Search results for "GENERAL-RELATIVITY"

showing 3 items of 3 documents

New horizons for fundamental physics with LISA

2022

K. G. Arun et al.

AstrofísicaPROTOPLANET MIGRATIONFísica-Modelos matemáticosPhysics and Astronomy (miscellaneous)gr-qcFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)GRAVITATIONAL-WAVEShorizonFundamental physicGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsGravitational wavesLIGO (Observatory)Tests of general relativitySettore FIS/05 - Astronomia e AstrofisicaDARK-MATTERFísica matemáticaKOZAI MECHANISMHigh Energy PhysicsGENERAL-RELATIVITYFundamental physics; Gravitational waves; LISA; Tests of general relativityFundamental physicsPRIMORDIAL BLACK-HOLESLISAScience & TechnologyGeneral Relativity and Cosmology83CXXPhysicsgravitation: interactiongravitational radiationFísicaCompactQUANTUM-GRAVITYPhysical SciencesAstronomia[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]fundamental physics; gravitational waves; LISA; test of general relativityMODIFIED GRAVITYtest of general relativityGravitational waveMULTIPOLE MOMENTSHUBBLE CONSTANT
researchProduct

Critical point Higgs inflation in the Palatini formulation

2021

We study Higgs inflation in the Palatini formulation with the renormalisation group improved potential in the case when loop corrections generate a feature similar to an inflection point. Assuming that there is a threshold correction for the Higgs quartic coupling $\lambda$ and the top Yukawa coupling $y_t$, we scan the three-dimensional parameter space formed by the two jumps and the non-minimal coupling $\xi$. The spectral index $n_s$ can take any value in the observationally allowed range. The lower limit for the running is $\alpha_s>-3.5\times10^{-3}$, and $\alpha_s$ can be as large as the observational upper limit. Running of the running is small. The tensor-to-scalar ratio is $2.2\tim…

Nuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesRIEMANNGeneral Relativity and Quantum Cosmology (gr-qc)Parameter spaceINITIAL CONDITIONSkosmologia01 natural sciences114 Physical sciencesGeneral Relativity and Quantum CosmologyEINSTEINCritical point (thermodynamics)0103 physical sciencesRenormalization Grouplcsh:Nuclear and particle physics. Atomic energy. Radioactivityteoreettinen fysiikkaGENERAL-RELATIVITY010306 general physicscosmology of theories beyond the SMDISSIPATIONBosonMathematical physicsInflation (cosmology)Physics010308 nuclear & particles physicsYukawa potentialCONSTRAINTSBOSONGRAVITATIONRenormalization groupAFFINE VARIATIONAL-PRINCIPLESCosmology of Theories beyond the SMInflection pointHiggs bosonSCALARONlcsh:QC770-798renormalization groupAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
researchProduct

Importance of torsion and invariant volumes in Palatini theories of gravity

2013

We study the field equations of extensions of general relativity formulated within a metric-affine formalism setting torsion to zero (Palatini approach). We find that different (second-order) dynamical equations arise depending on whether torsion is set to zero (i) a priori or (ii) a posteriori, i.e., before or after considering variations of the action. Considering a generic family of Ricci-squared theories, we show that in both cases the connection can be decomposed as the sum of a Levi-Civita connection and terms depending on a vector field. However, while in case (i) this vector field is related to the symmetric part of the connection, in (ii) it comes from the torsion part and, therefo…

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsGeneral-relativitybusiness.industryLibrary scienceFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Invariant (physics)General Relativity and Quantum CosmologyTheoretical physicsCosmological constantsHigh Energy Physics - Theory (hep-th)Research councilHospitalityPartial supportbusinessField equation
researchProduct