 nuclear & particles physicsprimordial black holesAstronomy and Astrophysicsquantum field theory on curved spaceBlack holeHigh Energy Physics - Theory (hep-th)WormholesAstrophysics - Cosmology and Nongalactic Astrophysics
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Multicenter solutions in Eddington-inspired Born-Infeld gravity

2020

We find multicenter (Majumdar-Papapetrou type) solutions of Eddington-inspired Born-Infeld gravity coupled to electromagnetic fields governed by a Born-Infeld-like Lagrangian. We construct the general solution for an arbitrary number of centers in equilibrium and then discuss the properties of their one-particle configurations, including the existence of bounces and the regularity (geodesic completeness) of these spacetimes. Our method can be used to construct multicenter solutions in other theories of gravity.

Electromagnetic fieldHigh Energy Physics - TheoryGravity (chemistry)Física-Modelos matemáticosPhysics and Astronomy (miscellaneous)GeodesicFOS: Physical scienceslcsh:AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Type (model theory)01 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesakeGeneral Relativity and Quantum CosmologyCompleteness (order theory)0103 physical scienceslcsh:QB460-466Física matemáticalcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsEngineering (miscellaneous)Mathematical physicsPhysics010308 nuclear & particles physicsHigh Energy Physics - Theory (hep-th)symbolslcsh:QC770-798Lagrangian
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Dispersion Interactions between Neutral Atoms and the Quantum Electrodynamical Vacuum

2018

Dispersion interactions are long-range interactions between neutral ground-state atoms or molecules, or polarizable bodies in general, due to their common interaction with the quantum electromagnetic field. They arise from the exchange of virtual photons between the atoms, and, in the case of three or more atoms, are not additive. In this review, after having introduced the relevant coupling schemes and effective Hamiltonians, as well as properties of the vacuum fluctuations, we~outline the main properties of dispersion interactions, both in the nonretarded (van der Waals) and retarded (Casimir--Polder) regime. We then discuss their deep relation with the existence of the vacuum fluctuation…

Electromagnetic fieldHigh Energy Physics - TheoryPhysics and Astronomy (miscellaneous)Field (physics)General MathematicsVan der Waals forceFOS: Physical sciencesVirtual particleCasimir-Polder interactionGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum Cosmologyvacuum energyCasimir–Polder interactionssymbols.namesakeMany-body dispersion interactionVacuum energyQuantum mechanics0103 physical sciencesDispersion (optics)Computer Science (miscellaneous)Vacuum fluctuation010306 general physicsvacuum fluctuationsQuantum fluctuationPhysicsQuantum Physics010308 nuclear & particles physicslcsh:Mathematicsmany-body dispersion interactionslcsh:QA1-939Unruh effectHigh Energy Physics - Theory (hep-th)Chemistry (miscellaneous)symbolsvan der Waals forcesvan der Waals forceQuantum Physics (quant-ph)
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Van der Waals and resonance interactions between accelerated atoms in vacuum and the Unruh effect

2017

We discuss different physical effects related to the uniform acceleration of atoms in vacuum, in the framework of quantum electrodynamics. We first investigate the van der Waals/Casimir-Polder dispersion and resonance interactions between two uniformly accelerated atoms in vacuum. We show that the atomic acceleration significantly affects the van der Waals force, yielding a different scaling of the interaction with the interatomic distance and an explicit time dependence of the interaction energy. We argue how these results could allow for an indirect detection of the Unruh effect through dispersion interactions between atoms. We then consider the resonance interaction between two accelerat…

Electromagnetic fieldHistoryField (physics)Vacuum stateFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesResonance (particle physics)General Relativity and Quantum CosmologyEducationsymbols.namesake0103 physical sciencesPhysics::Atomic and Molecular Clusters010306 general physicsQuantum fluctuationPhysicsQuantum Physics010308 nuclear & particles physicsInteraction energyComputer Science ApplicationsUnruh effectsymbolsAtomic physicsvan der Waals forceQuantum Physics (quant-ph)Dispersion Interactions Resonance interactions Vacuum field fluctuations Unruh effect.Journal of Physics: Conference Series
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Generalized Einstein-Maxwell field equations in the Palatini formalism

2013

We derive a new set of field equations within the framework of the Palatini formalism.These equations are a natural generalization of the Einstein-Maxwell equations which arise by adding a function $\mathcal{F}(\mathcal{Q})$, with $\mathcal{Q}\equiv F^{\alpha\beta}F_{\alpha\beta}$ to the Palatini Lagrangian $f(R,Q)$.The result we obtain can be viewed as the coupling of gravity with a nonlinear extension of the electromagnetic field.In addition,a new method is introduced to solve the algebraic equation associated to the Ricci tensor.

Electromagnetic fieldPhysicsAstronomy and AstrophysicsMaxwell fieldGeneral Relativity and Quantum CosmologyGravitationFormalism (philosophy of mathematics)Nonlinear systemAlgebraic equationsymbols.namesakeGeneral Relativity and Quantum CosmologySpace and Planetary SciencesymbolsEinsteinMathematical PhysicsRicci curvatureMathematical physics
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The role of the ergosphere in the Blandford-Znajek process

2012

The Blandford-Znajek process, one of the most promising model for powering the relativistic jets from black holes, was initially introduced as a mechanism in which the magnetic fields extract energy from a rotating black hole. We study the evolution of force-free electromagnetic fields on regular spacetimes with an ergosphere, which are generated by rapidly rotating stars. Our conclusive results confirm previous works, claiming that the Blandford-Znajek mechanism is not directly related to the horizon of the black hole. We also show that the radiated energy depends exponentially on the compactness of the star.

Electromagnetic fieldPhysicsGeneral Relativity and Quantum CosmologyStarsRotating black holeAstrophysical jetSpace and Planetary ScienceAstrophysics::High Energy Astrophysical PhenomenaQuantum electrodynamicsBlandford–Znajek processAstronomy and AstrophysicsErgosphereMagnetic fieldMonthly Notices of the Royal Astronomical Society
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