Search results for "cosmology theory"

showing 2 items of 2 documents

Non-circular rotating beams and CMB experiments

2002

This paper is concerned with small angular scale experiments for the observation of cosmic microwave background anisotropies. In the absence of beam, the effects of partial coverage and pixelisation are disentangled and analyzed (using simulations). Then, appropriate maps involving the CMB signal plus the synchrotron and dust emissions from the Milky Way are simulated, and an asymmetric beam --which turns following different strategies-- is used to smooth the simulated maps. An associated circular beam is defined to estimate the deviations in the angular power spectrum produced by beam asymmetry without rotation and, afterwards, the deviations due to beam rotation are calculated. For a cert…

Cosmic microwave background ; Cosmology theory ; Large-scale structure of the universe ; Numerical method ; Data analysis methodmedia_common.quotation_subjectCosmic microwave backgroundFOS: Physical sciencesAstrophysicsNumerical methodUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsRotationAsymmetryCosmic microwave backgroundlaw.inventionsymbols.namesakelawCosmology theoryLarge-scale structure of the universePlanckAnisotropymedia_commonPhysicsData analysis methodAstrophysics (astro-ph)Spectral densityAstronomy and Astrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]SynchrotronComputational physicsSpace and Planetary SciencesymbolsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Beam (structure)Astronomy & Astrophysics
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Light bosons in the photosphere and the solar abundance problem

2013

Spectroscopy is used to measure the elemental abundances in the outer layers of the Sun, whereas helioseismology probes the interior. It is well known that current spectroscopic determinations of the chemical composition are starkly at odds with the metallicity implied by helioseismology. We investigate whether the discrepancy may be due to conversion of photons to a new light boson in the solar photosphere. We examine the impact of particles with axion-like interactions with the photon on the inferred photospheric abundances, showing that resonant axion-photon conversion is not possible in the region of the solar atmosphere in which line formation occurs. Although non-resonant conversion i…

PhotonMetallicitysunelementary particlesElementary particleAstrophysics01 natural sciencesAbundance (ecology)0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsAbundancesHelioseismologysun atmosphere010303 astronomy & astrophysicsBosonLine (formation)PhysicsPhotosphere010308 nuclear & particles physicsformationAstronomy and Astrophysicscosmology theory13. Climate actionSpace and Planetary SciencelineAstrophysics::Earth and Planetary AstrophysicsMonthly Notices of the Royal Astronomical Society
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