0000000000038550

AUTHOR

A. Sánchez

showing 4 related works from this author

Mixing asymmetries inBmeson systems, the D0 like-sign dimuon asymmetry, and generic new physics

2015

The measurement of a large like-sign dimuon asymmetry $A^b_{SL}$ by the D0 experiment at the Tevatron departs noticeably from Standard Model expectations and it may be interpreted as a hint of physics beyond the Standard Model contributing to $\Delta B\neq 0$ transitions. In this work we analyse how the natural suppression of $A^b_{SL}$ in the SM can be circumvented by New Physics. We consider generic Standard Model extensions where the charged current mixing matrix is enlarged with respect to the usual $3\times 3$ unitary Cabibbo-Kobayashi-Maskawa matrix, and show how, within this framework, a significant enhancement over Standard Model expectations for $A^b_{SL}$ is easily reachable throu…

PhysicsNuclear and High Energy PhysicsParticle physicsPhysics beyond the Standard Modelmedia_common.quotation_subjectTevatronFísicaFOS: Physical sciencesAsymmetryHigh Energy Physics - Experiment3. Good healthStandard ModelHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)CP violationB mesonCharged currentMixing (physics)media_commonPhysical Review D
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The polarimetric and helioseismic imager on solar orbiter

2020

This paper describes the Polarimetric and Helioseismic Imager on the Solar Orbiter mission (SO/PHI), the first magnetograph and helioseismology instrument to observe the Sun from outside the Sun-Earth line. It is the key instrument meant to address the top-level science question: How does the solar dynamo work and drive connections between the Sun and the heliosphere? SO/PHI will also play an important role in answering the other top-level science questions of Solar Orbiter, as well as hosting the potential of a rich return in further science. SO/PHI measures the Zeeman effect and the Doppler shift in the FeI 617.3nm spectral line. To this end, the instrument carries out narrow-band imaging…

Solar Telescope010504 meteorology & atmospheric sciencesphotosphere [Sun]FiltegramsHighly elliptical orbitFOS: Physical sciencesAstrophysics01 natural scienceslaw.inventionTelescopeOrbiterPhotospherelaw0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsHelioseismologySolar dynamo010303 astronomy & astrophysicsSun: magnetic fieldsInstrumentation and Methods for Astrophysics (astro-ph.IM)0105 earth and related environmental sciencesSun: helioseismologyPhysics[PHYS]Physics [physics]PhotosphereEllipsometrypolarimeters [Instrumentation]Spacecraftbusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyinstrumentation: polarimetersSun: photosphereHeliosismologiaAstronomy and AstrophysicsAstrophysics - Astrophysics of Galaxiestechniques: polarimetricmagnetic fields [Sun]Space and Planetary Sciencetechniques: imaging spectroscopyAstrophysics of Galaxies (astro-ph.GA)Physics::Space PhysicsHelioseismologyAstrophysics::Earth and Planetary AstrophysicsbusinessAstrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]HeliosphereEl·lipsometria
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OMC: An Optical Monitoring Camera for INTEGRAL

2003

The Optical Monitoring Camera (OMC) will observe the optical emission from the prime targets of the gammaray instruments onboard the ESA mission INTEGRAL, with the support of the JEM-X monitor in the X-ray domain. This capability will provide invaluable diagnostic information on the nature and the physics of the sources over a broad wavelength range. Its main scientific objectives are: (1) to monitor the optical emission from the sources observed by the gamma- and X-ray instruments, measuring the time and intensity structure of the optical emission for comparison with variability at high energies, and (2) to provide the brightness and position of the optical counterpart of any gamma- or X-r…

PhotometersUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Astronomía ópticaSpace vehiclesPhotometricPhotometers ; Space vehicles ; Instruments ; Photometric ; StarsUNESCO::ASTRONOMÍA Y ASTROFÍSICAInstrumentsStars:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]:ASTRONOMÍA Y ASTROFÍSICA::Astronomía óptica [UNESCO]
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Searches for violation of lepton flavour and baryon number in tau lepton decays at LHCb

2013

Searches for the lepton flavour violating decay tau(-) -> mu(-)mu(+)mu(-) and the lepton flavour and baryon number violating decays tau(-) -> (p) over bar mu(+)mu(-) and tau(-) -> p mu(-)mu(-) have been carried out using proton-proton collision data, corresponding to an integrated luminosity of 1.0 fb(-1), taken by the LHCb experiment at root s = 7 TeV. No evidence has been found for any signal, and limits have been set at 90% confidence level on the branching fractions: B(tau(-) -> mu(-)mu(+)mu(-) mu(+)mu(-)) p mu(-)mu(-)) (p) over bar mu(+)mu(-) and tau(-) -> p mu(-)mu(-) decay modes represent the first direct experimental limits on these channels.

Nuclear and High Energy PhysicsParticle physicsFlavourDecays of leptons; Global symmetries (e.g. baryon number lepton number); 13.35.-r; 11.30.Fs;FOS: Physical sciences01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentSettore FIS/04 - Fisica Nucleare e SubnucleareNuclear physicslepton number)High Energy Physics - Experiment (hep-ex)Violació CP (Física nuclear)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]LHC flavour physics lepton number11.30.FsNeutrinsNeutrinos010306 general physicsParticles (Nuclear physics)Physics13.35.-rDecays of leptonsLarge Hadron Collider010308 nuclear & particles physicsGlobal symmetries (e.g. baryon number lepton number)Leptons (Física nuclear)Global symmetries (e.g.High Energy Physics::Phenomenologybaryon numberDecays of lepton3. Good healthFIS/01 - FISICA SPERIMENTALELeptons (Nuclear physics)Física nuclearHigh Energy Physics::ExperimentBaryon numberNeutrino11.30.FFIS/04 - FISICA NUCLEARE E SUBNUCLEAREParticle Physics - ExperimentLeptonCP violation (Nuclear physics)Physics Letters B
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