Sökning: WFRF:(Vorster M) > (2010-2014) > Constraints on axio...
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001 | oai:DiVA.org:su-97631 | |
003 | SwePub | |
008 | 131216s2013 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:lnu-33166 | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-976312 URI |
024 | 7 | a https://doi.org/10.1103/PhysRevD.88.1020032 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:lnu:diva-331662 URI |
040 | a (SwePub)sud (SwePub)lnu | |
041 | a engb eng | |
042 | 9 SwePub | |
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100 | 1 | a Abramowski, A.4 aut |
245 | 1 0 | a Constraints on axionlike particles with HESS from the irregularity of the PKS 2155-304 energy spectrum |
264 | 1 | c 2013 |
338 | a print2 rdacarrier | |
500 | a AuthorCount:214; | |
520 | a Axionlike particles (ALPs) are hypothetical light (sub-eV) bosons predicted in some extensions of the Standard Model of particle physics. In astrophysical environments comprising high-energy gamma rays and turbulent magnetic fields, the existence of ALPs can modify the energy spectrum of the gamma rays for a sufficiently large coupling between ALPs and photons. This modification would take the form of an irregular behavior of the energy spectrum in a limited energy range. Data from the H. E. S. S. observations of the distant BL Lac object PKS 2155 - 304 (z = 0.116) are used to derive upper limits at the 95% C. L. on the strength of the ALP coupling to photons, g(gamma a) < 2.1 x 10(-11) GeV-1 for an ALP mass between 15 and 60 neV. The results depend on assumptions on the magnetic field around the source, which are chosen conservatively. The derived constraints apply to both light pseudoscalar and scalar bosons that couple to the electromagnetic field. | |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
653 | a Astroparticle Physics | |
700 | 1 | a Acero, F.4 aut |
700 | 1 | a Aharonian, F.4 aut |
700 | 1 | a Benkhali, F. Ait4 aut |
700 | 1 | a Akhperjanian, A. G.4 aut |
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700 | 1 | a Balenderan, S.4 aut |
700 | 1 | a Balzer, A.4 aut |
700 | 1 | a Barnacka, A.4 aut |
700 | 1 | a Becherini, Yvonneu Universität Heidelberg, Germany;Universite ́ Paris Diderot, France;Ecole Polytechnique, France4 aut0 (Swepub:lnu)yvbeaa |
700 | 1 | a Tjus, J. Becker4 aut |
700 | 1 | a Bernloehr, K.4 aut |
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700 | 1 | a Punch, Michaelu Univ Paris Diderot, APC, AstroParticule & Cosmology, CNRS,IN2P3,CEA,Irfu, Observ Paris,Sorbonne Paris C, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France4 aut0 (Swepub:lnu)mipuaa |
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710 | 2 | a Universität Heidelberg, Germany;Universite ́ Paris Diderot, France;Ecole Polytechnique, Franceb Univ Paris Diderot, APC, AstroParticule & Cosmology, CNRS,IN2P3,CEA,Irfu, Observ Paris,Sorbonne Paris C, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France4 org |
773 | 0 | t Physical Review Dg 88:10, s. 102003-q 88:10<102003-x 1550-7998x 1550-2368 |
856 | 4 | u https://arxiv.org/abs/1311.3148y arXiv:1311.3148 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-97631 |
856 | 4 8 | u https://doi.org/10.1103/PhysRevD.88.102003 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:lnu:diva-33166 |
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