Sökning: onr:"swepub:oai:DiVA.org:su-130872" > Search for Spectral...
Fältnamn | Indikatorer | Metadata |
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000 | 06403naa a2201561 4500 | |
001 | oai:DiVA.org:su-130872 | |
003 | SwePub | |
008 | 160607s2016 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:kth-187721 | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1308722 URI |
024 | 7 | a https://doi.org/10.1103/PhysRevLett.116.1611012 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-1877212 URI |
040 | a (SwePub)sud (SwePub)kth | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Ajello, M.4 aut |
245 | 1 0 | a Search for Spectral Irregularities due to Photon-Axionlike-Particle Oscillations with the Fermi Large Area Telescope |
264 | 1 | b American Physical Society,c 2016 |
338 | a print2 rdacarrier | |
500 | a Funding Details: NASA, National Aeronautics and Space AdministrationQC 20160527 | |
520 | a We report on the search for spectral irregularities induced by oscillations between photons and axionlike-particles (ALPs) in the gamma-ray spectrum of NGC 1275, the central galaxy of the Perseus cluster. Using 6 years of Fermi Large Area Telescope data, we find no evidence for ALPs and exclude couplings above 5 x 10(-12) GeV-1 for ALP masses 0.5 less than or similar to m(a) less than or similar to 5 neV at 95% confidence. The limits are competitive with the sensitivity of planned laboratory experiments, and, together with other bounds, strongly constrain the possibility that ALPs can reduce the gamma-ray opacity of the Universe. | |
650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
653 | a Photons | |
700 | 1 | a Albert, A.4 aut |
700 | 1 | a Anderson, Brandonu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)braan |
700 | 1 | a Baldini, L.4 aut |
700 | 1 | a Barbiellini, G.4 aut |
700 | 1 | a Bastieri, D.4 aut |
700 | 1 | a Bellazzini, R.4 aut |
700 | 1 | a Bissaldi, E.4 aut |
700 | 1 | a Blandford, R. D.4 aut |
700 | 1 | a Bloom, E. D.4 aut |
700 | 1 | a Bonino, R.4 aut |
700 | 1 | a Bottacini, E.4 aut |
700 | 1 | a Bregeon, J.4 aut |
700 | 1 | a Bruel, P.4 aut |
700 | 1 | a Buehler, R.4 aut |
700 | 1 | a Caliandro, G. A.4 aut |
700 | 1 | a Cameron, R. A.4 aut |
700 | 1 | a Caragiulo, M.4 aut |
700 | 1 | a Caraveo, P. A.4 aut |
700 | 1 | a Cecchi, C.4 aut |
700 | 1 | a Chekhtman, A.4 aut |
700 | 1 | a Ciprini, S.4 aut |
700 | 1 | a Cohen-Tanugi, J.4 aut |
700 | 1 | a Conrad, Janu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)conrad |
700 | 1 | a Costanza, F.4 aut |
700 | 1 | a D'Ammando, F.4 aut |
700 | 1 | a de Angelis, A.4 aut |
700 | 1 | a de Palma, F.4 aut |
700 | 1 | a Desiante, R.4 aut |
700 | 1 | a Meyer, Manuelu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)mmanu |
700 | 1 | a Li, L.u KTH,Partikel- och astropartikelfysik,Oskar Klein Centre for Cosmoparticle Physics, Sweden4 aut0 (Swepub:kth)- |
700 | 1 | a Dominguez, A.4 aut |
700 | 1 | a Drell, P. S.4 aut |
700 | 1 | a Favuzzi, C.4 aut |
700 | 1 | a Focke, W. B.4 aut |
700 | 1 | a Franckowiak, A.4 aut |
700 | 1 | a Fukazawa, Y.4 aut |
700 | 1 | a Funk, S.4 aut |
700 | 1 | a Fusco, P.4 aut |
700 | 1 | a Gargano, F.4 aut |
700 | 1 | a Gasparrini, D.4 aut |
700 | 1 | a Giglietto, N.4 aut |
700 | 1 | a Glanzman, T.4 aut |
700 | 1 | a Godfrey, G.4 aut |
700 | 1 | a Guiriec, S.4 aut |
700 | 1 | a Horan, D.4 aut |
700 | 1 | a Johannesson, G.4 aut |
700 | 1 | a Katsuragawa, M.4 aut |
700 | 1 | a Kensei, S.4 aut |
700 | 1 | a Kuss, M.4 aut |
700 | 1 | a Larsson, Stefanu KTH,Partikel- och astropartikelfysik,Oskar Klein Centre for Cosmoparticle Physics, Sweden4 aut0 (Swepub:kth)u1xfjjbn |
700 | 1 | a Latronico, L.4 aut |
700 | 1 | a Li, J.4 aut |
700 | 1 | a Li, L.4 aut |
700 | 1 | a Longo, F.4 aut |
700 | 1 | a Loparco, F.4 aut |
700 | 1 | a Lubrano, P.4 aut |
700 | 1 | a Madejski, G. M.4 aut |
700 | 1 | a Maldera, S.4 aut |
700 | 1 | a Manfreda, A.4 aut |
700 | 1 | a Mayer, M.4 aut |
700 | 1 | a Mazziotta, M. N.4 aut |
700 | 1 | a Meyer, Manuelu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)mmanu |
700 | 1 | a Michelson, P. F.4 aut |
700 | 1 | a Mirabal, N.4 aut |
700 | 1 | a Mizuno, T.4 aut |
700 | 1 | a Monzani, M. E.4 aut |
700 | 1 | a Morselli, A.4 aut |
700 | 1 | a Moskalenko, I. V.4 aut |
700 | 1 | a Murgia, S.4 aut |
700 | 1 | a Negro, M.4 aut |
700 | 1 | a Nuss, E.4 aut |
700 | 1 | a Okada, C.4 aut |
700 | 1 | a Orlando, E.4 aut |
700 | 1 | a Ormes, J. F.4 aut |
700 | 1 | a Paneque, D.4 aut |
700 | 1 | a Perkins, J. S.4 aut |
700 | 1 | a Pesce-Rollins, M.4 aut |
700 | 1 | a Piron, F.4 aut |
700 | 1 | a Pivato, G.4 aut |
700 | 1 | a Porter, T. A.4 aut |
700 | 1 | a Raino, S.4 aut |
700 | 1 | a Rando, R.4 aut |
700 | 1 | a Razzano, M.4 aut |
700 | 1 | a Reimer, A.4 aut |
700 | 1 | a Sanchez-Conde, Miguelu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)msanc |
700 | 1 | a Sgro, C.4 aut |
700 | 1 | a Simone, D.4 aut |
700 | 1 | a Siskind, E. J.4 aut |
700 | 1 | a Spada, F.4 aut |
700 | 1 | a Spandre, G.4 aut |
700 | 1 | a Spinelli, P.4 aut |
700 | 1 | a Takahashi, H.4 aut |
700 | 1 | a Thayer, J. B.4 aut |
700 | 1 | a Torres, D. F.4 aut |
700 | 1 | a Tosti, G.4 aut |
700 | 1 | a Troja, E.4 aut |
700 | 1 | a Uchiyama, Y.4 aut |
700 | 1 | a Wood, K. S.4 aut |
700 | 1 | a Wood, M.4 aut |
700 | 1 | a Zaharijas, G.4 aut |
700 | 1 | a Zimmer, Stephanu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)stzi0820 |
710 | 2 | a Stockholms universitetb Fysikum4 org |
773 | 0 | t Physical Review Lettersd : American Physical Societyg 116:16q 116:16x 0031-9007x 1079-7114 |
856 | 4 | u https://doi.org/10.1103/PhysRevLett.116.161101y Fulltext |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-130872 |
856 | 4 8 | u https://doi.org/10.1103/PhysRevLett.116.161101 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-187721 |
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