0000000000363049

AUTHOR

Paolo Serra

showing 5 related works from this author

Asymmetric Dark Matter and Dark Radiation

2012

Asymmetric Dark Matter (ADM) models invoke a particle-antiparticle asymmetry, similar to the one observed in the Baryon sector, to account for the Dark Matter (DM) abundance. Both asymmetries are usually generated by the same mechanism and generally related, thus predicting DM masses around 5 GeV in order to obtain the correct density. The main challenge for successful models is to ensure efficient annihilation of the thermally produced symmetric component of such a light DM candidate without violating constraints from collider or direct searches. A common way to overcome this involves a light mediator, into which DM can efficiently annihilate and which subsequently decays into Standard Mod…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectCosmic microwave backgroundDark matterFOS: Physical sciences01 natural sciencesStandard Modelsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPlanck010306 general physicsParticle Physics - Phenomenologymedia_commonPhysicsCosmologia010308 nuclear & particles physicsMatter power spectrumAstronomy and AstrophysicsUniverseBaryonHigh Energy Physics - Phenomenology13. Climate actionDark radiationsymbolsAstrophysics - Cosmology and Nongalactic Astrophysics
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Observables sensitive to absolute neutrino masses. II

2008

In this followup to Phys. Rev. D 75, 053001 (2007) [arXiv:hep-ph/0608060] we report updated constraints on neutrino mass-mixing parameters, in light of recent neutrino oscillation data (KamLAND, SNO, and MINOS) and cosmological observations (WMAP 5-year and other data). We discuss their interplay with the final 0nu2beta decay results in 76-Ge claimed by part of the Heidelberg-Moscow Collaboration, using recent evaluations of the corresponding nuclear matrix elements, and their uncertainties. We also comment on the 0nu2beta limits in 130-Te recently set by Cuoricino, and on prospective limits or signals from the KATRIN experiment.

PhysicsMass numberNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics (astro-ph)Cosmic background radiationFOS: Physical sciencesAstrophysicsCMB cold spotHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)MINOSDouble beta decayHigh Energy Physics::ExperimentSensitivity (control systems)Nuclear Experiment (nucl-ex)NeutrinoNeutrino oscillationNuclear ExperimentPhysical Review D
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Impact of general reionization scenarios on extraction of inflationary parameters

2010

Determination of whether the Harrison-Zel'dovich spectrum for primordial scalar perturbations is consistent with observations is sensitive to assumptions about the reionization scenario. In light of this result, we revisit constraints on inflationary models using more general reionization scenarios. While the bounds on the tensor-to-scalar ratio are largely unmodified, when different reionization schemes are addressed, hybrid models are back into the inflationary game. In the general reionization picture, we reconstruct both the shape and amplitude of the inflaton potential. We discuss how relaxing the simple reionization restriction affects the reconstruction of the potential through the c…

Inflation (cosmology)PhysicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmic microwave backgroundCosmic background radiationAstrophysics::Instrumentation and Methods for AstrophysicsSpectral densityFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsInflatonCMB cold spotCosmologyGeneral Relativity and Quantum CosmologyFísica nuclearReionizationAstrophysics - Cosmology and Nongalactic Astrophysics
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Apolipoprotein E genotype does not influence the progression of multiple sclerosis

2003

OBJECTIVE: To investigate the association between apolipoprotein E (APOE) polymorphisms and the progression of MS. METHODS: We investigated 428 subjects affected by clinically defined MS, with a disease duration of at least three years. We collected data concerning the age at onset of MS, clinical type, disease duration and disability according to the expanded disability status scale (EDSS). We also calculated the progression index (PI) to evaluate disease progression. APOE genotyping and the -491 A/T polymorphism of the APOE promoter were determined. RESULTS: No association was observed between the APOE epsilon4 allele and clinical characteristics of our study population. We also investiga…

OncologyApolipoprotein EAdultMalemedicine.medical_specialtyMultiple SclerosisGenotypeAdolescentOdds Ratio; Polymorphism Genetic; Chi-Square Distribution; Humans; Disease Progression; Apolipoproteins E; Genotype; Multiple Sclerosis; Adult; Confidence Intervals; Adolescent; Statistics Nonparametric; Female; MalePopulationAPOE polymorphismBiologyStatistics NonparametricApolipoproteins EGeneticPolymorphism (computer science)Internal medicineGenotypeMultiple SclerosimedicineOdds RatioConfidence IntervalsHumansNonparametricPolymorphismeducationGenotypingAPOE promotereducation.field_of_studyExpanded Disability Status ScalePolymorphism GeneticChi-Square DistributionMS progressionStatisticsOdds ratioNeurologyImmunologyDisease ProgressionPopulation studylipids (amino acids peptides and proteins)FemaleSettore MED/26 - NeurologiaNeurology (clinical)Confidence IntervalHuman
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Harrison-Zel'dovich primordial spectrum is consistent with observations

2010

Inflation predicts primordial scalar perturbations with a nearly scale-invariant spectrum and a spectral index approximately unity (the Harrison--Zel'dovich (HZ) spectrum). The first important step for inflationary cosmology is to check the consistency of the HZ primordial spectrum with current observations. Recent analyses have claimed that a HZ primordial spectrum is excluded at more than 99% c.l.. Here we show that the HZ spectrum is only marginally disfavored if one considers a more general reionization scenario. Data from the Planck mission will settle the issue.

Inflation (cosmology)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Nuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Scalar (mathematics)Spectral densityFOS: Physical sciencesFísicaAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsCMB cold spotGeneral Relativity and Quantum CosmologyCosmologyHigh Energy Physics - Phenomenologysymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Observational cosmologysymbolsPlanckAstrophysics - High Energy Astrophysical PhenomenaReionizationAstrophysics - Cosmology and Nongalactic Astrophysics
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