Search for Electronic Recoil Event Rate Modulation with 4 Years of XENON100 Data - PubMed

Search for Event Rate Modulation in XENON100 Electronic Recoil Data.

Aprile E, Aalbers J, Agostini F, Alfonsi M, Anthony M, Arazi L, Arisaka K, Arneodo F, Balan C, Barrow P, Baudis L, Bauermeister B, Breur PA, Brown A, Brown E, Bruenner S, Bruno G, Budnik R, Bütikofer L, Cardoso JM, Cervantes M, Coderre D, Colijn AP, Contreras H, Cussonneau JP, Decowski MP, de Perio P, Di Giovanni A, Duchovni E, Fattori S, Ferella AD, Fieguth A, Fulgione W, Gao F, Garbini M, Geis C, Goetzke LW, Grignon C, Gross E, Hampel W, Hasterok C, Itay R, Kaether F, Kaminsky B, Kessler G, Kish A, Landsman H, Lang RF, Le Calloch M, Lellouch D, Levinson L, Levy C, Lindemann S, Lindner M, Lopes JA, Lyashenko A, Macmullin S, Marrodán Undagoitia T, Masbou J, Massoli FV, Mayani D, Melgarejo Fernandez AJ, Meng Y, Messina M, Micheneau K, Miguez B, Molinario A, Murra M, Naganoma J, Ni K, Oberlack U, Orrigo SE, Pakarha P, Persiani R, Piastra F, Pienaar J, Plante G, Priel N, Rauch L, Reichard S, Reuter C, Rizzo A, Rosendahl S, Dos Santos JM, Sartorelli G, Schindler S, Schreiner J, Schumann M, Scotto Lavina L, Selvi M, Shagin P, Simgen H, Teymourian A, Thers D, Tiseni A, Trinchero G, Tunnell C, Wall R, Wang H, Weber M, Weinheimer C, Zhang Y; XENON Collaboration. Aprile E, et al. Phys Rev Lett. 2015 Aug 28;115(9):091302. doi: 10.1103/PhysRevLett.115.091302. Epub 2015 Aug 28. Phys Rev Lett. 2015. PMID: 26371638

ASTROPHYSICS. Exclusion of leptophilic dark matter models using XENON100 electronic recoil data.

XENON Collaboration. XENON Collaboration. Science. 2015 Aug 21;349(6250):851-4. doi: 10.1126/science.aab2069. Science. 2015. PMID: 26293959

Astrophysics-independent bounds on the annual modulation of dark matter signals.

Herrero-Garcia J, Schwetz T, Zupan J. Herrero-Garcia J, et al. Phys Rev Lett. 2012 Oct 5;109(14):141301. doi: 10.1103/PhysRevLett.109.141301. Epub 2012 Oct 4. Phys Rev Lett. 2012. PMID: 23083235

Dark matter results from 225 live days of XENON100 data.

Aprile E, Alfonsi M, Arisaka K, Arneodo F, Balan C, Baudis L, Bauermeister B, Behrens A, Beltrame P, Bokeloh K, Brown E, Bruno G, Budnik R, Cardoso JM, Chen WT, Choi B, Cline D, Colijn AP, Contreras H, Cussonneau JP, Decowski MP, Duchovni E, Fattori S, Ferella AD, Fulgione W, Gao F, Garbini M, Ghag C, Giboni KL, Goetzke LW, Grignon C, Gross E, Hampel W, Kaether F, Kish A, Lamblin J, Landsman H, Lang RF, Le Calloch M, Levy C, Lim KE, Lin Q, Lindemann S, Lindner M, Lopes JA, Lung K, Marrodán Undagoitia T, Massoli FV, Melgarejo Fernandez AJ, Meng Y, Molinario A, Nativ E, Ni K, Oberlack U, Orrigo SE, Pantic E, Persiani R, Plante G, Priel N, Rizzo A, Rosendahl S, dos Santos JM, Sartorelli G, Schreiner J, Schumann M, Scotto Lavina L, Scovell PR, Selvi M, Shagin P, Simgen H, Teymourian A, Thers D, Vitells O, Wang H, Weber M, Weinheimer C; XENON100 Collaboration. Aprile E, et al. Phys Rev Lett. 2012 Nov 2;109(18):181301. doi: 10.1103/PhysRevLett.109.181301. Epub 2012 Nov 2. Phys Rev Lett. 2012. PMID: 23215267