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1. Improved limits on dark matter annihilation in the Sun with the 79-string IceCube detector and implications for supersymmetry

Author: IceCube Collaboration, Aartsen, M. G., Abraham, K., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Altmann, D., Anderson, T., Ansseau, I., Anton, G., Archinger, M., Arguelles, C., Arlen, T. C., Auffenberg, J., Bai, X., Barwick, S. W., Baum, V., Bay, R., Beatty, J. J., Tjus, J. Becker, Becker, K. -H., Beiser, E., BenZvi, S., Berghaus, P., Berley, D., Bernardini, E., Bernhard, A., Besson, D. Z., Binder, G., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D. J., Bohm, C., Börner, M., Bos, F., Bose, D., Böser, S., Botner, O., Braun, J., Brayeur, L., Bretz, H. -P., Buzinsky, N., Casey, J., Casier, M., Cheung, E., Chirkin, D., Christov, A., Clark, K., Classen, L., Coenders, S., Collin, G. H., Conrad, J. M., Cowen, D. F., Silva, A. H. Cruz, Danninger, M., Daughhetee, J., Davis, J. C., Day, M., de André, J. P. A. M., De Clercq, C., Rosendo, E. del Pino, Dembinski, H., De Ridder, S., Desiati, P., de Vries, K. D., de Wasseige, G., de With, M., DeYoung, T., Díaz-Vélez, J. C., di Lorenzo, V., Dumm, J. P., Dunkman, M., Eberhardt, B., Edsjö, J., Ehrhardt, T., Eichmann, B., Euler, S., Evenson, P. A., Fahey, S., Fazely, A. R., Feintzeig, J., Felde, J., Filimonov, K., Finley, C., Flis, S., Fösig, C. -C., Fuchs, T., Gaisser, T. K., Gaior, R., Gallagher, J., Gerhardt, L., Ghorbani, K., Gier, D., Gladstone, L., Glagla, M., Glüsenkamp, T., Goldschmidt, A., Golup, G., Gonzalez, J. G., Góra, D., Grant, D., Griffith, Z., Groß, A., Ha, C., Haack, C., Ismail, A. Haj, Hallgren, A., Halzen, F., Hansen, E., Hansmann, B., Hanson, K., Hebecker, D., Heereman, D., Helbing, K., Hellauer, R., Hickford, S., Hignight, J., Hill, G. C., Hoffman, K. D., Hoffmann, R., Holzapfel, K., Homeier, A., Hoshina, K., Huang, F., Huber, M., Huelsnitz, W., Hulth, P. O., Hultqvist, K., In, S., Ishihara, A., Jacobi, E., Japaridze, G. S., Jeong, M., Jero, K., Jones, B. J. P., Jurkovic, M., Kappes, A., Karg, T., Karle, A., Katz, U., Kauer, M., Keivani, A., Kelley, J. L., Kemp, J., Kheirandish, A., Kiryluk, J., Klein, S. R., Kohnen, G., Koirala, R., Kolanoski, H., Konietz, R., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Krings, K., Kroll, G., Kroll, M., Krückl, G., Kunnen, J., Kurahashi, N., Kuwabara, T., Labare, M., Lanfranchi, J. L., Larson, M. J., Lesiak-Bzdak, M., Leuermann, M., Leuner, J., Lu, L., Lünemann, J., Madsen, J., Maggi, G., Mahn, K. B. M., Mandelartz, M., Maruyama, R., Mase, K., Matis, H. S., Maunu, R., McNally, F., Meagher, K., Medici, M., Meier, M., Meli, A., Menne, T., Merino, G., Meures, T., Miarecki, S., Middell, E., Mohrmann, L., Montaruli, T., Morse, R., Nahnhauer, R., Naumann, U., Neer, G., Niederhausen, H., Nowicki, S. C., Nygren, D. R., Pollmann, A. Obertacke, Olivas, A., Omairat, A., O'Murchadha, A., Palczewski, T., Pandya, H., Pankova, D. V., Paul, L., Pepper, J. A., Heros, C. Pérez de los, Pfendner, C., Pieloth, D., Pinat, E., Posselt, J., Price, P. B., Przybylski, G. T., Quinnan, M., Raab, C., Rädel, L., Rameez, M., Rawlins, K., Reimann, R., Relich, M., Resconi, E., Rhode, W., Richman, M., Richter, S., Riedel, B., Robertson, S., Rongen, M., Rott, C., Ruhe, T., Ryckbosch, D., Sabbatini, L., Sander, H. -G., Sandrock, A., Sandroos, J., Sarkar, S., Savage, C., Schatto, K., Schimp, M., Schlunder, P., Schmidt, T., Schoenen, S., Schöneberg, S., Schönwald, A., Schulte, L., Schumacher, L., Scott, P., Seckel, D., Seunarine, S., Silverwood, H., Soldin, D., Song, M., Spiczak, G. M., Spiering, C., Stahlberg, M., Stamatikos, M., Stanev, T., Stasik, A., Steuer, A., Stezelberger, T., Stokstad, R. G., Stößl, A., Ström, R., Strotjohann, N. L., Sullivan, G. W., Sutherland, M., Taavola, H., Taboada, I., Tatar, J., Ter-Antonyan, S., Terliuk, A., Tešić, G., Tilav, S., Toale, P. A., Tobin, M. N., Toscano, S., Tosi, D., Tselengidou, M., Turcati, A., Unger, E., Usner, M., Vallecorsa, S., Vandenbroucke, J., van Eijndhoven, N., Vanheule, S., van Santen, J., Veenkamp, J., Vehring, M., Voge, M., Vraeghe, M., Walck, C., Wallace, A., Wallraff, M., Wandkowsky, N., Weaver, Ch., Wendt, C., Westerhoff, S., Whelan, B. J., Wiebe, K., Wiebusch, C. H., Wille, L., Williams, D. R., Wills, L., Wissing, H., Wolf, M., Wood, T. R., Woschnagg, K., Xu, D. L., Xu, X. W., Xu, Y., Yanez, J. P., Yodh, G., Yoshida, S., and Zoll, M.
Subjects: High Energy Physics - Phenomenology, Astrophysics - Cosmology and Nongalactic Astrophysics, High Energy Physics - Experiment
Abstract: We present an improved event-level likelihood formalism for including neutrino telescope data in global fits to new physics. We derive limits on spin-dependent dark matter-proton scattering by employing the new formalism in a re-analysis of data from the 79-string IceCube search for dark matter annihilation in the Sun, including explicit energy information for each event. The new analysis excludes a number of models in the weak-scale minimal supersymmetric standard model (MSSM) for the first time. This work is accompanied by the public release of the 79-string IceCube data, as well as an associated computer code for applying the new likelihood to arbitrary dark matter models., Comment: 24 pages, 8 figs, 1 table. Contact authors: Pat Scott & Matthias Danninger. Likelihood tool available at http://nulike.hepforge.org. v2: small updates to address JCAP referee report
Published: 2016
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2. Improved limits on dark matter annihilation in the Sun with the 79-string IceCube detector and implications for supersymmetry

Author: Aartsen, MG, Abraham, K, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Altmann, D, Anderson, T, Ansseau, I, Anton, G, Archinger, M, Arguelles, C, Arlen, TC, Auffenberg, J, Bai, X, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Tjus, JB, Becker, KH, Beiser, E, Benzvi, S, Berghaus, P, Berley, D, Bernardini, E, Bernhard, A, Besson, DZ, Binder, G, Bindig, D, Bissok, M, Blaufuss, E, Blumenthal, J, Boersma, DJ, Bohm, C, Börner, M, Bos, F, Bose, D, Böser, S, Botner, O, Braun, J, Brayeur, L, Bretz, HP, Buzinsky, N, Casey, J, Casier, M, Cheung, E, Chirkin, D, Christov, A, Clark, K, Classen, L, Coenders, S, Collin, GH, Conrad, JM, Cowen, DF, Silva, AHC, Danninger, M, Daughhetee, J, Davis, JC, Day, M, De André, JPAM, Clercq, CD, Rosendo, EDP, Dembinski, H, Ridder, SD, Desiati, P, De Vries, KD, De Wasseige, G, De With, M, Deyoung, T, Díaz-Vélez, JC, Di Lorenzo, V, Dumm, JP, Dunkman, M, Eberhardt, B, Edsjö, J, Ehrhardt, T, Eichmann, B, Euler, S, Evenson, PA, Fahey, S, Fazely, AR, Feintzeig, J, Felde, J, Filimonov, K, Finley, C, Flis, S, Fösig, CC, Fuchs, T, Gaisser, TK, Gaior, R, Gallagher, J, Gerhardt, L, Ghorbani, K, Gier, D, Gladstone, L, Glagla, M, Glüsenkamp, T, and Goldschmidt, A
Subjects: dark matter experiments, dark matter theory, neutrino experiments, hep-ph, astro-ph.CO, hep-ex, Nuclear & Particles Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Atomic, Molecular, Nuclear, Particle and Plasma Physics
Abstract: We present an improved event-level likelihood formalism for including neutrino telescope data in global fits to new physics. We derive limits on spin-dependent dark matter-proton scattering by employing the new formalism in a re-analysis of data from the 79-string IceCube search for dark matter annihilation in the Sun, including explicit energy information for each event. The new analysis excludes a number of models in the weak-scale minimal supersymmetric standard model (MSSM) for the first time. This work is accompanied by the public release of the 79-string IceCube data, as well as an associated computer code for applying the new likelihood to arbitrary dark matter models.
Published: 2016

3. Use of event-level neutrino telescope data in global fits for theories of new physics

Author: Scott, P., Savage, C., Edsjö, J., Collaboration, the IceCube, Abbasi, R., Abdou, Y., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Altmann, D., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S. W., Baum, V., Bay, R., Beattie, K., Beatty, J. J., Bechet, S., Tjus, J. Becker, Becker, K. -H., Bell, M., Benabderrahmane, M. L., BenZvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D. Z., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D. J., Bohm, C., Bose, D., Böser, S., Botner, O., Brayeur, L., Brown, A. M., Bruijn, R., Brunner, J., Buitink, S., Caballero-Mora, K. S., Carson, M., Casey, J., Casier, M., Chirkin, D., Christy, B., Clevermann, F., Cohen, S., Cowen, D. F., Silva, A. H. Cruz, Danninger, M., Daughhetee, J., Davis, J. C., De Clercq, C., Descamps, F., Desiati, P., de Vries-Uiterweerd, G., DeYoung, T., Díaz-Vélez, J. C., Dreyer, J., Dumm, J. P., Dunkman, M., Eagan, R., Eisch, J., Ellsworth, R. W., Engdegård, O., Euler, S., Evenson, P. A., Fadiran, O., Fazely, A. R., Fedynitch, A., Feintzeig, J., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Flis, S., Franckowiak, A., Franke, R., Frantzen, K., Fuchs, T., Gaisser, T. K., Gallagher, J., Gerhardt, L., Gladstone, L., Glüsenkamp, T., Goldschmidt, A., Goodman, J. A., Góra, D., Grant, D., Groß, A., Grullon, S., Gurtner, M., Ha, C., Ismail, A. Haj, Hallgren, A., Halzen, F., Hanson, K., Heereman, D., Heimann, P., Heinen, D., Helbing, K., Hellauer, R., Hickford, S., Hill, G. C., Hoffman, K. D., Hoffmann, R., Homeier, A., Hoshina, K., Huelsnitz, W., Hulth, P. O., Hultqvist, K., Hussain, S., Ishihara, A., Jacobi, E., Jacobsen, J., Japaridze, G. S., Jlelati, O., Johansson, H., Kappes, A., Karg, T., Karle, A., Kiryluk, J., Kislat, F., Kläs, J., Klein, S. R., Köhne, J. -H., Kohnen, G., Kolanoski, H., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Krasberg, M., Kroll, G., Kunnen, J., Kurahashi, N., Kuwabara, T., Labare, M., Laihem, K., Landsman, H., Larson, M. J., Lauer, R., Lesiak-Bzdak, M., Lünemann, J., Madsen, J., Maruyama, R., Mase, K., Matis, H. S., McNally, F., Meagher, K., Merck, M., Mészáros, P., Meures, T., Miarecki, S., Middell, E., Milke, N., Miller, J., Mohrmann, L., Montaruli, T., Morse, R., Movit, S. M., Nahnhauer, R., Naumann, U., Nowicki, S. C., Nygren, D. R., Obertacke, A., Odrowski, S., Olivas, A., Olivo, M., O'Murchadha, A., Panknin, S., Paul, L., Pepper, J. A., Heros, C. Pérez de los, Pieloth, D., Pirk, N., Posselt, J., Price, P. B., Przybylski, G. T., Rädel, L., Rawlins, K., Redl, P., Resconi, E., Rhode, W., Ribordy, M., Richman, M., Riedel, B., Rodrigues, J. P., Rothmaier, F., Rott, C., Ruhe, T., Rutledge, D., Ruzybayev, B., Ryckbosch, D., Saba, S. M., Salameh, T., Sander, H. -G., Santander, M., Sarkar, S., Schatto, K., Scheel, M., Scheriau, F., Schmidt, T., Schmitz, M., Schoenen, S., Schöneberg, S., Schönherr, L., Schönwald, A., Schukraft, A., Schulte, L., Schulz, O., Seckel, D., Seo, S. H., Sestayo, Y., Seunarine, S., Smith, M. W. E., Soiron, M., Soldin, D., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stasik, A., Stezelberger, T., Stokstad, R. G., Stößl, A., Strahler, E. A., Ström, R., Sullivan, G. W., Taavola, H., Taboada, I., Tamburro, A., Ter-Antonyan, S., Tilav, S., Toale, P. A., Toscano, S., Usner, M., van Eijndhoven, N., van der Drift, D., Van Overloop, A., van Santen, J., Vehring, M., Voge, M., Walck, C., Waldenmaier, T., Wallraff, M., Walter, M., Wasserman, R., Weaver, Ch., Wendt, C., Westerhoff, S., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Williams, D. R., Wissing, H., Wolf, M., Wood, T. R., Woschnagg, K., Xu, C., Xu, D. L., Xu, X. W., Yanez, J. P., Yodh, G., Yoshida, S., Zarzhitsky, P., Ziemann, J., Zilles, A., and Zoll, M.
Subjects: High Energy Physics - Phenomenology, Astrophysics - Cosmology and Extragalactic Astrophysics, High Energy Physics - Experiment, Physics - Data Analysis, Statistics and Probability
Abstract: We present a fast likelihood method for including event-level neutrino telescope data in parameter explorations of theories for new physics, and announce its public release as part of DarkSUSY 5.0.6. Our construction includes both angular and spectral information about neutrino events, as well as their total number. We also present a corresponding measure for simple model exclusion, which can be used for single models without reference to the rest of a parameter space. We perform a number of supersymmetric parameter scans with IceCube data to illustrate the utility of the method: example global fits and a signal recovery in the constrained minimal supersymmetric standard model (CMSSM), and a model exclusion exercise in a 7-parameter phenomenological version of the MSSM. The final IceCube detector configuration will probe almost the entire focus-point region of the CMSSM, as well as a number of MSSM-7 models that will not otherwise be accessible to e.g. direct detection. Our method accurately recovers the mock signal, and provides tight constraints on model parameters and derived quantities. We show that the inclusion of spectral information significantly improves the accuracy of the recovery, providing motivation for its use in future IceCube analyses., Comment: 29 pages, 6 figures. v2 adds additional explanation in p-value derivation, matches version accepted for publication in JCAP
Published: 2012
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4. Les Houches 2011: Physics at TeV Colliders New Physics Working Group Report

Author: Brooijmans, G., Gripaios, B., Moortgat, F., Santiago, J., Skands, P., Vásquez, D. Albornoz, Allanach, B. C., Alloul, A., Arbey, A., Azatov, A., Baer, H., Balázs, C., Barr, A., Basso, L., Battaglia, M., Bechtle, P., Bélanger, G., Belyaev, A., Benslama, K., Bergström, L., Bharucha, A., Boehm, C., Bondarenko, M., Bondu, O., Boos, E., Boudjema, F., Bringmann, T., Brown, M., Bunichev, V., Calvet, S., Campanelli, M., Carmona, A., Cerdeño, D. G., Chala, M., Chivukula, R. S., Chowdhury, D., Christensen, N. D., Cirelli, M., Cox, S., Cranmer, K., Da Silva, J., Delahaye, T., De Roeck, A., Djouadi, A., Dobson, E., Dolan, M., Donato, F., La Rochelle, G. Drieu, Duda, G., Duhr, C., Dumont, B., Edsjö, J., Ellis, J., Evoli, C., Falkowski, A., Felcini, M., Fuks, B., Gabrielli, E., Gaggero, D., Gascon-Shotkin, S., Ghosh, D. K., Giammanco, A., Godbole, R. M., Gondolo, P., Goto, T., Grasso, D., Gris, P., Guadagnoli, D., Gunion, J. F., Haisch, U., Hartgring, L., Heinemeyer, S., Hirsch, M., Hewett, J., Ismail, A., Jeltema, T., Kadastik, M., Kakizaki, M., Kannike, K., Khalil, S., Kneur, J-L., Krämer, M., Kraml, S., Kreiss, S., Lavalle, J., Leane, R., Lykken, J., Maccione, L., Mahmoudi, F., Mangano, M., Martin, S. P., Maurin, D., Moreau, G., Moretti, S., Moskalenko, I., Moultaka, G., Muhlleitner, M., Niessen, I., O'Leary, B., Orlando, E., Panci, P., Polesello, G., Porod, W., Porter, T., Profumo, S., Prosper, H., Pukhov, A., Racioppi, A., Raidal, M., de Traubenberg, M. Rausch, Renaud, A., Reuter, J., Rizzo, T. G., Robens, T., Rodríguez-Marrero, A. Y., Salati, P., Savage, C., Scott, P., Sekmen, S., Semenov, A., Shan, C. -L., Shepherd-Themistocleous, C., Simmons, E. H., Slavich, P., Speckner, C., Staub, F., Strong, A., Taillet, R., Thomas, F. S., Thomas, M. C., Tomalin, I., Tytgat, M., Ughetto, M., Valéry, L., Walker, D. G. E., Weiler, A., West, S. M., White, C. D., Williams, A. J., Wingerter, A., Wymant, C., Yu, J. -H., Yuan, C. -P., and Zerwas, D.
Subjects: High Energy Physics - Phenomenology, High Energy Physics - Experiment
Abstract: We present the activities of the "New Physics" working group for the "Physics at TeV Colliders" workshop (Les Houches, France, 30 May-17 June, 2011). Our report includes new agreements on formats for interfaces between computational tools, new tool developments, important signatures for searches at the LHC, recommendations for presentation of LHC search results, as well as additional phenomenological studies., Comment: 243 pages, report of the Les Houches 2011 New Physics Group; fix three figures
Published: 2012

5. Limits on the WIMP-nucleon scattering cross-section from neutrino telescopes

Author: Wikström, G. and Edsjö, J.
Subjects: Astrophysics - Cosmology and Extragalactic Astrophysics
Abstract: Neutrino-telescopes like Super-Kamiokande and IceCube have started to explore the neutrino fluxes from WIMP annihilations in the Sun. The non-observation of a signal can put constraints on the WIMP properties. We here focus on the neutrino signal from WIMP annihilation in the Sun and show that under reasonable assumptions, the non-observation of a signal from IceCube puts a much tighter constraint on the spin-dependent WIMP-proton scattering cross-section than current direct detection experiments like COUPP and KIMS. For the spin-independent scattering cross-section, the limits from IceCube and current direct detection experiments like XENON10 and CDMS place similar constraints. We here go through the assumptions being made and the uncertainties that arise in converting from limits on the muon flux from the Sun to limits on the WIMP-proton cross-section, and present our results as easy to use conversion factors., Comment: 10 pages, 6 figures. Accepted for publication in JCAP
Published: 2009
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6. Les Houches 2011: Physics at TeV Colliders New Physics Working Group Report

Author: Brooijmans, G, Gripaios, B, Moortgat, F, Santiago, J, Skands, P, Vásquez, D Albornoz, Allanach, BC, Alloul, A, Arbey, A, Azatov, A, Baer, H, Balázs, C, Barr, A, Basso, L, Battaglia, M, Bechtle, P, Bélanger, G, Belyaev, A, Benslama, K, Bergström, L, Bharucha, A, Boehm, C, Bondarenko, M, Bondu, O, Boos, E, Boudjema, F, Bringmann, T, Brown, M, Bunichev, V, Calvet, S, Campanelli, M, Carmona, A, Cerdeño, DG, Chala, M, Chivukula, RS, Chowdhury, D, Christensen, ND, Cirelli, M, Cox, S, Cranmer, K, Silva, J Da, Delahaye, T, Roeck, A De, Djouadi, A, Dobson, E, Dolan, M, Donato, F, Rochelle, G Drieu La, Duda, G, Duhr, C, Dumont, B, Edsjö, J, Ellis, J, Evoli, C, Falkowski, A, Felcini, M, Fuks, B, Gabrielli, E, Gaggero, D, Gascon-Shotkin, S, Ghosh, DK, Giammanco, A, Godbole, RM, Gondolo, P, Goto, T, Grasso, D, Gris, P, Guadagnoli, D, Gunion, JF, Haisch, U, Hartgring, L, Heinemeyer, S, Hirsch, M, Hewett, J, Ismail, A, Jeltema, T, Kadastik, M, Kakizaki, M, Kannike, K, Khalil, S, Kneur, J-L, Krämer, M, Kraml, S, Kreiss, S, Lavalle, J, Leane, R, Lykken, J, Maccione, L, Mahmoudi, F, Mangano, M, Martin, SP, Maurin, D, Moreau, G, Moretti, S, Moskalenko, I, Moultaka, G, Muhlleitner, M, Niessen, I, O'Leary, B, and Orlando, E
Subjects: hep-ph, hep-ex
Abstract: We present the activities of the "New Physics" working group for the "Physicsat TeV Colliders" workshop (Les Houches, France, 30 May-17 June, 2011). Ourreport includes new agreements on formats for interfaces between computationaltools, new tool developments, important signatures for searches at the LHC,recommendations for presentation of LHC search results, as well as additionalphenomenological studies.
Published: 2012

7. Status of the Neutrino Telescope AMANDA: Monopoles and WIMPS : Presented by Wolfgang Rhode for the AMANDA Collaboration

Author: Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becker, K.-H., Bergström, L., Bertrand, D., Biron, A., Botner, O., Bouchta, A., Boyce, M. M., Carius, S., Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dailing, J., Dalberg, E., DeYoung, T., Desiati, P., Dewulf, J.-P., Doksus, P., Edsjö, J., Ekström, P., Feser, T., Gaug, M., Goldschmidt, A., Goobar, A., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., Hellwig, M., Hill, G. C., Hulth, P. O., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Lamoureux, J. I., Leich, H., Leuthold, M., Lindahl, P., Loaiza, P., Lowder, D. M., Ludvig, J., Madsen, J., Marciniewski, P., Matis, H. S., Miller, T. C., Minaeva, Y., Miočinović, P., Morse, R., Neunhöffer, T., Niessen, P., Nygren, D. R., Ogelman, H., Pérez de los Heros, C., Price, P. B., Rawlins, K., Rhode, W., Richter, S., Martino, J. Rodríguez, Romenesko, P., Ross, D., Rubinstein, H., Sander, H.-G., Scheider, T., Schmidt, T., Schneider, D., Schwarz, R., Silvestri, A., Smoot, G., Solarz, M., Spiczak, G. M., Spiering, C., Starinsky, N., Steele, D., Steffen, P., Stokstad, R. G., Streicher, O., Sudhoff, P., Taboada, I., Vander Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C. H., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., Young, S., and Klapdor-Kleingrothaus, H. V., editor
Published: 2001
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8. Long-lived stops in MSSM scenarios with a neutralino LSP

Author: Johansen, M., Edsjö, J., Hellman, S., and Milstead, D.
Published: 2010
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9. SUSY tools

Author: Boudjema, F., primary, Edsjö, J., additional, and Gondolo, P., additional
Published: 2010
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10. Indirect detection of WIMPs

Author: Edsjö, J.
Published: 2005
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11. Observation of high-energy neutrinos using Čerenkov detectors embedded deep in Antarctic ice

Author: Andrés, E., Askebjer, P., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becker, K.-H., Bergstrōm, L., Bertrand, D., Bierenbaum, D., Biron, A., Booth, J., Botner, O., Bouchta, A., Boyce, M. M., Carius, S., Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dailing, J., Dalberg, E., DeYoung, T., Desiati, P., Dewulf, J.-P., Doksus, P., Edsjö, J., Ekström, P., Erlandsson, B., Feser, T., Gaug, M., Goldschmidt, A., Goobar, A., Gray, L., Haase, H., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., He, Y. D., Hellwig, M., Heukenkamp, H., Hill, G. C., Hulth, P. O., Hundertmark, S., Jacobsen, J., Kandhadai, V., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Loaiza, P., Lowder, D. M., Ludvig, J., Madsen, J., Marciniewski, P., Matis, H. S., Mihalyi, A., Mikolajski, T., Miller, T. C., Minaeva, Y., Miočinović, P., Mock, P. C., Morse, R., Neunhöffer, T., Newcomer, F. M., Niessen, P., Nygren, D. R., Ögelman, H., Pérez de los Heros, C., Porrata, R., Price, P. B., Rawlins, K., Reed, C., Rhode, W., Richards, A., Richter, S., Martino, J. Rodríguez, Romenesko, P., Ross, D., Rubinstein, H., Sander, H.-G., Scheider, T., Schmidt, T., Schneider, D., Schneider, E., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G. M., Spiering, C., Starinsky, N., Steele, D., Steffen, P., Stokstad, R. G., Streicher, O., Sun, Q., Taboada, I., Thollander, L., Thon, T., Tilav, S., Usechak, N., Donckt, M. Vander, Walck, C., Weinheimer, C., Wiebusch, C. H., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., and Young, S.
Published: 2001

12. Search for supernova neutrino bursts with the AMANDA detector

Author: Ahrens, J., Bai, X., Barouch, G., Barwick, S.W., Bay, R.C., Becka, T., Becker, K.-H., Bertrand, D., Biron, A., Booth, J., Botner, O., Bouchta, A., Boyce, M.M., Carius, S., Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C.G.S., Cowen, D.F., Dalberg, E., DeYoung, T., Desiati, P., Dewulf, J.-P., Doksus, P., Edsjö, J., Ekström, P., Feser, T., Gaug, M., Goldschmidt, A., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., Hellwig, M., Heukenkamp, H., Hill, G.C., Hulth, P.O., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Lamoureux, J.I., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Loaiza, P., Lowder, D.M., Madsen, J., Marciniewski, P., Matis, H.S., Miller, T.C., Minaeva, Y., Miočinović, P., Mock, P.C., Morse, R., Neunhöffer, T., Niessen, P., Nygren, D.R., Ogelman, H., Pérez de los Heros, C., Porrata, R., Price, P.B., Rawlins, K., Reed, C., Rhode, W., Richter, S., Rodrı́guez Martino, J., Romenesko, P., Ross, D., Sander, H.-G., Schmidt, T., Schneider, D., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G.M., Spiering, C., Starinsky, N., Steele, D., Steffen, P., Stokstad, R.G., Streicher, O., Sudhoff, P., Taboada, I., Thollander, L., Thon, T., Tilav, S., Vander Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C.H., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., and Young, S.
Published: 2002
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13. Results from the AMANDA high energy neutrino detector

Author: Andres, E., Askebjer, P., Bai, X., Barouch, G., Barwick, S.W., Bay, R.C., Becker, K.-H., Bergström, L., Bertrand, D., Biron, A., Booth, J., Botner, O., Bouchta, A., Boyce, M.M., Carius, S., Chirkin, D., Conrad, J., Costa, C.G.S., Cowen, D.F., Dailing, J., Dalberg, E., DeYoung, T., Desiati, P., Dewulf, J.-P., Doksus, P., Edsjö, J., Ekström, P., Erlandsson, B., Feser, T., Gaug, M., Goldschmidt, A., Goobar, A., Haase, H., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., He, Y.D., Hellwig, M., Heukenkamp, H., Hill, G.C., Hulth, P.O., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Loaiza, P., Lowder, D.M., Ludvig, J., Madsen, J., Marciniewski, P., Matis, H., Mikolajski, T., Miller, T.C., Minaeva, Y., Miocinovic, P., Mock, P., Morse, R., Neunhöffer, T., Newcomer, F.M., Niessen, P., Nygren, D.R., Pérez de los Heros, C., Porrata, R., Price, P.B., Rawlins, K., Reed, C., Rhode, W., Richards, A., Richter, S., Rodriguez Martino, J., Romenesko, P., Ross, D., Rubinstein, H., Sander, H.-G., Scheider, T., Schmidt, T., Schneider, D., Schneider, E., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G., Spiering, C., Starinski, N., Steele, D., Steffen, P., Stokstad, R.G., Streicher, O., Sun, Q., Taboada, I., Thollander, L., Thon, T., Tilav, S., Vander Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C.H., Wischnewski, R., Woschnagg, K., Wu, W., Yodh, G., and Young, S.
Published: 2001
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14. The AMANDA neutrino telescope

Author: Andrés, E.C., Askebjer, P., Barwick, S.W., Bay, R.C., Bergström, L., Biron, A., Booth, J., Botner, O., Bouchta, A., Carius, S., Carlson, M., Chinowsky, W., Chirkin, D., Conrad, J., Costa, C.G.S., Cowen, D., Dalberg, E., DeYoung, T., Edsjö, J., Ekström, P., Goobar, A., Gray, L., Hallgren, A., Halzen, F., Hardtke, R., Hart, S., He, Y., de los Heros, C.P., Hill, G., Hulth, P.O., Hundertmark, S., Jacobsen, J., Jones, A., Kandhadai, V., Karle, A., Kim, J., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Loaiza, P., Lowder, D., Marciniewski, P., Miller, T.C., Miocinovic, P., Mock, P.C., Morse, R., Newcomer, M., Niessen, P., Nygren, D., Porrata, R., Potter, D., Price, P.B., Przybylski, G., Rhode, W., Richter, S., Rodriguez, J., Romenesko, P., Ross, D., Rubinstein, H., Schmidt, T., Schneider, E., Schwarz, R., Schwendicke, U., Smoot, G., Solarz, M., Sorin, V., Spiering, C., Steffen, P., Stokstad, R., Streicher, O., Taboada, I., Thon, T., Tilav, S., Walck, C., Wiebusch, C.H., Wischnewski, R., Woschnagg, K., Wu, W., Yodh, G., and Young, S.
Published: 1999
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15. Neutralino relic density including coannihilations

Author: Gondolo, P. and Edsjö, J.
Published: 1999
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16. Neutrinos from cosmic ray interactions in the Sun

Author: Edsjö, J., primary, Elevant, J., additional, Enberg, R., additional, and Niblaeus, C., additional
Published: 2017
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17. Limits to the muon flux from WIMP annihilation in the center of the Earth with the AMANDA detector

Author: Ahrens, J., Andrés, E., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becka, T., Becker, K.-H., Bertrand, D., Biron, A., Botner, O., Bouchta, A., Carius, S., Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dalberg, E., De Clercq, C., DeYoung, T., Desiati, P., Dewulf, J.-P., Doksus, P., Edsjö, J., Ekström, P., Feser, T., Gaisser, T. K., Gaug, M., Gerhardt, L., Goldschmidt, A., Goobar, A., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., Hauschildt, T., Hellwig, M., Hill, G. C., Hulth, P. O., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Lamoureux, J. I., Leich, H., Leuthold, M., Lindahl, P., Loaiza, P., Lowder, D. M., Ludvig, J., Madsen, J., Marciniewski, P., Matis, H. S., McParland, C. P., Miller, T. C., Minaeva, Y., Miočinović, P., Mock, P. C., Morse, R., Neunhöffer, T., Niessen, P., Nygren, D. R., Ogelman, H., Olbrechts, Ph., Pérez De Los Heros, C., Pohl, A., Porrata, R., Price, P. B., Przybylski, G. T., Rawlins, K., Rhode, W., Ribordy, M., Richter, S., Rodríguez Martino, J., Romenesko, P., Ross, D., Sander, H.-G., Schmidt, T., Schneider, D., Schneider, E., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G. M., Spiering, C., Steele, D., Steffen, P., Stokstad, R. G., Streicher, O., Sudhoff, P., Sulanke, K. H., Taboada, I., Thollander, L., Thon, T., Tilav, S., Vander Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C. H., Wiedemann, C., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., and Young, S.
Abstract: Physical review / D 66(3), 032006 (2002). doi:10.1103/PhysRevD.66.032006, Published by Inst., Woodbury, NY
Published: 2002
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18. Observation of high energy atmospheric neutrinos with the Antarctic muon and neutrino detector array

Author: Ahrens, J., Andrés, E., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becka, T., Becker, K.-H., Bertrand, D., Binon, F., Biron, A., Booth, J., Botner, O., Bouchta, A., Bouhali, O., Boyce, M. M., Carius, S., Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dalberg, E., De Clercq, C., DeYoung, T., Desiati, P., Dewulf, J.-P., Doksus, P., Edsjö, J., Ekström, P., Feser, T., Frère, J.-M., Gaisser, T. K., Gaug, M., Goldschmidt, A., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., Hauschildt, T., Hellwig, M., Heukenkamp, H., Hill, G. C., Hulth, P. O., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Lamoureux, J. I., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Loaiza, P., Lowder, D. M., Madsen, J., Marciniewski, P., Matis, H. S., McParland, C. P., Miller, T. C., Minaeva, Y., Miočinović, P., Mock, P. C., Morse, R., Neunhöffer, T., Niessen, P., Nygren, D. R., Ögelman, H., Olbrechts, Ph., Pérez De Los Heros, C., Pohl, A. C., Porrata, R., Price, P. B., Przybylski, G. T., Rawlins, K., Reed, C., Rhode, W., Ribordy, M., Richter, S., Rodríguez Martino, J., Romenesko, P., Ross, D., Sander, H.-G., Schmidt, T., Schneider, D., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G. M., Spiering, C., Starinsky, N., Steele, D., Steffen, P., Stokstad, R. G., Streicher, O., Sudhoff, P., Sulanke, K.-H., Taboada, I., Thollander, L., Thon, T., Tilav, S., Vander Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C. H., Wiedeman, C., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., and Young, S.
Abstract: Physical review / D 66(1), 012005 (2002). doi:10.1103/PhysRevD.66.012005, Published by Inst., Woodbury, NY
Published: 2002
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19. Dark stars at the Galactic Centre : the main sequence

Author: Scott, P., Fairbairn, M., Edsjö, J., Scott, P., Fairbairn, M., and Edsjö, J.
Abstract: In regions of very high dark matter density such as the Galactic Centre, the capture and annihilation of WIMP dark matter by stars has the potential to significantly alter their evolution. We describe the dark stellar evolution code DarkStars, and present a series of detailed grids of WIMP-influenced stellar models for main-sequence stars. We describe the changes in stellar structure and main-sequence evolution which occur as a function of the rate of energy injection by WIMPs, for masses of 0.3–2.0 M⊙ and metallicities Z= 0.0003–0.02 . We show what rates of energy injection can be obtained using realistic orbital parameters for stars at the Galactic Centre, including detailed consideration of the velocity and density profiles of dark matter. Capture and annihilation rates are strongly boosted when stars follow elliptical rather than circular orbits. If there is a spike of dark matter induced by the supermassive black hole at the Galactic Centre, single solar mass stars following orbits with periods as long as 50 yr and eccentricities as low as 0.9 could be significantly affected. Binary systems with similar periods about the Galactic Centre could be affected on even less eccentric orbits. The most striking observational effect of this scenario would be the existence of a binary consisting of a low-mass protostar and a higher mass evolved star. The observation of low-mass stars and/or binaries on such orbits would either provide a detection of WIMP dark matter, or place stringent limits on the combination of the WIMP mass, spin-dependent nuclear-scattering cross-section, halo density and velocity distribution near the Galactic Centre. In some cases, the derived limits on the WIMP mass and spin-dependent nuclear-scattering cross-section would be of comparable sensitivity to current direct-detection experiments.
Published: 2009
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20. The zero age main sequence of WIMP burners

Author: Fairbairn, M., Scott, P., Edsjö, J., Fairbairn, M., Scott, P., and Edsjö, J.
Abstract: We modify a stellar structure code to estimate the effect upon the main sequence of the accretion of weakly-interacting dark matter onto stars and its subsequent annihilation. The effect upon the stars depends upon whether the energy generation rate from dark matter annihilation is large enough to shut off the nuclear burning in the star. Main sequence weakly-interacting massive particles (WIMP) burners look much like proto-stars moving on the Hayashi track, although they are in principle completely stable. We make some brief comments about where such stars could be found, how they might be observed and more detailed simulations which are currently in progress. Finally we comment on whether or not it is possible to link the paradoxically hot, young stars found at the galactic center with WIMP burners.
Published: 2008
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21. Cosmological wimps, higgs dark matter and GLAST

Author: Sellerholm, A., Conrad, Jan, Bergström, L., Edsjö, J., Sellerholm, A., Conrad, Jan, Bergström, L., and Edsjö, J.
Abstract: Measurement of the extragalactic background (EGBR) of diffuse gamma- rays is perhaps one of the most challenging tasks for future gamma- ray observatories, such as GLAST. This is because any determination will depend on accurate subtraction of the galactic diffuse and celestial foregrounds, as well as point sources. However, the EGBR is likely to contain very rich information about the high energy-gamma ray sources of the Universe at cosmological distances. We focus on the ability of GLAST to detect a signal from dark matter in the EGBR. We present sensitivities for generic thermal WIMPs and the Inert Higgs Doublet Model. Also we discuss the various aspects of astro- physics and particle physics that determines the shape and strength of the signal, such as dark matter halo properties and different dark matter candidates. Other possible sources to the EGBR are also discussed, such as unresolved AGNs, and viewed as backgrounds., QC 20141028
Published: 2007

22. GLAST sensitivity to cosmological dark matter annihilations into γ-rays

Author: Bergström, L., Conrad, Jan, Edsjö, J., Sellerholm, A., Bergström, L., Conrad, Jan, Edsjö, J., and Sellerholm, A.
Abstract: Pair annihilation of weakly interacting massive particle (WIMP) dark matter into high energy photons taking place in dark matter halos at all redshifts might contribute to the extragalactic diffuse gamma-ray radiation. The γ- annihilation channel would give rise to a distinct feature in the spectrum, a line which is distorted by the integration over all cosmological redshifts. We present a study of GLAST sensitivity to detect an extragalactic signal from a generic, thermal WIMP with a continuous spectrum part, modeled with annihilations into bb̄, and a γ-line, from the 2γ final state., QC 20141126
Published: 2007
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23. Is the dark matter interpretation of the EGRET gamma excess compatible with antiproton measurements?

Author: Bergström, L, Edsjö, J, Gustafsson, Michael, Salati, P, Bergström, L, Edsjö, J, Gustafsson, Michael, and Salati, P
Abstract: We investigate the internal consistency of the halo dark matter model which has been proposed by de Boer et al. to explain the excess of diffuse galactic gamma rays observed by the EGRET experiment. Any model based on dark matter annihilation into quark jets, such as the supersymmetric model proposed by de Boer et al., inevitably also predicts a primary flux of antiprotons from the same jets. Since propagation of the antiprotons in the unconventional, disk-dominated type of halo model used by de Boer et al. is strongly constrained by the measured ratio of boron to carbon nuclei in cosmic rays, we investigate the viability of the model using the DarkSUSY package to compute the gamma-ray and antiproton fluxes. We are able to show that their model is excluded by a wide margin from the measured flux of antiprotons. We therefore find that a model of the type suggested by Moskalenko et al., where the intensities of protons and electrons in the cosmic rays vary with galactic position, is far more plausible to explain the gamma excess.
Published: 2006

24. Use of event-level neutrino telescope data in global fits for theories of new physics

Author: Scott, P, primary, Savage, C, additional, Edsjö, J, additional, and collaboration, The IceCube, additional
Published: 2012
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25. Weakly interacting massive particle diffusion in the solar system including solar depletion and its effect on Earth capture

Author: Lundberg, J., Edsjö, J., Lundberg, J., and Edsjö, J.
Published: 2004

26. Search for point sources of high-energy neutrinos with AMANDA

Author: Ahrens, J., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becka, T., Becker, K. -H, Bertrand, D., Binon, F., Biron, A., Boeser, S., Botner, O., Bouchta, A., Bouhali, O., Burgess, T., Carius, Staffan, Castermans, T., Chirkin, D., Conrad, J., Cooley, J., Cowen, D. F., Davour, A., de Clercq, C., DeYoung, T., Desiati, P., Dewulf, J. -P, Doksus, P., Edsjö, J., Ekström, P., Feser, T., Gaisser, T. K., Gaug, M., Gerhardt, L., Goldschmidt, A., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., Hauschildt, T., Hellwig, M., Herquet, P., Hill, G. C., Hulth, P. O., Hultqvist, K., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Köpke, L., Kowalski, M., Kuehn, K., Lamoureux, J. I., Leich, H., Leuthold, M., Lindahl, P., Madsen, J., Marciniewski, P., Matis, H., McParland, C. P., Miller, T. C., Minaeva, Y., Miocinoví, P., Mock, P. C., Morse, R., Neunhöffer, T., Niessen, P., Nygren, D. R., Ögelman, H., Olbrechts, P., Pérez de los Heros, C., Pohl, A. C., Price, P. B., Przybylski, G. T., Rawlins, K., Resconi, E., Rhode, W., Ribordy, M., Richter, S., Rodríguez Martino, J., Romenesko, P., Ross, D., Sander, H. -G, Schmidt, T., Schneider, D., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G. M., Spiering, C., Steele, D., Steffen, P., Stokstad, R. G., Sulanke, K. -H, Taboada, I., Thollander, L., Tilav, S., Walck, C., Weinheimer, C., Wiebusch, C. H., Wiedemann, C., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., Young, S., Ahrens, J., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becka, T., Becker, K. -H, Bertrand, D., Binon, F., Biron, A., Boeser, S., Botner, O., Bouchta, A., Bouhali, O., Burgess, T., Carius, Staffan, Castermans, T., Chirkin, D., Conrad, J., Cooley, J., Cowen, D. F., Davour, A., de Clercq, C., DeYoung, T., Desiati, P., Dewulf, J. -P, Doksus, P., Edsjö, J., Ekström, P., Feser, T., Gaisser, T. K., Gaug, M., Gerhardt, L., Goldschmidt, A., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., Hauschildt, T., Hellwig, M., Herquet, P., Hill, G. C., Hulth, P. O., Hultqvist, K., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Köpke, L., Kowalski, M., Kuehn, K., Lamoureux, J. I., Leich, H., Leuthold, M., Lindahl, P., Madsen, J., Marciniewski, P., Matis, H., McParland, C. P., Miller, T. C., Minaeva, Y., Miocinoví, P., Mock, P. C., Morse, R., Neunhöffer, T., Niessen, P., Nygren, D. R., Ögelman, H., Olbrechts, P., Pérez de los Heros, C., Pohl, A. C., Price, P. B., Przybylski, G. T., Rawlins, K., Resconi, E., Rhode, W., Ribordy, M., Richter, S., Rodríguez Martino, J., Romenesko, P., Ross, D., Sander, H. -G, Schmidt, T., Schneider, D., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G. M., Spiering, C., Steele, D., Steffen, P., Stokstad, R. G., Sulanke, K. -H, Taboada, I., Thollander, L., Tilav, S., Walck, C., Weinheimer, C., Wiebusch, C. H., Wiedemann, C., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., and Young, S.
Abstract: This paper describes the search for astronomical sources of high-energy neutrinos using the AMANDA-B10 detector, an array of 302 photomultiplier tubes used for the detection of Cerenkov light from upward-traveling neutrino-induced muons, buried deep in ice at the South Pole. The absolute pointing accuracy and angular resolution were studied by using coincident events between the AMANDA detector and two independent telescopes on the surface, the GASP air Cerenkov telescope and the SPASE extensive air shower array. Using data collected from 1997 April to October (130.1 days of live time), a general survey of the northern hemisphere revealed no statistically significant excess of events from any direction. The sensitivity for a flux of muon neutrinos is based on the effective detection area for through-going muons. Averaged over the northern sky, the effective detection area exceeds 10,000 m2 for E μ ≈ 10 TeV. Neutrinos generated in the atmosphere by cosmic-ray interactions were used to verify the predicted performance of the detector. For a source with a differential energy spectrum proportional to Eν -2 and declination larger than +40°, we obtain E2(dNν/dE) ≤ 10-6 GeV cm-2 s-1 for an energy threshold of 10 GeV., Source: Scopus
Published: 2003
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27. Limits on the WIMP-nucleon scattering cross-section from neutrino telescopes

Author: Wikström, G, primary and Edsjö, J, additional
Published: 2009
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28. Physics results from the AMANDA neutrino detector

Author: Kowalski, Marek, Ahrens, J., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becka, T., Becker, K.-H., Bertrand, D., Biron, A., Böser, S., Booth, J., Botner, O., Bouchta, A., Boyce, M. M., Carius, Staffan, Chen, A., Chrikin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., De Clercq, C., DeYoung, T., Desiati, P., Dewulf, J.-P., Doksus, P., Edsjö, J., Ekström, P., Feser, T., Frère, J.-M., Gaug, M., Gerhardt, L., Goldschmidt, A., Hallgren, A., Halzen, F., Hansson, K., Hardtke, R., Hauschildt, T., Hellwig, M., Herquet, P., Hill, G. C., Hulth, P. O., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Kuehn, K., Lamoureux, J. I., Leich, H., Leuthold, M., Lindahl, P., Madsen, J., Maciniewski, P., Matis, H. S., Minaeva, Y., Mioncinovic, P., Morse, R., Neunhöffer, T., Niessen, P., Nygren, D. R., Ogelman, H., Olbechts, Ph., Péres de los Heros, C., Pohl, A., Price, P. B., Przybylski, G. T., Rawlins, K., Reed, C., Rhode, W., Ribordy, M., Richter, S., Rodrígiez Martino, J., Romenesko, P., Ross, D., Sander, H.-G., Schmidt, T., Schneider, D., Silvestri, A., Solarz, M., Spiczak, G. M., Spiering, C., Starinsky, N., Steele, D., Steffen, P., Stokstad, R. G., Sudhoff, P., Sulanke, K.-H., Taboda, I., Vander Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C. H., Wischnewski, R., Wissing, H., Woschnagg, K., Yodh, G., Young, S., Kowalski, Marek, Ahrens, J., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becka, T., Becker, K.-H., Bertrand, D., Biron, A., Böser, S., Booth, J., Botner, O., Bouchta, A., Boyce, M. M., Carius, Staffan, Chen, A., Chrikin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., De Clercq, C., DeYoung, T., Desiati, P., Dewulf, J.-P., Doksus, P., Edsjö, J., Ekström, P., Feser, T., Frère, J.-M., Gaug, M., Gerhardt, L., Goldschmidt, A., Hallgren, A., Halzen, F., Hansson, K., Hardtke, R., Hauschildt, T., Hellwig, M., Herquet, P., Hill, G. C., Hulth, P. O., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Kuehn, K., Lamoureux, J. I., Leich, H., Leuthold, M., Lindahl, P., Madsen, J., Maciniewski, P., Matis, H. S., Minaeva, Y., Mioncinovic, P., Morse, R., Neunhöffer, T., Niessen, P., Nygren, D. R., Ogelman, H., Olbechts, Ph., Péres de los Heros, C., Pohl, A., Price, P. B., Przybylski, G. T., Rawlins, K., Reed, C., Rhode, W., Ribordy, M., Richter, S., Rodrígiez Martino, J., Romenesko, P., Ross, D., Sander, H.-G., Schmidt, T., Schneider, D., Silvestri, A., Solarz, M., Spiczak, G. M., Spiering, C., Starinsky, N., Steele, D., Steffen, P., Stokstad, R. G., Sudhoff, P., Sulanke, K.-H., Taboda, I., Vander Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C. H., Wischnewski, R., Wissing, H., Woschnagg, K., Yodh, G., and Young, S.
Abstract: In the winter season of 2000, the AMANDA (Antarctic Muon And NeutrinoDetector Array) detector was completed to its nal state. We report on major physicsresults obtained from the AMANDA-B10 detector, as well as initial results of the fullAMANDA-II detector.
Published: 2001

29. Recent results from AMANDA

Author: Andrés, E., Askebjer, P., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becker, K. -H, Bergström, L., Bertrand, D., Bierenbaum, D., Biron, A., Booth, J., Botner, O., Bouchta, A., Boyce, M. M., Carius, Staffan, Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dailing, J., Dalberg, E., De Young, T., Desiati, P., Dewulf, J. -P, Doksus, P., Edsjö, J., Ekström, P., Erlandsson, B., Feser, T., Gaug, M., Goldschmidt, A., Goobar, A., Gray, L., Haase, H., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., He, Y. D., Hellwig, M., Heukenkamp, H., Hill, G. C., Hulth, P. O., Hundertmark, S., Jacobsen, J., Kandhadai, V., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Loaiza, P., Lowder, D. M., Ludvig, J., Madsen, J., Marciniewski, P., Matis, H. S., Mihalyi, A., Mikolajski, T., Miller, T. C., Minaeva, Y., Miočinović, P., Mock, P. C., Morse, R., Neunhöffer, T., Newcomer, F. M., Niessen, P., Nygren, D. R., Ogelman, H., Pérez De Los Heros, C., Porrata, R., Price, P. B., Rawlins, K., Reed, C., Rhode, W., Richards, A., Richter, S., Rodríguez Martino, J., Romenesko, P., Ross, D., Rubinstein, H., Sander, H. -G, Scheider, T., Schmidt, T., Schneider, D., Schneider, E., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G. M., Spiering, C., Starinsky, N., Steele, D., Steffen, P., Stokstad, R. G., Streicher, O., Sun, Q., Taboada, I., Thollander, L., Thon, T., Tilav, S., Usechak, N., Vander Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C. H., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., Young, S., Andrés, E., Askebjer, P., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becker, K. -H, Bergström, L., Bertrand, D., Bierenbaum, D., Biron, A., Booth, J., Botner, O., Bouchta, A., Boyce, M. M., Carius, Staffan, Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dailing, J., Dalberg, E., De Young, T., Desiati, P., Dewulf, J. -P, Doksus, P., Edsjö, J., Ekström, P., Erlandsson, B., Feser, T., Gaug, M., Goldschmidt, A., Goobar, A., Gray, L., Haase, H., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., He, Y. D., Hellwig, M., Heukenkamp, H., Hill, G. C., Hulth, P. O., Hundertmark, S., Jacobsen, J., Kandhadai, V., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Loaiza, P., Lowder, D. M., Ludvig, J., Madsen, J., Marciniewski, P., Matis, H. S., Mihalyi, A., Mikolajski, T., Miller, T. C., Minaeva, Y., Miočinović, P., Mock, P. C., Morse, R., Neunhöffer, T., Newcomer, F. M., Niessen, P., Nygren, D. R., Ogelman, H., Pérez De Los Heros, C., Porrata, R., Price, P. B., Rawlins, K., Reed, C., Rhode, W., Richards, A., Richter, S., Rodríguez Martino, J., Romenesko, P., Ross, D., Rubinstein, H., Sander, H. -G, Scheider, T., Schmidt, T., Schneider, D., Schneider, E., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G. M., Spiering, C., Starinsky, N., Steele, D., Steffen, P., Stokstad, R. G., Streicher, O., Sun, Q., Taboada, I., Thollander, L., Thon, T., Tilav, S., Usechak, N., Vander Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C. H., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., and Young, S.
Abstract: We present results based on data taken in 1997 with the 302-PMT Antarctic Muon and Neutrino Detector Array-B10 ("AMANDA-B10") array. Atmospheric neutrinos created in the northern hemisphere are observed indirectly through their charged current interactions which produce relativistic, Cherenkov-light-emitting upgoing muons in the South Pole ice cap. The reconstructed angular distribution of these events is in good agreement with expectation and demonstrates the viability of this ice-based device as a neutrino telescope., Source: Scopus
Published: 2001
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30. Search for supernova neutrino bursts with the AMANDA detector

Author: Ahrens, J., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becka, T., Becker, K. -H, Bertrand, D., Biron, A., Booth, J., Botner, O., Bouchta, A., Boyce, M. M., Carius, Staffan, Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dalberg, E., DeYoung, T., Desiati, P., Dewulf, J. -P, Doksus, P., Edsjö, J., Ekström, P., Feser, T., Gaug, M., Goldschmidt, A., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., Hellwig, M., Heukenkamp, H., Hill, G. C., Hulth, P. O., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Lamoureux, J. I., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Loaiza, P., Lowder, D. M., Madsen, J., Marciniewski, P., Matis, H. S., Miller, T. C., Minaeva, Y., Miočinović, P., Mock, P. C., Morse, R., Neunhöffer, T., Niessen, P., Nygren, D. R., Ogelman, H., Pérez de los Heros, C., Porrata, R., Price, P. B., Rawlins, K., Reed, C., Rhode, W., Richter, S., Rodríguez Martino, J., Romenesko, P., Ross, D., Sander, H. -G, Schmidt, T., Schneider, D., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G. M., Spiering, C., Starinsky, N., Steele, D., Steffen, P., Stokstad, R. G., Streicher, O., Sudhoff, P., Taboada, I., Thollander, L., Thon, T., Tilav, S., Vander Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C. H., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., Young, S., Ahrens, J., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becka, T., Becker, K. -H, Bertrand, D., Biron, A., Booth, J., Botner, O., Bouchta, A., Boyce, M. M., Carius, Staffan, Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dalberg, E., DeYoung, T., Desiati, P., Dewulf, J. -P, Doksus, P., Edsjö, J., Ekström, P., Feser, T., Gaug, M., Goldschmidt, A., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., Hellwig, M., Heukenkamp, H., Hill, G. C., Hulth, P. O., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Lamoureux, J. I., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Loaiza, P., Lowder, D. M., Madsen, J., Marciniewski, P., Matis, H. S., Miller, T. C., Minaeva, Y., Miočinović, P., Mock, P. C., Morse, R., Neunhöffer, T., Niessen, P., Nygren, D. R., Ogelman, H., Pérez de los Heros, C., Porrata, R., Price, P. B., Rawlins, K., Reed, C., Rhode, W., Richter, S., Rodríguez Martino, J., Romenesko, P., Ross, D., Sander, H. -G, Schmidt, T., Schneider, D., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G. M., Spiering, C., Starinsky, N., Steele, D., Steffen, P., Stokstad, R. G., Streicher, O., Sudhoff, P., Taboada, I., Thollander, L., Thon, T., Tilav, S., Vander Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C. H., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., and Young, S.
Abstract: The core collapse of a massive star in the Milky Way will produce a neutrino burst, intense enough to be detected by existing underground detectors. The AMANDA neutrino telescope located deep in the South Pole ice can detect MeV neutrinos by a collective rate increase in all photo-multipliers on top of dark noise. The main source of light comes from positrons produced in the CC reaction of anti-electron neutrinos on free protons ve + p → e+ + n. This paper describes the first supernova search performed on the full sets of data taken during 1997 and 1998 (215 days of live time) with 302 of the detector's optical modules. No candidate events resulted from this search. The performance of the detector is calculated, yielding a 70% coverage of the galaxy with one background fake per year with 90% efficiency for the detector configuration under study. An upper limit at the 90% c.l. on the rate of stellar collapses in the Milky Way is derived, yielding 4.3 events per year. A trigger algorithm is presented and its performance estimated. Possible improvements of the detector hardware are reviewed., Source: Scopus
Published: 2001
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31. Status of the Neutrino Telescope AMANDA : Monopoles and WIMPS

Author: Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becker, K. -H, Bergström, L., Bertrand, D., Biron, A., Botner, O., Bouchta, A., Boyce, M. M., Carius, Staffan, Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dailing, J., Dalberg, E., DeYoung, T., Desiati, P., Dewulf, J. -P, Doksus, P., Edsjö, J., Ekström, P., Feser, T., Gaug, M., Goldschmidt, A., Goobar, A., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., Hellwig, M., Hill, G. C., Hulth, P. O., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Lamoureux, J. I., Leich, H., Leuthold, M., Lindahl, P., Loaiza, P., Lowder, D. M., Ludvig, J., Madsen, J., Marciniewski, P., Matis, H. S., Miller, T. C., Minaeva, Y., Miočinović, P., Morse, R., Neunhöffer, T., Niessen, P., Nygren, D. R., Ogelman, H., Pérez de los Heros, C., Price, P. B., Rawlins, K., Rhode, W., Richter, S., Martino, J.Rodríguez, Romenesko, P., Ross, D., Rubinstein, H., Sander, H. -G, Scheider, T., Schmidt, T., Schneider, D., Schwarz, R., Silvestri, A., Smoot, G., Solarz, M., Spiczak, G. M., Spiering, C., Starinsky, N., Steele, D., Steffen, P., Stokstad, R. G., Streicher, O., Sudhoff, P., Taboada, I., Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C. H., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., Young, S., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becker, K. -H, Bergström, L., Bertrand, D., Biron, A., Botner, O., Bouchta, A., Boyce, M. M., Carius, Staffan, Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dailing, J., Dalberg, E., DeYoung, T., Desiati, P., Dewulf, J. -P, Doksus, P., Edsjö, J., Ekström, P., Feser, T., Gaug, M., Goldschmidt, A., Goobar, A., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., Hellwig, M., Hill, G. C., Hulth, P. O., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Lamoureux, J. I., Leich, H., Leuthold, M., Lindahl, P., Loaiza, P., Lowder, D. M., Ludvig, J., Madsen, J., Marciniewski, P., Matis, H. S., Miller, T. C., Minaeva, Y., Miočinović, P., Morse, R., Neunhöffer, T., Niessen, P., Nygren, D. R., Ogelman, H., Pérez de los Heros, C., Price, P. B., Rawlins, K., Rhode, W., Richter, S., Martino, J.Rodríguez, Romenesko, P., Ross, D., Rubinstein, H., Sander, H. -G, Scheider, T., Schmidt, T., Schneider, D., Schwarz, R., Silvestri, A., Smoot, G., Solarz, M., Spiczak, G. M., Spiering, C., Starinsky, N., Steele, D., Steffen, P., Stokstad, R. G., Streicher, O., Sudhoff, P., Taboada, I., Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C. H., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., and Young, S.
Abstract: The neutrino telescope AMANDA has been set up at the geographical South Pole as first step to a neutrino telescope of the scale of one cubic kilometer, which is the canonical size for a detector sensitive to neutrinos from Active Galactic Nuclei (AGN), Gamma Ray Bursts (GRB) and Topological Defects (TD). The location and depth in which the detector is installed is given by the requirement to detect neutrinos by the Cherenkov light produced by their reaction products and to keep the background due to atmospheric muons as small as possible. However, a detector optimized for this purpose is also capable to detect the bright Cherenkov light from relativistic Monopoles and neutrino signals from regions with high gravitational potential, where WIMPS are accumulated and possibly annihilate. Both hypothetical particles might contribute to the amount of dark matter. Therefore here a report about the status of the experiment (autumn 2000) and about the status of the search for these particles with the AMANDA B10 sub-detector is given.
Published: 2001
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32. Pre-launch estimates for GLAST sensitivity to dark matter annihilation signals

Author: Baltz, E A, primary, Berenji, B, additional, Bertone, G, additional, Bergström, L, additional, Bloom, E, additional, Bringmann, T, additional, Chiang, J, additional, Cohen-Tanugi, J, additional, Conrad, J, additional, Edmonds, Y, additional, Edsjö, J, additional, Godfrey, G, additional, Hughes, R E, additional, Johnson, R P, additional, Lionetto, A, additional, Moiseev, A A, additional, Morselli, A, additional, Moskalenko, I V, additional, Nuss, E, additional, Ormes, J F, additional, Rando, R, additional, Sander, A J, additional, Sellerholm, A, additional, Smith, P D, additional, Strong, A W, additional, Wai, L, additional, Wang, P, additional, and Winer, B L, additional
Published: 2008
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33. LOW MASS STELLAR EVOLUTION WITH WIMP CAPTURE AND ANNIHILATION

Author: SCOTT, P. C., primary, EDSJÖ, J., additional, and FAIRBAIRN, M., additional
Published: 2008
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34. Results from the AMANDA high energy neutrino detector

Author: Andres, E., Askebjer, P., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becker, K. -H, Bergström, L., Bertrand, D., Biron, A., Booth, J., Botner, O., Bouchta, A., Boyce, M. M., Carius, Staffan, Chirkin, D., Conrad, J., Costa, C. G. S., Cowen, D. F., Dailing, J., Dalberg, E., DeYoung, T., Desiati, P., Dewulf, J. -P, Doksus, P., Edsjö, J., Ekström, P., Erlandsson, B., Feser, T., Gaug, M., Goldschmidt, A., Goobar, A., Haase, H., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., He, Y. D., Hellwig, M., Heukenkamp, H., Hill, G. C., Hulth, P. O., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Loaiza, P., Lowder, D. M., Ludvig, J., Madsen, J., Marciniewski, P., Matis, H., Mikolajski, T., Miller, T. C., Minaeva, Y., Miocinovic, P., Mock, P., Morse, R., Neunhöffer, T., Newcomer, F. M., Niessen, P., Nygren, D. R., Pérez de los Heros, C., Porrata, R., Price, P. B., Rawlins, K., Reed, C., Rhode, W., Richards, A., Richter, S., Rodriguez Martino, J., Romenesko, P., Ross, D., Rubinstein, H., Sander, H. -G, Scheider, T., Schmidt, T., Schneider, D., Schneider, E., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G., Spiering, C., Starinski, N., Steele, D., Steffen, P., Stokstad, R. G., Streicher, O., Sun, Q., Taboada, I., Thollander, L., Thon, T., Tilav, S., Vander Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C. H., Wischnewski, R., Woschnagg, K., Wu, W., Yodh, G., Young, S., Andres, E., Askebjer, P., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becker, K. -H, Bergström, L., Bertrand, D., Biron, A., Booth, J., Botner, O., Bouchta, A., Boyce, M. M., Carius, Staffan, Chirkin, D., Conrad, J., Costa, C. G. S., Cowen, D. F., Dailing, J., Dalberg, E., DeYoung, T., Desiati, P., Dewulf, J. -P, Doksus, P., Edsjö, J., Ekström, P., Erlandsson, B., Feser, T., Gaug, M., Goldschmidt, A., Goobar, A., Haase, H., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., He, Y. D., Hellwig, M., Heukenkamp, H., Hill, G. C., Hulth, P. O., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Loaiza, P., Lowder, D. M., Ludvig, J., Madsen, J., Marciniewski, P., Matis, H., Mikolajski, T., Miller, T. C., Minaeva, Y., Miocinovic, P., Mock, P., Morse, R., Neunhöffer, T., Newcomer, F. M., Niessen, P., Nygren, D. R., Pérez de los Heros, C., Porrata, R., Price, P. B., Rawlins, K., Reed, C., Rhode, W., Richards, A., Richter, S., Rodriguez Martino, J., Romenesko, P., Ross, D., Rubinstein, H., Sander, H. -G, Scheider, T., Schmidt, T., Schneider, D., Schneider, E., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G., Spiering, C., Starinski, N., Steele, D., Steffen, P., Stokstad, R. G., Streicher, O., Sun, Q., Taboada, I., Thollander, L., Thon, T., Tilav, S., Vander Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C. H., Wischnewski, R., Woschnagg, K., Wu, W., Yodh, G., and Young, S.
Abstract: This paper briefly summarizes the search for astronomical sources of high-energy neutrinos using the AMANDA-B10 detector. The complete data set from 1997 was analyzed. For Eμ > 10 TeV, the detector exceeds 10,000 m2 in effective area between declinations of 25 and 90 degrees. Neutrinos generated in the atmosphere by cosmic ray interactions were used to verify the overall sensitivity of the detector. The absolute pointing accuracy and angular resolution has been confirmed by the analysis of coincident events between the SPASE air shower array and the AMANDA detector. Preliminary flux limits from point source candidates are presented. For declinations larger than +45 degrees, our results compare favorably to existing limits for sources in the Southern sky. We also present the current status of the searches for high energy neutrino emission from diffusely distributed sources, GRBs, and WIMPs from the center of the earth., Source: Scopus
Published: 2000
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35. The AMANDA neutrino detector : Status report

Author: Wischnewski, R., Andrés, E., Bai, X., Barouch, G., Barwick, S., Bay, R., Becker, K., Bergström, L., Bertrand, D., Besson, D., Biron, A., Booth, J., Botner, O., Bouchta, A., Carius, Staffan, Carlson, M., Chinowsky, W., Chirkin, D., Conrad, J., Cowen, D. F., Costa, C., Dalberg, E., Desiati, P., Dewulf, J., Deyoung, T., Doksus, P., Edsjö, J., Ekström, P., Feser, T., Frichter, G., Gaisser, T., Goldschmidt, A., Goobar, A., Hallgren, A., Halzen, F., Hardtke, R., Hellwig, M., Hill, G., Hulth, P., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Koepke, L., Kowalski, M., Kravchenko, I., Lamoureux, J., Leich, H., Leuthold, M., Lindahl, P., Liss, T., Loaiza, P., Lowder, D., Ludvig, J., Marciniewski, P., Matis, H., Miller, T., Miocinovic, P., Mock, P., Morse, R., Neunhoeffer, T., Newcomer, M., Niessen, P., Nygren, D., de los Heros, C. P., Porrata, R., Price, P., Przybylski, G., Rawlins, K., Rhode, W., Richter, S., Rodriguez, J., Romenesko, P., Ross, D., Rubinstein, H., Sander, H., Schäfer, U., Schmidt, T., Schneider, E., Schwarz, R., Schwendicke, U., Silvestri, A., Smoot, G., Solarz, M., Spiczak, G., Spiering, C., Starinski, N., Steffen, P., Stokstad, R., Streicher, O., Taboada, I., Thollander, L., Thon, T., Tilav, S., vander Donckt, M., Walck, C., Wiebusch, C., Woschnagg, K., Wu, W., Yodh, G., Young, S., Wischnewski, R., Andrés, E., Bai, X., Barouch, G., Barwick, S., Bay, R., Becker, K., Bergström, L., Bertrand, D., Besson, D., Biron, A., Booth, J., Botner, O., Bouchta, A., Carius, Staffan, Carlson, M., Chinowsky, W., Chirkin, D., Conrad, J., Cowen, D. F., Costa, C., Dalberg, E., Desiati, P., Dewulf, J., Deyoung, T., Doksus, P., Edsjö, J., Ekström, P., Feser, T., Frichter, G., Gaisser, T., Goldschmidt, A., Goobar, A., Hallgren, A., Halzen, F., Hardtke, R., Hellwig, M., Hill, G., Hulth, P., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Koepke, L., Kowalski, M., Kravchenko, I., Lamoureux, J., Leich, H., Leuthold, M., Lindahl, P., Liss, T., Loaiza, P., Lowder, D., Ludvig, J., Marciniewski, P., Matis, H., Miller, T., Miocinovic, P., Mock, P., Morse, R., Neunhoeffer, T., Newcomer, M., Niessen, P., Nygren, D., de los Heros, C. P., Porrata, R., Price, P., Przybylski, G., Rawlins, K., Rhode, W., Richter, S., Rodriguez, J., Romenesko, P., Ross, D., Rubinstein, H., Sander, H., Schäfer, U., Schmidt, T., Schneider, E., Schwarz, R., Schwendicke, U., Silvestri, A., Smoot, G., Solarz, M., Spiczak, G., Spiering, C., Starinski, N., Steffen, P., Stokstad, R., Streicher, O., Taboada, I., Thollander, L., Thon, T., Tilav, S., vander Donckt, M., Walck, C., Wiebusch, C., Woschnagg, K., Wu, W., Yodh, G., and Young, S.
Abstract: The first stage of the AMANDA High Energy Neutrino Detector at the South Pole, the 302 PMT array AMANDA-B10, is taking data since 1997. We describe results on atmospheric neutrinos, limits on indirect WIMP detection, seasonal muon flux variation, relativistic monopole flux limits, a search for gravitational collapse neutrinos, and a depth scan of the optical ice properties. The next stage 19-string detector AMANDA-II with ∼650 PMTs will be completed in spring 2000., Source: Scopus
Published: 2000
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36. The 2nd Scandinavian NeutrinO Workshop

Author: Ohlsson, T, primary, Blennow, M, additional, Badelek, B, additional, Edsjö, J, additional, Hällgren, T, additional, Konstandin, T, additional, and Pearce, M, additional
Published: 2006
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37. INDIRECT DETECTION OF NEUTRALINOS

Author: EDSJÖ, J., primary
Published: 2005
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38. The AMANDA neutrino telescope

Author: Andrés, E. C., Askebjer, P., Barwick, S. W., Bay, R. C., Bergström, L., Biron, A., Booth, J., Botner, O., Bouchta, A., Carius, Staffan, Carlson, M., Chinowsky, W., Chirkin, D., Conrad, J., Costa, C. G. S., Cowen, D., Dalberg, E., DeYoung, T., Edsjö, J., Ekström, P., Goobar, A., Gray, L., Hallgren, A., Halzen, F., Hardtke, R., Hart, S., He, Y., De Los Heros, C. P., Hill, G., Hulth, P. O., Hundertmark, S., Jacobsen, J., Jones, A., Kandhadai, V., Karle, A., Kim, J., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Loaiza, P., Lowder, D., Marciniewski, P., Miller, T. C., Miocinovic, P., Mock, P. C., Morse, R., Newcomer, M., Niessen, P., Nygren, D., Porrata, R., Potter, D., Price, P. B., Przybylski, G., Rhode, W., Richter, S., Rodriguez, J., Romenesko, P., Ross, D., Rubinstein, H., Schmidt, T., Schneider, E., Schwarz, R., Schwendicke, U., Smoot, G., Solarz, M., Sorin, V., Spiering, C., Steffen, P., Stokstad, R., Streicher, O., Taboada, I., Thon, T., Tilav, S., Walck, C., Wiebusch, C. H., Wischnewski, R., Woschnagg, K., Wu, W., Yodh, G., Young, S., Andrés, E. C., Askebjer, P., Barwick, S. W., Bay, R. C., Bergström, L., Biron, A., Booth, J., Botner, O., Bouchta, A., Carius, Staffan, Carlson, M., Chinowsky, W., Chirkin, D., Conrad, J., Costa, C. G. S., Cowen, D., Dalberg, E., DeYoung, T., Edsjö, J., Ekström, P., Goobar, A., Gray, L., Hallgren, A., Halzen, F., Hardtke, R., Hart, S., He, Y., De Los Heros, C. P., Hill, G., Hulth, P. O., Hundertmark, S., Jacobsen, J., Jones, A., Kandhadai, V., Karle, A., Kim, J., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Loaiza, P., Lowder, D., Marciniewski, P., Miller, T. C., Miocinovic, P., Mock, P. C., Morse, R., Newcomer, M., Niessen, P., Nygren, D., Porrata, R., Potter, D., Price, P. B., Przybylski, G., Rhode, W., Richter, S., Rodriguez, J., Romenesko, P., Ross, D., Rubinstein, H., Schmidt, T., Schneider, E., Schwarz, R., Schwendicke, U., Smoot, G., Solarz, M., Sorin, V., Spiering, C., Steffen, P., Stokstad, R., Streicher, O., Taboada, I., Thon, T., Tilav, S., Walck, C., Wiebusch, C. H., Wischnewski, R., Woschnagg, K., Wu, W., Yodh, G., and Young, S.
Abstract: With an effective telescope area of order 104 m2 for TeV neutrinos, a threshold near ∼50 GeV and a pointing accuracy of 2.5 degrees per muon track, the AMANDA detector represents the first of a new generation of high energy neutrino telescopes, reaching a scale envisaged over 25 years ago. We describe early results on the calibration of natural deep ice as a particle detector as well as on AMANDA's performance as a neutrino telescope., Source: Scopus
Published: 1999
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39. AMANDA : Status, results and future

Author: Andres, E., Askebjer, P., Barouch, G., Barwick, S., Bai, X., Becker, K., Bay, R., Bergström, L., Bertrand, D., Besson, D., Biron, A., Booth, J., Bothner, O., Bouchta, A., Carius, Staffan, Carlson, M., Chinowsky, W., Chirkin, D., Conrad, J., Costa, C., Cowen, D. F., Dahlberg, E., Dewulf, J., DeYoung, T., Edsjö, J., Ekström, P., Frichter, G., Goobar, A., Gray, L., Hallgren, A., Halzen, F., He, Y., Hardtke, R., Hill, G., Hulth, P.O., Hundertmark, S., Jacobsen, J., Kandhadai, V., Karle, A., Kim, J., Kroci, B., Kowalski, M., Kravchenko, I., Lamoureux, J., Loaiza, P., Leich, H., Lindahl, P., Liss, T., Liubarsky, I., Leuthold, M., Lowder, D.M., Ludvig, J., Marciniewski, P., Miller, T., Miocinovic, P., Mock, P., Newcomer, F. M., Morse, R., Niessen, P., Nygren, D., Perez de los Heros, C., Porrata, R., Price, P. B., Przybylski, G., Rawlins, K., Rhode, W., Richter, S., Rodriguez Martino, J., Romenesko, P., Ross, D., Rubenstein, H., Schneider, E., Schmidt, T., Schwarz, R., Silvestri, A., Smoot, G., Solarz, M., Spiczak, G., Spiering, C., Starinski, N., Steffen, P., Stokstad, R., Streicher, O., Taboada, I., Thon, T., Tilav, S., Vander Donckt, M., Walck, C., Wiebusch, C., Wischnewski, R., Woschnagg, K., Wu, W., Yodh, G., Young, S., Andres, E., Askebjer, P., Barouch, G., Barwick, S., Bai, X., Becker, K., Bay, R., Bergström, L., Bertrand, D., Besson, D., Biron, A., Booth, J., Bothner, O., Bouchta, A., Carius, Staffan, Carlson, M., Chinowsky, W., Chirkin, D., Conrad, J., Costa, C., Cowen, D. F., Dahlberg, E., Dewulf, J., DeYoung, T., Edsjö, J., Ekström, P., Frichter, G., Goobar, A., Gray, L., Hallgren, A., Halzen, F., He, Y., Hardtke, R., Hill, G., Hulth, P.O., Hundertmark, S., Jacobsen, J., Kandhadai, V., Karle, A., Kim, J., Kroci, B., Kowalski, M., Kravchenko, I., Lamoureux, J., Loaiza, P., Leich, H., Lindahl, P., Liss, T., Liubarsky, I., Leuthold, M., Lowder, D.M., Ludvig, J., Marciniewski, P., Miller, T., Miocinovic, P., Mock, P., Newcomer, F. M., Morse, R., Niessen, P., Nygren, D., Perez de los Heros, C., Porrata, R., Price, P. B., Przybylski, G., Rawlins, K., Rhode, W., Richter, S., Rodriguez Martino, J., Romenesko, P., Ross, D., Rubenstein, H., Schneider, E., Schmidt, T., Schwarz, R., Silvestri, A., Smoot, G., Solarz, M., Spiczak, G., Spiering, C., Starinski, N., Steffen, P., Stokstad, R., Streicher, O., Taboada, I., Thon, T., Tilav, S., Vander Donckt, M., Walck, C., Wiebusch, C., Wischnewski, R., Woschnagg, K., Wu, W., Yodh, G., and Young, S.
Abstract: We review the status of the AMANDA neutrino telescope. We present resultsobtained from the four-string prototype array AMANDA-B4 and describe themethods of track reconstruction and neutrino event separation. We give also firstresults of the analysis of the 10-string detector AMANDA-B10, in particular onatmospheric neutrinos and the search for magnetic monopoles. We sketch thefuture schedule on the way to a cube kilometer telescope at the South Pole,ICECUBE.
Published: 1999

40. DarkSUSY: computing supersymmetric dark matter properties numerically

Author: Gondolo, P, primary, Edsjö, J, additional, Ullio, P, additional, Bergström, L, additional, Schelke, M, additional, and Baltz, E A, additional
Published: 2004
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41. Limits to the muon flux from WIMP annihilation in the center of the Earth with the AMANDA detector

Author: Ahrens, J., primary, Andrés, E., additional, Bai, X., additional, Barouch, G., additional, Barwick, S. W., additional, Bay, R. C., additional, Becka, T., additional, Becker, K.-H., additional, Bertrand, D., additional, Biron, A., additional, Botner, O., additional, Bouchta, A., additional, Carius, S., additional, Chen, A., additional, Chirkin, D., additional, Conrad, J., additional, Cooley, J., additional, Costa, C. G. S., additional, Cowen, D. F., additional, Dalberg, E., additional, De Clercq, C., additional, DeYoung, T., additional, Desiati, P., additional, Dewulf, J.-P., additional, Doksus, P., additional, Edsjö, J., additional, Ekström, P., additional, Feser, T., additional, Gaisser, T. K., additional, Gaug, M., additional, Gerhardt, L., additional, Goldschmidt, A., additional, Goobar, A., additional, Hallgren, A., additional, Halzen, F., additional, Hanson, K., additional, Hardtke, R., additional, Hauschildt, T., additional, Hellwig, M., additional, Hill, G. C., additional, Hulth, P. O., additional, Hundertmark, S., additional, Jacobsen, J., additional, Karle, A., additional, Kim, J., additional, Koci, B., additional, Köpke, L., additional, Kowalski, M., additional, Lamoureux, J. I., additional, Leich, H., additional, Leuthold, M., additional, Lindahl, P., additional, Loaiza, P., additional, Lowder, D. M., additional, Ludvig, J., additional, Madsen, J., additional, Marciniewski, P., additional, Matis, H. S., additional, McParland, C. P., additional, Miller, T. C., additional, Minaeva, Y., additional, Miočinović, P., additional, Mock, P. C., additional, Morse, R., additional, Neunhöffer, T., additional, Niessen, P., additional, Nygren, D. R., additional, Ogelman, H., additional, Olbrechts, Ph., additional, Pérez de los Heros, C., additional, Pohl, A., additional, Porrata, R., additional, Price, P. B., additional, Przybylski, G.T., additional, Rawlins, K., additional, Rhode, W., additional, Ribordy, M., additional, Richter, S., additional, Rodríguez Martino, J., additional, Romenesko, P., additional, Ross, D., additional, Sander, H.-G., additional, Schmidt, T., additional, Schneider, D., additional, Schneider, E., additional, Schwarz, R., additional, Silvestri, A., additional, Solarz, M., additional, Spiczak, G. M., additional, Spiering, C., additional, Steele, D., additional, Steffen, P., additional, Stokstad, R. G., additional, Streicher, O., additional, Sudhoff, P., additional, Sulanke, K. H., additional, Taboada, I., additional, Thollander, L., additional, Thon, T., additional, Tilav, S., additional, Vander Donckt, M., additional, Walck, C., additional, Weinheimer, C., additional, Wiebusch, C. H., additional, Wiedemann, C., additional, Wischnewski, R., additional, Wissing, H., additional, Woschnagg, K., additional, Wu, W., additional, Yodh, G., additional, and Young, S., additional
Published: 2002
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42. Observation of high energy atmospheric neutrinos with the Antarctic muon and neutrino detector array

Author: Ahrens, J., primary, Andrés, E., additional, Bai, X., additional, Barouch, G., additional, Barwick, S. W., additional, Bay, R. C., additional, Becka, T., additional, Becker, K.-H., additional, Bertrand, D., additional, Binon, F., additional, Biron, A., additional, Booth, J., additional, Botner, O., additional, Bouchta, A., additional, Bouhali, O., additional, Boyce, M. M., additional, Carius, S., additional, Chen, A., additional, Chirkin, D., additional, Conrad, J., additional, Cooley, J., additional, Costa, C. G. S., additional, Cowen, D. F., additional, Dalberg, E., additional, De Clercq, C., additional, DeYoung, T., additional, Desiati, P., additional, Dewulf, J.-P., additional, Doksus, P., additional, Edsjö, J., additional, Ekström, P., additional, Feser, T., additional, Frère, J.-M., additional, Gaisser, T. K., additional, Gaug, M., additional, Goldschmidt, A., additional, Hallgren, A., additional, Halzen, F., additional, Hanson, K., additional, Hardtke, R., additional, Hauschildt, T., additional, Hellwig, M., additional, Heukenkamp, H., additional, Hill, G. C., additional, Hulth, P. O., additional, Hundertmark, S., additional, Jacobsen, J., additional, Karle, A., additional, Kim, J., additional, Koci, B., additional, Köpke, L., additional, Kowalski, M., additional, Lamoureux, J. I., additional, Leich, H., additional, Leuthold, M., additional, Lindahl, P., additional, Liubarsky, I., additional, Loaiza, P., additional, Lowder, D. M., additional, Madsen, J., additional, Marciniewski, P., additional, Matis, H. S., additional, McParland, C. P., additional, Miller, T. C., additional, Minaeva, Y., additional, Miočinović, P., additional, Mock, P. C., additional, Morse, R., additional, Neunhöffer, T., additional, Niessen, P., additional, Nygren, D. R., additional, Ögelman, H., additional, Olbrechts, Ph., additional, Pérez de los Heros, C., additional, Pohl, A. C., additional, Porrata, R., additional, Price, P. B., additional, Przybylski, G. T., additional, Rawlins, K., additional, Reed, C., additional, Rhode, W., additional, Ribordy, M., additional, Richter, S., additional, Rodríguez Martino, J., additional, Romenesko, P., additional, Ross, D., additional, Sander, H.-G., additional, Schmidt, T., additional, Schneider, D., additional, Schwarz, R., additional, Silvestri, A., additional, Solarz, M., additional, Spiczak, G. M., additional, Spiering, C., additional, Starinsky, N., additional, Steele, D., additional, Steffen, P., additional, Stokstad, R. G., additional, Streicher, O., additional, Sudhoff, P., additional, Sulanke, K.-H., additional, Taboada, I., additional, Thollander, L., additional, Thon, T., additional, Tilav, S., additional, Vander Donckt, M., additional, Walck, C., additional, Weinheimer, C., additional, Wiebusch, C. H., additional, Wiedeman, C., additional, Wischnewski, R., additional, Wissing, H., additional, Woschnagg, K., additional, Wu, W., additional, Yodh, G., additional, and Young, S., additional
Published: 2002
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43. Neutrino-induced muon fluxes from neutralino annihilations in the Sun and in the Earth

Author: Edsjö, J., primary
Published: 1995
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44. Les Houches 2011: Physics at TeV Colliders New Physics Working Group Report

Author: Brooijmans, G., Gripaios, B., Moortgat, F., Santiago, J., Skands, P., Albornoz Vásquez, D., Allanach, B. C., Alloul, A., Arbey, A., Azatov, A., Baer, H., Balázs, C., Barr, A., Basso, L., Battaglia, M., Bechtle, P., Bélanger, G., Belyaev, A., Benslama, K., Bergström, L., Bharucha, A., Boehm, C., Bondarenko, M., Bondu, O., Boos, E., Boudjema, F., Bringmann, T., Brown, M., Bunichev, V., Calvet, S., Campanelli, M., Carmona, A., Cerdeño, D. G., Chala, M., Chivukula, R. S., Chowdhury, D., Christensen, N. D., Cirelli, M., Cox, S., Cranmer, K., Da Silva, J., Delahaye, T., Roeck, A., Djouadi, A., Dobson, E., Dolan, M., Donato, F., Drieu La Rochelle, G., Duda, G., Claude Duhr, Dumont, B., Edsjö, J., Ellis, J., Evoli, C., Falkowski, A., Felcini, M., Fuks, B., Gabrielli, E., Gaggero, D., Gascon-Shotkin, S., Ghosh, D. K., Giammanco, A., Godbole, R. M., Gondolo, P., Goto, T., Grasso, D., Gris, P., Guadagnoli, D., Gunion, J. F., Haisch, U., Hartgring, L., Heinemeyer, S., Hirsch, M., Hewett, J., Ismail, A., Jeltema, T., Kadastik, M., Kakizaki, M., Kannike, K., Khalil, S., Kneur, J-L, Krämer, M., Kraml, S., Kreiss, S., Lavalle, J., Leane, R., Lykken, J., Maccione, L., Mahmoudi, F., Mangano, M., Martin, S. P., Maurin, D., Moreau, G., Moretti, S., Moskalenko, I., Moultaka, G., Muhlleitner, M., Niessen, I., O Leary, B., Orlando, E., Panci, P., Polesello, G., Porod, W., Porter, T., Profumo, S., Prosper, H., Pukhov, A., Racioppi, A., Raidal, M., Rausch Traubenberg, M., Renaud, A., Reuter, J., Rizzo, T. G., Robens, T., Rodríguez-Marrero, A. Y., Salati, P., Savage, C., Scott, P., Sekmen, S., Semenov, A., Shan, C. -L, Shepherd-Themistocleous, C., Simmons, E. H., Slavich, P., Speckner, C., Staub, F., Strong, A., Taillet, R., Thomas, F. S., Thomas, M. C., Tomalin, I., Tytgat, M., Ughetto, M., Valéry, L., Walker, D. G. E., Weiler, A., West, S. M., White, C. D., Williams, A. J., Wingerter, A., Wymant, C., Yu, J. -H, Yuan, C. -P, Zerwas, D., Institut d'Astrophysique de Paris (IAP), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre de Recherche Astrophysique de Lyon (CRAL), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire de Lyon (IPNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-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), Laboratoire de Physique Corpusculaire - Clermont-Ferrand (LPC), Université Blaise Pascal - Clermont-Ferrand 2 (UBP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Théorique - UMR CNRS 3681 (IPHT), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Théorique d'Orsay [Orsay] (LPT), Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Laboratoire Charles Coulomb (L2C), Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), 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)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Théorique et Hautes Energies (LPTHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), IN2P3, Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), École normale supérieure - Lyon (ENS Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), 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), and Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Subjects: High Energy Physics - Experiment (hep-ex), High Energy Physics - Phenomenology, High Energy Physics - Phenomenology (hep-ph), hep-ex, [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph], High Energy Physics - Experiment, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], FOS: Physical sciences, hep-ph, Particle Physics - Phenomenology
Abstract: We present the activities of the "New Physics" working group for the "Physics at TeV Colliders" workshop (Les Houches, France, 30 May-17 June, 2011). Our report includes new agreements on formats for interfaces between computational tools, new tool developments, important signatures for searches at the LHC, recommendations for presentation of LHC search results, as well as additional phenomenological studies., 243 pages, report of the Les Houches 2011 New Physics Group; fix three figures

45. Improved limits on dark matter annihilation in the Sun with the 79-string IceCube detector and implications for supersymmetry

Author: Aartsen, M. G., Abraham, K., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Altmann, D., Anderson, T., Ansseau, I., Anton, G., Archinger, M., Arguelles, C., Arlen, T. C., Auffenberg, J., Bai, X., Barwick, S. W., Baum, V., Bay, R., Beatty, J. J., Tjus, J. Becker, Becker, K.-H., Beiser, E., BenZvi, S., Berghaus, P., Berley, D., Bernardini, E., Bernhard, A., Besson, D. Z., Binder, G., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D. J., Bohm, C., Börner, M., Bos, F., Bose, D., Böser, S., Botner, O., Braun, J., Brayeur, L., Bretz, H.-P., Buzinsky, N., Casey, J., Casier, M., Cheung, E., Chirkin, D., Christov, A., Clark, K., Classen, L., Coenders, S., Collin, G. H., Conrad, J. M., Cowen, D. F., Silva, A. H. Cruz, Danninger, M., Daughhetee, J., Davis, J. C., Day, M., De André, J. P. A. M., Clercq, C. De, Rosendo, E. Del Pino, Dembinski, H., Ridder, S. De, Desiati, P., De Vries, K. D., De Wasseige, G., De With, M., DeYoung, T., Díaz-Vélez, J. C., Di Lorenzo, V., Dumm, J. P., Dunkman, M., Eberhardt, B., Edsjö, J., Ehrhardt, T., Eichmann, B., Euler, S., Evenson, P. A., Fahey, S., Fazely, A. R., Feintzeig, J., Felde, J., Filimonov, K., Finley, C., Flis, S., Fösig, C.-C., Fuchs, T., Gaisser, T. K., Gaior, R., Gallagher, J., Gerhardt, L., Ghorbani, K., Gier, D., Gladstone, L., Glagla, M., Glüsenkamp, T., Goldschmidt, A., Golup, G., Gonzalez, J. G., Góra, D., Grant, D., Griffith, Z., Groß, A., Ha, C., Haack, C., Ismail, A. Haj, Hallgren, A., Halzen, F., Hansen, E., Hansmann, B., Hanson, K., Hebecker, D., Heereman, D., Helbing, K., Hellauer, R., Hickford, S., Hignight, J., Hill, G. C., Hoffman, K. D., Hoffmann, R., Holzapfel, K., Homeier, A., Hoshina, K., Huang, F., Huber, M., Huelsnitz, W., Hulth, P. O., Hultqvist, K., In, S., Ishihara, A., Jacobi, E., Japaridze, G. S., Jeong, M., Jero, K., Jones, B. J. P., Jurkovic, M., Kappes, A., Karg, T., Karle, A., Katz, U., Kauer, M., Keivani, A., Kelley, J. L., Kemp, J., Kheirandish, A., Kiryluk, J., Klein, S. R., Kohnen, G., Koirala, R., Kolanoski, H., Konietz, R., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, Marek, Krings, K., Kroll, G., Kroll, M., Krückl, G., Kunnen, J., Kurahashi, N., Kuwabara, T., Labare, M., Lanfranchi, J. L., Larson, M. J., Lesiak-Bzdak, M., Leuermann, M., Leuner, J., Lu, L., Lünemann, J., Madsen, J., Maggi, G., Mahn, K. B. M., Mandelartz, M., Maruyama, R., Mase, K., Matis, H. S., Maunu, R., McNally, F., Meagher, K., Medici, M., Meier, M., Meli, A., Menne, T., Merino, G., Meures, T., Miarecki, S., Middell, E., Mohrmann, L., Montaruli, T., Morse, R., Nahnhauer, R., Naumann, U., Neer, G., Niederhausen, H., Nowicki, S. C., Nygren, D. R., Pollmann, A. Obertacke, Olivas, A., Omairat, A., O'Murchadha, A., Palczewski, T., Pandya, H., Pankova, D. V., Paul, L., Pepper, J. A., Heros, C. Pérez De Los, Pfendner, C., Pieloth, D., Pinat, E., Posselt, J., Price, P. B., Przybylski, G. T., Quinnan, M., Raab, C., Rädel, L., Rameez, M., Rawlins, K., Reimann, R., Relich, M., Resconi, E., Rhode, W., Richman, M., Richter, S., Riedel, B., Robertson, S., Rongen, M., Rott, C., Ruhe, T., Ryckbosch, D., Sabbatini, L., Sander, H.-G., Sandrock, A., Sandroos, J., Sarkar, S., Savage, C., Schatto, K., Schimp, M., Schlunder, P., Schmidt, T., Schoenen, S., Schöneberg, S., Schönwald, A., Schulte, L., Schumacher, L., Scott, P., Seckel, D., Seunarine, S., Silverwood, H., Soldin, D., Song, M., Spiczak, G. M., Spiering, C., Stahlberg, M., Stamatikos, M., Stanev, T., Stasik, A., Steuer, A., Stezelberger, T., Stokstad, R. G., Stößl, A., Ström, R., Strotjohann, N. L., Sullivan, G. W., Sutherland, M., Taavola, H., Taboada, I., Tatar, J., Ter-Antonyan, S., Terliuk, A., Tešić, G., Tilav, S., Toale, P. A., Tobin, M. N., Toscano, S., Tosi, D., Tselengidou, M., Turcati, A., Unger, E., Usner, M., Vallecorsa, S., Vandenbroucke, J., Eijndhoven, N. Van, Vanheule, S., Santen, J. Van, Veenkamp, J., Vehring, M., Voge, M., Vraeghe, M., Walck, C., Wallace, A., Wallraff, M., Wandkowsky, N., Weaver, Ch., Wendt, C., Westerhoff, S., Whelan, B. J., Wiebe, K., Wiebusch, C. H., Wille, L., Williams, D. R., Wills, L., Wissing, H., Wolf, M., Wood, T. R., Woschnagg, K., Xu, D. L., Xu, X. W., Xu, Y., Yanez, J. P., Yodh, G., Yoshida, S., and Zoll, M.
Subjects: 13. Climate action
Abstract: Journal of cosmology and astroparticle physics 2016(04), 022 (2016). doi:10.1088/1475-7516/2016/04/022, We present an improved event-level likelihood formalism for including neutrino telescope data in global fits to new physics. We derive limits on spin-dependent dark matter-proton scattering by employing the new formalism in a re-analysis of data from the 79-string IceCube search for dark matter annihilation in the Sun, including explicit energy information for each event. The new analysis excludes a number of models in the weak-scale minimal supersymmetric standard model (MSSM) for the first time. This work is accompanied by the public release of the 79-string IceCube data, as well as an associated computer code for applying the new likelihood to arbitrary dark matter models., Published by IOP, London

46. Observation of high energy atmospheric neutrinos with the Antarctic muon and neutrino detector array

Author: Ahrens, J., Andrés, E., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becka, T., Becker, K. -H, Bertrand, D., Binon, F., Biron, A., Booth, J., Botner, O., Bouchta, A., Bouhali, O., Boyce, M. M., Carius, S., Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dalberg, E., Clercq, C., Young, T., Desiati, P., Dewulf, J. -P, Doksus, P., Edsjö, J., Ekström, P., Feser, T., Frère, J. -M, Gaisser, T. K., Gaug, M., Goldschmidt, A., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., Hauschildt, T., Hellwig, M., Heukenkamp, H., Gary Hill, Hulth, P. O., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Lamoureux, J. I., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Loaiza, P., Lowder, D. M., Madsen, J., Marciniewski, P., Matis, H. S., Mcparland, C. P., Miller, T. C., Minaeva, Y., Miočinović, P., Mock, P. C., Morse, R., Neunhöffer, T., Niessen, P., Nygren, D. R., Ögelman, H., Olbrechts, Ph, Pérez Los Heros, C., Pohl, A. C., Porrata, R., Price, P. B., Przybylski, G. T., Rawlins, K., Reed, C., Rhode, W., Ribordy, M., Richter, S., Rodríguez Martino, J., Romenesko, P., Ross, D., Sander, H. -G, Schmidt, T., Schneider, D., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G. M., Spiering, C., Starinsky, N., Steele, D., Steffen, P., Stokstad, R. G., Streicher, O., Sudhoff, P., Sulanke, K. -H, Taboada, I., Thollander, L., Thon, T., Tilav, S., Vander Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C. H., Wiedeman, C., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., and Young, S.

47. Status of the scalar singlet dark matter model.

Author: Athron P, Balázs C, Bringmann T, Buckley A, Chrząszcz M, Conrad J, Cornell JM, Dal LA, Edsjö J, Farmer B, Jackson P, Kahlhoefer F, Krislock A, Kvellestad A, McKay J, Mahmoudi F, Martinez GD, Putze A, Raklev A, Rogan C, Saavedra A, Savage C, Scott P, Serra N, Weniger C, and White M
Abstract: One of the simplest viable models for dark matter is an additional neutral scalar, stabilised by a Z 2 symmetry. Using the GAMBIT package and combining results from four independent samplers, we present Bayesian and frequentist global fits of this model. We vary the singlet mass and coupling along with 13 nuisance parameters, including nuclear uncertainties relevant for direct detection, the local dark matter density, and selected quark masses and couplings. We include the dark matter relic density measured by Planck , direct searches with LUX, PandaX, SuperCDMS and XENON100, limits on invisible Higgs decays from the Large Hadron Collider, searches for high-energy neutrinos from dark matter annihilation in the Sun with IceCube, and searches for gamma rays from annihilation in dwarf galaxies with the Fermi -LAT. Viable solutions remain at couplings of order unity, for singlet masses between the Higgs mass and about 300 GeV, and at masses above ∼ 1 TeV. Only in the latter case can the scalar singlet constitute all of dark matter. Frequentist analysis shows that the low-mass resonance region, where the singlet is about half the mass of the Higgs, can also account for all of dark matter, and remains viable. However, Bayesian considerations show this region to be rather fine-tuned., (© The Author(s) 2017.)
Published: 2017
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48. Dark matter interpretation of recent electron and positron data.

Author: Bergström L, Edsjö J, and Zaharijas G
Abstract: We analyze the recently released Fermi-LAT data on the sum of electrons and positrons. Compared to a conventional, pre-Fermi, background model, a surprising excess in the several hundred GeV range is found and here we analyze it in terms of dark matter models. We also compare with newly published results from PAMELA and H.E.S.S., and find models giving very good fits to these data sets as well. If this dark matter interpretation is correct, we also predict the possibility of a sharp break in the diffuse gamma-ray spectrum coming from final state radiation.
Published: 2009
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49. Significant gamma lines from inert Higgs dark matter.

Author: Gustafsson M, Lundström E, Bergström L, and Edsjö J
Abstract: One way to unambiguously confirm the existence of particle dark matter and determine its mass would be to detect its annihilation into monochromatic gamma-rays in upcoming telescopes. One of the most minimal models for dark matter is the inert doublet model, obtained by adding another Higgs doublet with no direct coupling to fermions. For a mass between 40 and 80 GeV, the lightest of the new inert Higgs particles can give the correct cosmic abundance of cold dark matter in agreement with current observations. We show that for this scalar dark matter candidate, the annihilation signal of monochromatic gammagamma and Zgamma final states would be exceptionally strong. The energy range and rates for these gamma-ray line signals make them ideal to search for with the soon upcoming GLAST satellite.
Published: 2007
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50. Spectral gamma-ray signatures of cosmological dark matter annihilations.

Author: Bergström L, Edsjö J, and Ullio P
Abstract: We propose a new signature for weakly interacting massive particle (WIMP) dark matter, a spectral feature in the diffuse extragalactic gamma-ray radiation. This feature, a sudden drop of the gamma-ray intensity at an energy corresponding to the WIMP mass, comes from the asymmetric distortion of the line due to WIMP annihilation into two gamma rays caused by the cosmological redshift. Unlike other proposed searches for a line signal, this method is not very sensitive to the exact dark matter density distribution in halos and subhalos.
Published: 2001
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