0000000000650032

AUTHOR

Diego Blas

0000-0003-2646-0112

showing 3 related works from this author

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

No chiral light bending by clumps of axion-like particles

2019

We study the propagation of light in the presence of a parity-violating coupling between photons and axion-like particles (ALPs). Naively, this interaction could lead to a split of light rays into two separate beams of different polarization chirality and with different refraction angles. However, by using the eikonal method we explicitly show that this is not the case and that ALP clumps do not produce any spatial birefringence. This happens due to non-trivial variations of the photon's frequency and wavevector, which absorb time-derivatives and gradients of the ALP field. We argue that these variations represent a new way to probe the ALP-photon couping with precision frequency measuremen…

High Energy Physics - TheoryPhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)BirefringencePhoton010308 nuclear & particles physicsEikonal equationFOS: Physical sciencesPhysics::OpticsAstronomy and AstrophysicsPolarization (waves)01 natural sciencesMolecular physicsRayPhysics::GeophysicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Space and Planetary Science0103 physical sciencesWave vectorChirality (chemistry)010303 astronomy & astrophysicsAxionAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Constraints on millicharged dark matter and axionlike particles from timing of radio waves

2019

We derive novel constraints on millicharged dark matter and ultralight axion-like particles using pulsar timing and fast radio burst observations. Millicharged dark matter affects the dispersion measure of the time of arrival of radio pulses in a way analogous to free electrons. Light pseudo-scalar dark matter, on the other hand, causes the polarization angle of radio signals to oscillate. We show that current and future data can set strong constraints in both cases. For dark matter particles of charge $\epsilon e$, these constraints are ${\epsilon}/{m_{\rm milli}} \lesssim 10^{-8}{\rm eV}^{-1}$, for masses $m_{\rm milli}\gtrsim 10^{-6}\,$eV. For axion-like particles, the analysis of signal…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Particle physicsaxionsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsaxions; gravity; radio astronomy; pulsarsAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)radio astronomy01 natural sciencesGeneral Relativity and Quantum CosmologygravityHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Computer Science::Systems and Control0103 physical sciencesEnergy densitypulsars010306 general physicsAstrophysics - High Energy Astrophysical PhenomenaRadio waveAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
researchProduct