0000000000200901

AUTHOR

Alessio Notari

showing 3 related works from this author

Axion search with BabyIAXO in view of IAXO

2020

Axions are a natural consequence of the Peccei-Quinn mechanism, the most compelling solution to the strong-CP problem. Similar axion-like particles (ALPs) also appear in a number of possible extensions of the Standard Model, notably in string theories. Both axions and ALPs are very well motivated candidates for Dark Matter, and in addition, they would be copiously produced at the sun's core. A relevant effort during the last decade has been the CAST experiment at CERN, the most sensitive axion helioscope to-date. The International Axion Observatory (IAXO) is a large-scale 4th generation helioscope. As its primary physics goal, IAXO will look for solar axions or ALPs with a signal to backgro…

Particle physicsPhysics - Instrumentation and Detectorssolar axion[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]experimental methodsDark matterFOS: Physical sciences7. Clean energyString (physics)Standard Modelaxion helioscopedesign [detector]International Axion Observatory (IAXO)ObservatoryPeccei-Quinn mechanismDark Matterdetector design[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Detectors and Experimental TechniquesAxionsun-tracking systemsphysics.ins-detactivity reportdetector: designPhysicsinstrumentationHelioscopeLarge Hadron Colliderdetectorsolar [axion]DESYInstrumentation and Detectors (physics.ins-det)[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]IAXOmagnetopticsaxion: solar
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Observational constraints on inhomogeneous cosmological models without dark energy

2011

It has been proposed that the observed dark energy can be explained away by the effect of large-scale nonlinear inhomogeneities. In the present paper we discuss how observations constrain cosmological models featuring large voids. We start by considering Copernican models, in which the observer is not occupying a special position and homogeneity is preserved on a very large scale. We show how these models, at least in their current realizations, are constrained to give small, but perhaps not negligible in certain contexts, corrections to the cosmological observables. We then examine non-Copernican models, in which the observer is close to the center of a very large void. These models can gi…

Void (astronomy)Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmologysymbols.namesakeTheoretical physics0103 physical sciencesHomogeneity (physics)98.62.Sb010303 astronomy & astrophysicsPhysics010308 nuclear & particles physics98.80.EsObservable95.36.+xCopernican principleNonlinear systemDark energysymbols[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]98.65.DxAstrophysics - Cosmology and Nongalactic AstrophysicsSpecial position
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Next Generation Search for Axion and ALP Dark Matter with the International Axion Observatory

2018

International audience; More than 80 years after the postulation of dark matter, its nature remains one of the fundamental questions in cosmology. Axions are currently one of the leading candidates for the hypothetical, non-baryonic dark matter that is expected to account for about 25% of the energy density of the Universe. Especially in the light of the Large Hadron Collider at CERN slowly closing in on Weakly-Interacting Massive Particle (WIMP) searches, axions and axion-like particles (ALPs) provide a viable alternative approach to solving the dark matter problem. The fact that makes them particularly appealing is that they were initially introduced to solve a long-standing problem in qu…

Particle physicsCERN LabPhysics::Instrumentation and DetectorsDark matterObservatoriesaxion: detector7. Clean energy01 natural sciencesCosmologyHigh Energy Physics::TheoryPrimakoff effectSensitivityWIMP0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsAxionPrimakoff effectactivity reportPhysicsHelioscopeLarge Hadron Collider010308 nuclear & particles physicsPhysicsHigh Energy Physics::PhenomenologyToroidal magnetic fieldsDetectorsobservatory13. Climate actionCouplingsaxion-like particlesproposed experimentCERN Axion Solar Telescopeaxion: solarTelescopes
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