المؤلفون: David Maurin, P. Salati, Nathanael Weinrich, Marco Cirelli, Julien Lavalle, Laurent Derome, Yoann Génolini, Mathieu Boudaud

المساهمون: Niels Bohr Institute [Copenhagen] (NBI), Faculty of Science [Copenhagen], University of Copenhagen = Københavns Universitet (KU)-University of Copenhagen = Københavns Universitet (KU), Instituto de Física Teórica UAM/CSIC (IFT), Universidad Autonoma de Madrid (UAM)-Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), Laboratoire de Physique Théorique et Hautes Energies (LPTHE), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Laboratoire Univers et Particules de Montpellier (LUPM), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)

المصدر: Physical Review D
Physical Review D, American Physical Society, 2021, 104 (8), pp.083005. ⟨10.1103/PhysRevD.104.083005⟩
Genolini, Y, Boudaud, M, Cirelli, M, Derome, L, Lavalle, J, Maurin, D, Salati, P & Weinrich, N 2021, ' New minimal, median, and maximal propagation models for dark matter searches with Galactic cosmic rays ', Physical Review D, vol. 104, no. 8, 083005 . https://doi.org/10.1103/PhysRevD.104.083005Test

مصطلحات موضوعية: electron, HIGH-ENERGY, POWER REQUIREMENTS, halo, Primordial black hole, Astrophysics, Electron, antinucleus, 01 natural sciences, 98.70.Sa, High Energy Physics - Phenomenology (hep-ph), benchmark, Positron, PAMELA, propagation, transport theory, AMS, 12.60.-i, 010303 astronomy & astrophysics, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, REACCELERATION, Annihilation, High Energy Physics - Phenomenology, SAMPLE TRANSPORT, covariance, cosmic radiation: galaxy, PARTICLE PHYSICS, 95.35.+d, Halo, Astrophysics - High Energy Astrophysical Phenomena, black hole: primordial, positron: background, 96.50.S, IN-DIFFUSION MODELS, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, FOS: Physical sciences, SOURCE PARAMETERS, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, SPATIAL ORIGIN, 0103 physical sciences, MONTE-CARLO TECHNIQUE, 010306 general physics, 98.35.Gi, anti-p: secondary, dark matter: annihilation, flux, Antiproton, [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph], SOLAR MODULATION, Physics::Accelerator Physics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], statistical

وصف الملف: application/pdf

الوصول الحر: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a283b15acd8ef20b197d57e1034df0f6Test
https://doi.org/10.1103/physrevd.104.083005Test

المؤلفون: Génolini, Yoann, Boudaud, Mathieu, Cirelli, Marco, Derome, Laurent, Lavalle, Julien, Maurin, David, Salati, Pierre, Weinrich, Nathanael

المساهمون: Niels Bohr Institute Copenhagen (NBI), Faculty of Science Copenhagen, University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH), Instituto de Física Teórica UAM/CSIC (IFT), Consejo Superior de Investigaciones Cientificas España = Spanish National Research Council Spain (CSIC)-Universidad Autónoma de Madrid (UAM), Laboratoire de Physique Théorique et Hautes Energies (LPTHE), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Laboratoire Univers et Particules de Montpellier (LUPM), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS), ANR-18-CE31-0006,GaDaMa,Matière Noire Galactique(2018)

المصدر: ISSN: 1550-7998.

مصطلحات موضوعية: 12.60.-i, 95.35.+d, 96.50.S-, 98.35.Gi, 98.70.Sa, cosmic radiation: galaxy, dark matter: annihilation, positron: background, anti-p: secondary, black hole: primordial, transport theory, antinucleus, propagation, statistical, covariance, benchmark, electron, flux, AMS, PAMELA, halo, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]

العلاقة: info:eu-repo/semantics/altIdentifier/arxiv/2103.04108; hal-03178521; https://hal.science/hal-03178521Test; ARXIV: 2103.04108; INSPIRE: 1850561

الإتاحة: https://doi.org/10.1103/PhysRevD.104.083005Test
https://hal.science/hal-03178521Test

المؤلفون: Kappl, Rolf, Winkler, Martin Wolfgang

المصدر: Journal of cosmology and astroparticle physics 2014(09), 051 (2014). doi:10.1088/1475-7516/2014/09/051

مصطلحات موضوعية: info:eu-repo/classification/ddc/530, anti-p: cosmic radiation, anti-p: secondary, anti-p: flux, anti-p: production, anti-n: production, isospin: effect, hyperon: decay, background, Monte Carlo, CERN Lab, fission, NA49

جغرافية الموضوع: DE

العلاقة: info:eu-repo/semantics/altIdentifier/wos/WOS:000342642500052; info:eu-repo/semantics/altIdentifier/issn/1475-7516; https://bib-pubdb1.desy.de/record/172406Test; https://bib-pubdb1.desy.de/searchTest?p=id:%22PUBDB-2014-03713%22

الإتاحة: https://doi.org/10.1088/1475-7516/2014/09/051Test
https://bib-pubdb1.desy.de/record/172406Test
https://bib-pubdb1.desy.de/searchTest?p=id:%22PUBDB-2014-03713%22

المؤلفون: Senger, P., CBM Collaboration

المصدر: Physica scripta 96(5), 054002-(2021). doi:10.1088/1402-4896/abebfe
Physica Scripta

مصطلحات موضوعية: CBM, heavy [nucleus], accelerator, Qcd phase diagram, nuclear astrophysics, Nuclear Theory, secondary beam [anti-p], FOS: Physical sciences, 01 natural sciences, 7. Clean energy, 010305 fluids & plasmas, anti-p: secondary beam, Nuclear physics, 0103 physical sciences, Nuclear astrophysics, matter [quantum chromodynamics], ddc:530, Darmstadt GSI FAIR, Nuclear Experiment (nucl-ex), 010306 general physics, neutron star, Nuclear Experiment, Mathematical Physics, equation of state, QCD phase diagram, quantum chromodynamics: matter, Physics, baryon: density: high, nucleosynthesis, p: beam, heavy-ion collisions, Condensed Matter Physics, Atomic and Molecular Physics, and Optics, beam [p], nucleus: heavy, density: high [baryon], Physics::Accelerator Physics, Heavy ion, heavy ion [beam], beam: heavy ion

الوصول الحر: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::159c616a671718dad5287bdf7c205ef0Test

المؤلفون: Boudaud, Mathieu, Génolini, Yoann, Derome, Laurent, Lavalle, Julien, Maurin, David, Salati, Pierre, Serpico, Pasquale D.

المساهمون: Laboratoire de Physique Théorique et Hautes Energies (LPTHE), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Laboratoire Univers et Particules de Montpellier (LUPM), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS)

المصدر: PoS ; 36th International Cosmic Ray Conference ; https://hal.science/hal-02973170Test ; 36th International Cosmic Ray Conference, Jul 2019, Madison, United States. pp.038, ⟨10.22323/1.358.0038⟩

مصطلحات موضوعية: anti-p: secondary, anti-p: flux, cosmic radiation, correlation, dark matter, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]

جغرافية الموضوع: United States

الوقت: Madison, United States

العلاقة: hal-02973170; https://hal.science/hal-02973170Test; INSPIRE: 1820402

الإتاحة: https://doi.org/10.22323/1.358.0038Test
https://hal.science/hal-02973170Test

المؤلفون: David Maurin, Julien Lavalle, Laurent Derome, Pasquale D. Serpico, Pierre Salati, Yoann Génolini, Mathieu Boudaud

المساهمون: Laboratoire de Physique Théorique et Hautes Energies (LPTHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS), Service de Physique Théorique [Bruxelles] (SPT-ULB), Université libre de Bruxelles (ULB), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Laboratoire Univers et Particules de Montpellier (LUPM), Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Montpellier 2 - Sciences et Techniques (UM2), IFAC, Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Montpellier 2 - Sciences et Techniques (UM2)-Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Montpellier 2 - Sciences et Techniques (UM2), Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), ANR-18-CE31-0006,GaDaMa,Matière Noire Galactique(2018), European Project: 690575,H2020,H2020-MSCA-RISE-2015,InvisiblesPlus(2016), European Project: 674896,H2020,H2020-MSCA-ITN-2015,ELUSIVES(2016), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS)

المصدر: Physical Review Research
Physical Review Research, American Physical Society, 2020, 2, pp.023022. ⟨10.1103/PhysRevResearch.2.023022⟩
Physical Review Research, 2020, 2 (2), pp.023022. ⟨10.1103/PhysRevResearch.2.023022⟩
Physical Review Research, 2 (2
PoS
36th International Cosmic Ray Conference
36th International Cosmic Ray Conference, Jul 2019, Madison, United States. pp.038, ⟨10.22323/1.358.0038⟩

مصطلحات موضوعية: Systematic error, Particle physics, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astrophysics::High Energy Astrophysical Phenomena, Dark matter, Flux, FOS: Physical sciences, Improved method, Cosmic ray, Galactic cosmic rays, 01 natural sciences, Nuclear physics, High-energy astrophysicsGalactic cosmic raysDark matter, High Energy Physics - Phenomenology (hep-ph), Consistency (statistics), 0103 physical sciences, Range (statistics), 010306 general physics, 010302 applied physics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), anti-p: secondary, 010308 nuclear & particles physics, Covariance matrix, anti-p: flux, Généralités, 3. Good health, High-energy astrophysics, High Energy Physics - Phenomenology, [PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA], cosmic radiation, Antiproton, correlation, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Communication channel

وصف الملف: 1 full-text file(s): application/pdf

الوصول الحر: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::49231634c720d8835097819a332ca1e3Test
https://hal.archives-ouvertes.fr/hal-02157654Test

المؤلفون: Cuoco, Alessandro, Heisig, Jan, Klamt, Lukas, Korsmeier, Michael, Krämer, Michael

المساهمون: Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS)

المصدر: ISSN: 1550-7998.

مصطلحات موضوعية: Astrophysics and astroparticle physics, dark matter: potential, anti-p: cosmic radiation, anti-p: secondary, cosmic radiation: secondary, cosmic radiation: spectrum, anti-p: production, correlation, propagation, covariance, antimatter, benchmark, nucleus, AMS, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]

العلاقة: info:eu-repo/semantics/altIdentifier/arxiv/1903.01472; hal-02073493; https://hal.science/hal-02073493Test; ARXIV: 1903.01472; INSPIRE: 1723718

الإتاحة: https://doi.org/10.1103/PhysRevD.99.103014Test
https://hal.science/hal-02073493Test