Search results for "Fysiikka"

showing 10 items of 1348 documents

Black Hole Shadow Drift and Photon Ring Frequency Drift

2021

The apparent angular size of the shadow of a black hole in an expanding Universe is redshift-dependent. Since cosmological redshifts change with time - known as the redshift drift - all redshift-dependent quantities acquire a time-dependence, and a fortiori so do black hole shadows. We find a mathematical description of the black hole shadow drift and show that the amplitude of this effect is of order $10^{-16}$ per day for M87$^{\star}$. While this effect is small, we argue that its non-detection can be used to constrain the accretion rate around supermassive black holes, as well as a novel probe of the equivalence principle. If general relativity is assumed, we infer from the data obtaine…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)General relativityAstrophysics::High Energy Astrophysical PhenomenasuhteellisuusteoriaFrequency driftFOS: Physical sciencesmustat aukotGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicskosmologiaGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyavaruustutkimusfysiikkaEvent Horizon TelescopePhysicsSupermassive black holemaailmankaikkeusOrder (ring theory)Coupling (probability)varjotRedshiftBlack holeavaruusvaloAstrophysics - Cosmology and Nongalactic AstrophysicsThe Open Journal of Astrophysics
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Shining primordial black holes

2021

We study the well-motivated mixed dark matter (DM) scenario composed of a dominant thermal WIMP, highlighting the case of $SU(2)_L$ triplet fermion "winos", with a small fraction of primordial black holes (PBHs). After the wino kinetic decoupling, the DM particles are captured by PBHs leading to the presence of PBHs with dark minihalos in the Milky Way today. The strongest constraints for the wino DM come from the production of narrow line gamma rays from wino annihilation in the Galactic Center. We analyse in detail the viability of the mixed wino DM scenario, and determine the constraints on the fraction of DM in PBHs assuming a cored halo profile in the Milky Way. We show that already wi…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Milky WayAstrophysics::High Energy Astrophysical PhenomenaastrofysiikkaDARK-MATTER ANNIHILATIONFOS: Physical sciencesmustat aukotPrimordial black holeAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicskosmologia7. Clean energy01 natural sciences114 Physical sciencesGeneral Relativity and Quantum Cosmologypimeä aineHigh Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciences010306 general physicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Annihilation010308 nuclear & particles physicsGalactic CenterGAMMA-RAYSCONSTRAINTSFermionHigh Energy Physics - PhenomenologyMixed dark matterMILKYHaloAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic Astrophysics
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Axion star nucleation in dark minihalos around primordial black holes

2020

We consider a general class of axion models, including the QCD and string axion, in which the PQ symmetry is broken before or during inflation. Assuming the axion is the dominant component of the dark matter, we discuss axion star formation in virialized dark minihalos around primordial black holes through gravitational Bose-Einstein condensation. We determine the conditions for minihalos to kinetically produce axion stars before galaxy formation. Today, we expect up to $\sim 10^{17}$ ($\sim 10^9$) axion stars in a radius of 100 parsecs around the Sun for the case of the QCD (string) axion.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and DetectorsDark matterFOS: Physical sciencesmustat aukotPrimordial black holeGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicshiukkasfysiikka01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationHigh Energy Physics::TheoryHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesGalaxy formation and evolution010306 general physicsAxionAstrophysics::Galaxy AstrophysicsPhysicsInflation (cosmology)010308 nuclear & particles physicsStar formationHigh Energy Physics::PhenomenologyHigh Energy Physics - PhenomenologyStarsydinfysiikkaAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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Mesonic enhancement of the weak axial charge and its effect on the half-lives and spectral shapes of first-forbidden J+↔J− decays

2018

The effects of the enhancement of the axial-charge matrix element γ5 were studied in medium heavy and heavy nuclei for first-forbidden J+↔J− decay transitions using the nuclear shell model. Noticeable dependence on the enhancement ϵMEC of the axial-charge matrix element, as well as on the value of the axial-vector coupling constant gA was found in the spectral shapes of $^{93}$Y, $^{95}$Sr, and $^{97}$Y. The importance of the spectrum of $^{138}$Cs in the determination of gA is discussed. Half-life analyses in the A≈95 and A≈135 regions were done, and consistent results gA≈0.90, 0.75, and 0.65, corresponding to the three enhancement scenarios ϵMEC=1.4, 1.7, and 2.0, were obtained. Connectio…

Coupling constantPhysicsNuclear and High Energy PhysicsSpectral shape analysista114010308 nuclear & particles physicsSpectrum (functional analysis)forbidden beta decaysNuclear shell modelCharge (physics)01 natural scienceslcsh:QC1-999nuclear medium effectsspectral shapemeson-exchange currents0103 physical sciencesweak interactionsMatrix elementAtomic physicsAnomaly (physics)ydinfysiikka010306 general physicslcsh:PhysicsPhysics Letters B
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Iʿtibārī Concepts in Suhrawardī : The Case of Substance

2020

Abstract Shihāb al-Dīn al-Suhrawardī (d. 587/1191) famously criticised the central concepts of Avicennian metaphysics as merely mind-dependent (or iʿtibārī) notions. This paper aims to show that despite his critique, Suhrawardī held that these concepts are meaningful, indeed necessary for human cognition. By the same token, it is argued that their re-emergence in Suhrawardī’s ishrāqī metaphysics is not a matter of incoherence. Although the paper’s findings can be generalised to hold of all iʿtibārī concepts, mutatis mutandis, our focus is on the concept of substance, mainly because of the importance of the concept of ‘dusky substance’ in ishrāqī metaphysics.

Cultural Studies060103 classicsPhilosophyReligious studies06 humanities and the artsrealismi (filosofia)metafysiikka0603 philosophy ethics and religioniʿtibārSuhrawardīPhilosophykonseptualismi060302 philosophyAvicenna0601 history and archaeologyarabialainen filosofia
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The Influence of the Avicennan Theory of Science on Philosophical Sufism

2020

Abstract This article discusses the application of the Avicennan theory of demonstrative science on taṣawwuf, or the Divine Science (al-ʿilm al-ilāhī), by members of the Akbarian tradition, particularly Ibn ʿArabī’s (d. 1240) stepson and most influential disciple, Ṣadr al-Dīn al-Qūnawī (d. 1274), and his commentators, among whom the most prominent was Mullā Muḥammad b. Ḥamza al-Fanārī (d. 1431). It aims to find out what kind of relationship was developed between Avicennan logic and Sufism by the two members of the Akbarian school in the post-classical Islamic thought. It also seeks to show that the convergence between different currents of Islamic thought—Sufism and philosophy in this case—…

Cultural StudiesMullā FanārīsufilaisuusAvicennan theory of demonstrative sciencetieteenfilosofiaPhilosophy05 social sciencesReligious studiesAkbarian tradition of Sufismmetafysiikka06 humanities and the arts16. Peace & justice0603 philosophy ethics and religionSufismislam0506 political scienceEpistemologyPhilosophyṢadr al-Dīn al-Qūnawī060302 philosophy050602 political science & public administrationarabialainen filosofialogiikkaTheory of scienceOriens
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Measurement of D0, D+, D*+ and D+s production in pp collisions at √s = 5.02 TeV with ALICE

2019

The measurements of the production of prompt D0 , D+ , D∗+ , and D+s mesons in proton–proton (pp) collisions at s√=5.02 TeV with the ALICE detector at the Large Hadron Collider (LHC) are reported. D mesons were reconstructed at mid-rapidity ( |y|<0.5 ) via their hadronic decay channels D0→K−π+ , D+→K−π+π+ , D∗+→D0π+→K−π+π+ , D+s→ϕπ+→K+K−π+ , and their charge conjugates. The production cross sections were measured in the transverse momentum interval 0<pT<36 GeV/c for D0 , 1<pT<36 GeV/c for D+ and D∗+ , and in 2<pT<24 GeV/c for D+s mesons. Thanks to the higher integrated luminosity, an analysis in finer pT bins with respect to the previous measurements at s√=7 TeV was performed, allowing for …

D mesonsHigh Energy Physics::PhenomenologyHigh Energy Physics::ExperimenthiukkasfysiikkaNuclear Experimentpp collisions
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D-Meson Azimuthal Anisotropy in Midcentral Pb-Pb Collisions at √sNN = 5.02 TeV

2018

The azimuthal anisotropy coefficient v 2 of prompt D 0 , D + , D * + , and D + s mesons was measured in midcentral (30%–50% centrality class) Pb-Pb collisions at a center-of-mass energy per nucleon pair √ s N N = 5.02     TeV , with the ALICE detector at the LHC. The D mesons were reconstructed via their hadronic decays at midrapidity, | y | < 0.8 , in the transverse momentum interval 1 < p T < 24     GeV / c . The measured D -meson v 2 has similar values as that of charged pions. The D + s v 2 , measured for the first time, is found to be compatible with that of nonstrange D mesons. The measurements are compared with theoretical calculations of charm-quark transport in a hydrodynamically e…

D mesonsHigh Energy Physics::PhenomenologyNuclear TheoryHigh Energy Physics::Experimentheavy-ion collisionsanisotropyPhysics and Astronomy(all)hiukkasfysiikkaNuclear Experiment
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Measurement of azimuthal correlations of D mesons with charged particles in pp collisions at √s = 7 TeV and p-Pb collisions at √sNN = 5.02 TeV

2017

The azimuthal correlations of D mesons with charged particles were measured with the ALICE apparatus in pp collisions at √s = 7 TeV and p–Pb collisions at √sNN = 5.02 TeV at the Large Hadron Collider. D0, D+, and D∗+ mesons and their charge conjugates with transverse momentum 3 0.3 GeV/c. The yield of charged particles in the correlation peak induced by the jet containing the D meson and the peak width are compatible within uncertainties in the two collision systems. The data are described within uncertainties by Monte-Carlo simulations based on PYTHIA, POWHEG, and EPOS 3 event generators. peerReviewed

D mesonsp–Pb collisionsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::Experimentproton-proton collisionshiukkasfysiikkaNuclear Experiment
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Theory for the stationary polariton response in the presence of vibrations

2019

We construct a model describing the response of a hybrid system where the electromagnetic field - in particular, surface plasmon polaritons - couples strongly with electronic excitations of atoms or molecules. Our approach is based on the input-output theory of quantum optics, and in particular it takes into account the thermal and quantum vibrations of the molecules. The latter is described within the $P(E)$ theory analogous to that used in the theory of dynamical Coulomb blockade. As a result, we are able to include the effect of the molecular Stokes shift on the strongly coupled response of the system. Our model then accounts for the asymmetric emission from upper and lower polariton mod…

DYNAMICSQuantum decoherenceFOS: Physical sciences02 engineering and technology01 natural sciencesplasmonicsvärähtelytQuantum mechanics0103 physical sciencesMesoscale and Nanoscale Physics (cond-mat.mes-hall)Polaritonhybrid quantum systemskvanttikemiaMOLECULE010306 general physicskvanttifysiikkaQuantumQuantum opticsPhysicsQuantum PhysicsCondensed Matter - Mesoscale and Nanoscale PhysicsSurface plasmonCoulomb blockade021001 nanoscience & nanotechnologySurface plasmon polaritonSURFACE-PLASMON POLARITONSpintailmiötLight emission0210 nano-technologyQuantum Physics (quant-ph)ENERGY-TRANSFERpolaritonsemissio (fysiikka)
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