Search results for "Strong gravity"

showing 3 items of 3 documents

Search for strong gravity signatures in same-sign dimuon final states using the ATLAS detector at the LHC

2012

A search for microscopic black holes has been performed in a same-sign dimuon final state using 1.3 fb[superscript −1] of proton–proton collision data collected with the ATLAS detector at a centre of mass energy of 7 TeV at the CERN Large Hadron Collider. The data are found to be consistent with the expectation from the Standard Model and the results are used to derive exclusion contours in the context of a low scale gravity model.

Atlas detectorPhysics::Instrumentation and DetectorsHadron01 natural sciencesHigh Energy Physics - ExperimentMicro black holeHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentDetectors de radiacióPhysicsINTERAÇÕES NUCLEARESLarge Hadron ColliderBLACK HOLEAtlas (topology)Strong gravityAcceleradors de partículesExtra DimensionsSettore FIS/01 - Fisica SperimentaleMicroscopic black holesATLASExtra dimensionsLarge Hadron ColliderComputingMethodologies_DOCUMENTANDTEXTPROCESSINGExtra dimensionsAtlasLHCParticle Physics - ExperimentNuclear and High Energy PhysicsParticle physicsDIMENSIONSCOLLISIONSSame-sign dimuonsCiências Naturais::Ciências Físicas:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesddc:500.2GRAVITY ON BRANE WORLDS530Partícules (Física nuclear)Nuclear physics0103 physical sciencesddc:530High Energy Physics010306 general physicsBLACK-HOLESMILLIMETERCiencias ExactasScience & TechnologyROOT-S=7 TEVATLAS detector010308 nuclear & particles physicssame-sign dimuons; microscopic black holes; extra dimensions; lhc; atlasFísicaCollisionLHC; ATLAS; Microscopic black holes; Extra dimensions; Same-sign dimuonsHADRON-HADRON COLLISIONSCol·lisions (Física nuclear)Experimental High Energy PhysicsPhysics::Accelerator PhysicsHigh Energy Physics::Experiment
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A deep study of the high–energy transient sky

2021

This is an open access article. This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds t…

Electromagnetic spectrumESA voyage 2050; High-energy transient sky; Multi-messenger astrophysics; Space mission concept; X–/γ–ray polarimetry; X–/γ–ray telescopes01 natural sciences7. Clean energylaw.inventionSettore FIS/05 - Astronomia E AstrofisicalawNuclear astrophysicsoptical010303 astronomy & astrophysicsmedia_commonPhysicsdensityStrong gravityAstrophysics::Instrumentation and Methods for AstrophysicsnucleosynthesisimagingParticle accelerationHigh-energy transient skyNeutrinoburstparticlelensmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenainterferometerSpace mission conceptTelescope0103 physical sciencesTeVequation of statepolarization010308 nuclear & particles physicsGravitational wavenucleusgravitational radiationAmbientaleAstronomyAstronomy and AstrophysicsaccelerationsensitivityMulti-messenger astrophysicsUniversemonitoringelectromagneticX–/γ–ray telescopesangular resolution[SDU]Sciences of the Universe [physics]13. Climate actionSpace and Planetary Sciencegamma raygravitationX–/γ–ray polarimetry[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]ESA voyage 2050
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Relativistic Low Angular Momentum Accretion: Long Time Evolution of Hydrodynamical Inviscid Flows

2018

We investigate relativistic low angular momentum accretion of inviscid perfect fluid onto a Schwarzschild black hole. The simulations are performed with a general-relativistic, high-resolution (second-order), shock-capturing, hydrodynamical numerical code. We use horizon-penetrating Eddington-Finkelstein coordinates to remove inaccuracies in regions of strong gravity near the black hole horizon and show the expected convergence of the code with the Michel solution and stationary Fishbone-Moncrief toroids. We recover, in the framework of relativistic hydrodynamics, the qualitative behavior known from previous Newtonian studies that used a Bondi background flow in a pseudo-relativistic gravit…

PhysicsAngular momentumPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsTurbulenceStrong gravityHorizonAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Mechanics01 natural sciencesAccretion (astrophysics)General Relativity and Quantum CosmologyGravitational potentialGeneral Relativity and Quantum CosmologyInviscid flow0103 physical sciencesSchwarzschild metric010303 astronomy & astrophysics
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