Sökning: onr:"swepub:oai:DiVA.org:su-146992" > Effective field the...
Fältnamn | Indikatorer | Metadata |
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000 | 06433naa a2201681 4500 | |
001 | oai:DiVA.org:su-146992 | |
003 | SwePub | |
008 | 170918s2017 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1469922 URI |
024 | 7 | a https://doi.org/10.1103/PhysRevD.96.0420042 DOI |
040 | a (SwePub)su | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Aprile, E.4 aut |
245 | 1 0 | a Effective field theory search for high-energy nuclear recoils using the XENON100 dark matter detector |
264 | 1 | c 2017 |
338 | a print2 rdacarrier | |
520 | a We report on weakly interacting massive particles (WIMPs) search results in the XENON100 detector using a nonrelativistic effective field theory approach. The data from science run II (34 kg x 224.6 live days) were reanalyzed, with an increased recoil energy interval compared to previous analyses, ranging from (6.6-240) keV(nr). The data are found to be compatible with the background-only hypothesis. We present 90% confidence level exclusion limits on the coupling constants of WIMP-nucleon effective operators using a binned profile likelihood method. We also consider the case of inelastic WIMP scattering, where incident WIMPs may up-scatter to a higher mass state, and set exclusion limits on this model as well. | |
650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
700 | 1 | a Aalbers, J.4 aut |
700 | 1 | a Agostini, F.4 aut |
700 | 1 | a Alfonsi, M.4 aut |
700 | 1 | a Amaro, F. D.4 aut |
700 | 1 | a Anthony, M.4 aut |
700 | 1 | a Arneodo, F.4 aut |
700 | 1 | a Barrow, P.4 aut |
700 | 1 | a Baudis, L.4 aut |
700 | 1 | a Bauermeister, Borisu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)bobau |
700 | 1 | a Benabderrahmane, M. L.4 aut |
700 | 1 | a Berger, T.4 aut |
700 | 1 | a Breur, P. A.4 aut |
700 | 1 | a Brown, A.4 aut |
700 | 1 | a Brown, E.4 aut |
700 | 1 | a Bruenner, S.4 aut |
700 | 1 | a Bruno, G.4 aut |
700 | 1 | a Budnik, R.4 aut |
700 | 1 | a Buetikofer, L.4 aut |
700 | 1 | a Calvén, Jakobu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)jaca6702 |
700 | 1 | a Cardoso, J. M. R.4 aut |
700 | 1 | a Cervantes, M.4 aut |
700 | 1 | a Cichon, D.4 aut |
700 | 1 | a Coderre, D.4 aut |
700 | 1 | a Colijn, A. P.4 aut |
700 | 1 | a Conrad, Janu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)conrad |
700 | 1 | a Cussonneau, J. P.4 aut |
700 | 1 | a Decowski, M. P.4 aut |
700 | 1 | a de Perio, P.4 aut |
700 | 1 | a Di Gangi, P.4 aut |
700 | 1 | a Di Giovanni, A.4 aut |
700 | 1 | a Diglio, S.4 aut |
700 | 1 | a Eurin, G.4 aut |
700 | 1 | a Fei, J.4 aut |
700 | 1 | a Ferella, Alfredo D.u Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)afere |
700 | 1 | a Fieguth, A.4 aut |
700 | 1 | a Fulgione, W.4 aut |
700 | 1 | a Rosso, A. Gallo4 aut |
700 | 1 | a Di Galloway, A.4 aut |
700 | 1 | a Gao, F.4 aut |
700 | 1 | a Garbini, M.4 aut |
700 | 1 | a Geis, C.4 aut |
700 | 1 | a Goetzke, L. W.4 aut |
700 | 1 | a Greene, Z.4 aut |
700 | 1 | a Grignon, C.4 aut |
700 | 1 | a Hasterok, C.4 aut |
700 | 1 | a Hogenbirk, E.4 aut |
700 | 1 | a Itay, R.4 aut |
700 | 1 | a Kaminsky, B.4 aut |
700 | 1 | a Kazama, S.4 aut |
700 | 1 | a Kessler, G.4 aut |
700 | 1 | a Kish, A.4 aut |
700 | 1 | a Landsman, H.4 aut |
700 | 1 | a Lang, R. F.4 aut |
700 | 1 | a Lellouch, D.4 aut |
700 | 1 | a Levinson, L.4 aut |
700 | 1 | a Lin, Q.4 aut |
700 | 1 | a Lindemann, S.4 aut |
700 | 1 | a Lindner, M.4 aut |
700 | 1 | a Lombardi, F.4 aut |
700 | 1 | a Lopes, J. A. M.4 aut |
700 | 1 | a Manfredini, A.4 aut |
700 | 1 | a Maris, I.4 aut |
700 | 1 | a Undagoitia, T. Marrodan4 aut |
700 | 1 | a Masbou, J.4 aut |
700 | 1 | a Massoli, F. V.4 aut |
700 | 1 | a Masson, D.4 aut |
700 | 1 | a Mayani, D.4 aut |
700 | 1 | a Messina, M.4 aut |
700 | 1 | a Micheneau, K.4 aut |
700 | 1 | a Molinario, A.4 aut |
700 | 1 | a Morå, Knutu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)kdund |
700 | 1 | a Murra, M.4 aut |
700 | 1 | a Naganoma, J.4 aut |
700 | 1 | a Ni, K.4 aut |
700 | 1 | a Oberlack, U.4 aut |
700 | 1 | a Pakarha, P.4 aut |
700 | 1 | a Pelssers, Bartu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)bpels |
700 | 1 | a Persiani, R.4 aut |
700 | 1 | a Piastra, F.4 aut |
700 | 1 | a Pienaar, J.4 aut |
700 | 1 | a Pizzella, V.4 aut |
700 | 1 | a Piro, M. -C.4 aut |
700 | 1 | a Plante, G.4 aut |
700 | 1 | a Priel, N.4 aut |
700 | 1 | a Rauch, L.4 aut |
700 | 1 | a Reichard, S.4 aut |
700 | 1 | a Reuter, C.4 aut |
700 | 1 | a Rizzo, A.4 aut |
700 | 1 | a Rosendahl, S.4 aut |
700 | 1 | a Rupp, N.4 aut |
700 | 1 | a dos Santos, J. M. F.4 aut |
700 | 1 | a Sartorelli, G.4 aut |
700 | 1 | a Scheibelhut, M.4 aut |
700 | 1 | a Schindler, S.4 aut |
700 | 1 | a Schreiner, J.4 aut |
700 | 1 | a Schumann, M.4 aut |
700 | 1 | a Lavina, L. Scotto4 aut |
700 | 1 | a Selvi, M.4 aut |
700 | 1 | a Shagin, P.4 aut |
700 | 1 | a Silva, M.4 aut |
700 | 1 | a Simgen, H.4 aut |
700 | 1 | a Sivers, M. V.4 aut |
700 | 1 | a Stein, A.4 aut |
700 | 1 | a Thers, D.4 aut |
700 | 1 | a Tiseni, A.4 aut |
700 | 1 | a Trinchero, G.4 aut |
700 | 1 | a Tunnell, C.4 aut |
700 | 1 | a Vargas, M.4 aut |
700 | 1 | a Wang, H.4 aut |
700 | 1 | a Wang, Z.4 aut |
700 | 1 | a Wei, Y.4 aut |
700 | 1 | a Weinheimer, C.4 aut |
700 | 1 | a Wulf, J.4 aut |
700 | 1 | a Ye, J.4 aut |
700 | 1 | a Zhang, Y.4 aut |
700 | 1 | a Farmer, Benjaminu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)bfarm |
710 | 2 | a Stockholms universitetb Fysikum4 org |
773 | 0 | t Physical Review Dg 96:4q 96:4x 2470-0010x 2470-0029 |
856 | 4 | u https://doi.org/10.1103/PhysRevD.96.042004y Fulltext |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-146992 |
856 | 4 8 | u https://doi.org/10.1103/PhysRevD.96.042004 |
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