检索结果-内蒙古大学图书馆

arXiv 2017年

作者： Natoli, P. Ashdown, M. Banerji, R. Borrill, J. Buzzelli, A. de Gasperis, G. Delabrouille, J. Hivon, E. Molinari, D. Patanchon, G. Polastri, L. Tomasi, M. Bouchet, F.R. Henrot-Versillé, S. Hoang, D.T. Keskitalo, R. Kiiveri, K. Kisner, T. Lindholm, V. McCarthy, D. Piacentini, F. Perdereau, O. Polenta, G. Tristram, M. Achucarro, A. Ade, P. Allison, R. Baccigalupi, C. Ballardini, M. Banday, A.J. Bartlett, J. Bartolo, N. Basak, S. Baselmans, J. Baumann, D. Bersanelli, M. Bonaldi, A. Bonato, M. Boulanger, F. Brinckmann, T. Bucher, M. Burigana, C. Cai, Z.-Y. Calvo, M. Carvalho, C.-S. Castellano, G. Challinor, A. Chluba, J. Clesse, S. Colantoni, I. Coppolecchia, A. Crook, M. D'Alessandro, G. de Bernardis, P. de Zotti, G. Di Valentino, E. Diego, J.-M. Errard, J. Feeney, S. Fernandez-Cobos, R. Finelli, F. Forastieri, F. Galli, S. Genova-Santos, R. Gerbino, M. González-Nuevo, J. Grandis, S. Greenslade, J. Gruppuso, A. Hagstotz, S. Hanany, S. Handley, W. Hernandez-Monteagudo, C. Hervías-Caimapo, C. Hills, M. Keihänen, E. Kitching, T. Kunz, M. Kurki-Suonio, H. Lamagna, L. Lasenby, A. Lattanzi, M. Lesgourgues, J. Lewis, A. Liguori, M. López-Caniego, M. Luzzi, G. Maffei, B. Mandolesi, N. Martinez-González, E. Martins, C.J.A.P. Masi, S. Melchiorri, A. Melin, J.-B. Migliaccio, M. Monfardini, A. Negrello, M. Notari, A. Pagano, L. Paiella, A. Paoletti, D. Piat, M. Pisano, G. Pollo, A. Poulin, V. Quartin, M. Remazeilles, M. Roman, M. Rossi, G. Rubino-Martin, J.-A. Salvati, L. Signorelli, G. Tartari, A. Tramonte, D. Trappe, N. Trombetti, T. Tucker, C. Valiviita, J. van de Weijgaert, R. van Tent, B. Vennin, V. Vielva, P. Vittorio, N. Wallis, C. Young, K. Zannoni, M. Dipartimento di Fisica e Scienze della Terra Università di Ferrara Via Saragat 1 Ferrara44122 Italy INFN Sezione di Ferrara Via Saragat 1 Ferrara44122 Italy Astrophysics Group Cavendish Laboratory University of Cambridge J. J. Thomson Avenue CambridgeCB3 0HE United Kingdom Kavli Institute for Cosmology Univerisity of Cambridge Madingley Road CambridgeCB3 0HA United Kingdom APC AstroParticule et Cosmologie Université Paris Diderot CNRS/IN2P3 CEA/lrfu Observatoire de Paris Sorbonne Paris Cité 10 rue Alice Domon et Léonie Duquet Paris Cedex 1375205 France Computational Cosmology Center Lawrence Berkeley National Laboratory BerkeleyCA United States Space Sciences Laboratory University of California BerkeleyCA94720 United States Dipartimento di Fisica Università di Roma La Sapienza P.le A. Moro 2 Roma00185 Italy Dipartimento di Fisica Università di Roma Tor Vergata Via della Ricerca Scientifica 1 RomaI-00133 Italy INFN Sezione di Tor Vergata Via della Ricerca Scientifica 1 RomaI-00133 Italy ParisF-75014 France INAF/IASF Bologna via Gobetti 101 BolognaI-40129 Italy Dipartimento di Fisica Università degli Studi di Milano Via Celoria 16 Milano Italy INAF/IASF Milano Via E. Bassini 15 Milano Italy Laboratoire de l'Accélérateur Linéaire Univ. Paris-Sud CNRS/IN2P3 Université Paris-Saclay Orsay France Department of Physics Gustaf Hällströmin katu 2a University of Helsinki Helsinki Finland Helsinki Institute of Physics University of Helsinki Gustaf Hällströmin katu 2 Helsinki Finland Department of Experimental Physics Maynooth University Maynooth Co. KildareW23 F2H6 Ireland INFN Sezione di Roma P.le Aldo Moro 5 RomaI-00185 Italy Agenzia Spaziale Italiana Science Data Center Via del Politecnico snc Roma00133 Italy INAF - Osservatorio Astronomico di Roma via di Frascati 33 Monte Porzio Catone Italy Instituut-Lorentz for Theoretical Physics Universiteit Leiden Leiden2333 CA Netherlands Department of Theoretical Physics Univ

We present an analysis of the main systematic effects that could impact the measurement of CMB polarization with the proposed CORE space mission. We employ timeline-to-map simulations to verify that the CORE instrumental set-up and scanning strategy allow us to measure sky polarization to a level of accuracy adequate to the mission science goals. We also show how the CORE observations can be processed to mitigate the level of contamination by potentially worrying systematics, including intensity-to-polarization leakage due to bandpass mismatch, asymmetric main beams, pointing errors and correlated noise. We use analysis techniques that are well validated on data from current missions such as Planck to demonstrate how the residual contamination of the measurements by these effects can be brought to a level low enough not to hamper the scientific capability of the mission, nor significantly increase the overall error budget. We also present a prototype of the CORE photometric calibration pipeline, based on that used for Planck, and discuss its robustness to systematics, showing how CORE can achieve its calibration requirements. While a fine-grained assessment of the impact of systematics requires a level of knowledge of the system that can only be achieved in a future study phase, the analysis presented here strongly suggests that the main areas of concern for the CORE mission can be addressed using existing knowledge, techniques and algorithms. Copyright © 2017, The Authors. All rights reserved.

关键词： Calibration

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Measurement of CP observables in B±→ DK∗± decays using two- and four-body D final states

arXiv

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arXiv 2017年

作者： Aaij, R. Adeva, B. Adinolfi, M. Ajaltouni, Z. Akar, S. Albrecht, J. Alessio, F. Alexander, M. Alfonso Albero, A. Ali, S. Alkhazov, G. Alvarez Cartelle, P. Alves, A.A. Amato, S. Amerio, S. Amhis, Y. An, L. Anderlini, L. Andreassi, G. Andreotti, M. Andrews, J.E. Appleby, R.B. Archilli, F. d'Argent, P. Arnau Romeu, J. Artamonov, A. Artuso, M. Aslanides, E. Atzeni, M. Auriemma, G. Baalouch, M. Babuschkin, I. Bachmann, S. Back, J.J. Badalov, A. Baesso, C. Baker, S. Balagura, V. Baldini, W. Baranov, A. Barlow, R.J. Barschel, C. Barsuk, S. Barter, W. Baryshnikov, F. Batozskaya, V. Battista, V. Bay, A. Beaucourt, L. Beddow, J. Bedeschi, F. Bediaga, I. Beiter, A. Bel, L.J. Beliy, N. Bellee, V. Belloli, N. Belous, K. Belyaev, I. Ben-Haim, E. Bencivenni, G. Benson, S. Beranek, S. Berezhnoy, A. Bernet, R. Berninghoff, D. Bertholet, E. Bertolin, A. Betancourt, C. Betti, F. Bettler, M.-O. van Beuzekom, M. Bezshyiko, Ia. Bifani, S. Billoir, P. Birnkraut, A. Bizzeti, A. Bjørn, M. Blake, T. Blanc, F. Blusk, S. Bocci, V. Boettcher, T. Bondar, A. Bondar, N. Bordyuzhin, I. Borgheresi, A. Borghi, S. Borisyak, M. Borsato, M. Bossu, F. Boubdir, M. Bowcock, T.J.V. Bowen, E. Bozzi, C. Braun, S. Britton, T. Brodzicka, J. Brundu, D. Buchanan, E. Burr, C. Bursche, A. Buytaert, J. Byczynski, W. Cadeddu, S. Cai, H. Calabrese, R. Calladine, R. Calvi, M. Calvo Gomez, M. Camboni, A. Campana, P. Campora Perez, D.H. Capriotti, L. Carbone, A. Carboni, G. Cardinale, R. Cardini, A. Carniti, P. Carson, L. Carvalho Akiba, K. Casse, G. Cassina, L. Cattaneo, M. Cavallero, G. Cenci, R. Chamont, D. Chapman, M.G. Charles, M. Charpentier, Ph. Chatzikonstantinidis, G. Chefdeville, M. Chen, S. Cheung, S.F. Chitic, S.-G. Chobanova, V. Chrzaszcz, M. Chubykin, A. Ciambrone, P. Cid Vidal, X. Ciezarek, G. Clarke, P.E.L. Clemencic, M. Cliff, H.V. Closier, J. Cogan, J. Cogneras, E. Cogoni, V. Cojocariu, L. Collins, P. Colombo, T. Comerma-Montells, A. Contu, A. Cook, A. Coombs, G. Rio de Janeiro Brazil Rio de Janeiro Brazil Center for High Energy Physics Tsinghua University Beijing China LAPP Université Savoie Mont-Blanc CNRS/IN2P3 Annecy-Le-Vieux France Clermont Université Université Blaise Pascal CNRS/IN2P3 LPC Clermont-Ferrand France Aix Marseille Univ CNRS/IN2P3 CPPM Marseille France LAL Université Paris-Sud CNRS/IN2P3 Orsay France LPNHE Université Pierre et Marie Curie Université Paris Diderot CNRS/IN2P3 Paris France I. Physikalisches Institut RWTH Aachen University Aachen Germany Fakultät Physik Technische Universität Dortmund Dortmund Germany Heidelberg Germany Physikalisches Institut Ruprecht-Karls-Universität Heidelberg Heidelberg Germany School of Physics University College Dublin Dublin Ireland Sezione INFN di Bari Bari Italy Sezione INFN di Bologna Bologna Italy Sezione INFN di Cagliari Cagliari Italy Universita e INFN Ferrara Ferrara Italy Sezione INFN di Firenze Firenze Italy Laboratori Nazionali dell'INFN di Frascati Frascati Italy Sezione INFN di Genova Genova Italy Universita & INFN Milano-Bicocca Milano Italy Sezione di Milano Milano Italy Sezione INFN di Padova Padova Italy Sezione INFN di Pisa Pisa Italy Sezione INFN di Roma Tor Vergata Roma Italy Sezione INFN di Roma La Sapienza Roma Italy Henryk Niewodniczanski Institute of Nuclear Physics Polish Academy of Sciences Kraków Poland AGH - University of Science and Technology Faculty of Physics and Applied Computer Science Kraków Poland Warsaw Poland Horia Hulubei National Institute of Physics and Nuclear Engineering Bucharest-Magurele Romania Gatchina Russia Moscow Russia Moscow Russia Moscow Russia Yandex School of Data Analysis Moscow Russia Novosibirsk Russia Protvino Russia ICCUB Universitat de Barcelona Barcelona Spain Universidad de Santiago de Compostela Santiago de Compostela Spain Geneva Switzerland Lausanne Switzerland Physik-Institut Universität Zürich Zürich Switzerland Nikhef National Institu

Measurements of CP observables in B± → DK∗± decays are presented, where D denotes a superposition of D0 and D0 meson states. Decays of the D meson to K−π+, K−K+, π−π+, K−π+π−π+ and π−π+π−π+ are used and the K∗± meson is reconstructed in the KS0π± final state. This analysis uses a data sample of pp collisions collected with the LHCb experiment, corresponding to integrated luminosities of 1 fb−1, 2 fb−1 and 1.8 fb−1 at centre-of-mass energies √s = 7 TeV, 8 TeV and 13 TeV, respectively. The sensitivity of the results to the CKM angle γ is discussed. Copyright © 2017, The Authors. All rights reserved.

关键词： Bosons

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Observation of the doubly charmed baryon Ξcc++

arXiv

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arXiv 2017年

作者： Aaij, R. Adeva, B. Adinolfi, M. Ajaltouni, Z. Akar, S. Albrecht, J. Alessio, F. Alexander, M. Alfonso Albero, A. Ali, S. Alkhazov, G. Alvarez Cartelle, P. Alves, A.A. Amato, S. Amerio, S. Amhis, Y. An, L. Anderlini, L. Andreassi, G. Andreotti, M. Andrews, J.E. Appleby, R.B. Archilli, F. d'Argent, P. Arnau Romeu, J. Artamonov, A. Artuso, M. Aslanides, E. Auriemma, G. Baalouch, M. Babuschkin, I. Bachmann, S. Back, J.J. Badalov, A. Baesso, C. Baker, S. Balagura, V. Baldini, W. Baranov, A. Barlow, R.J. Barschel, C. Barsuk, S. Barter, W. Baryshnikov, F. Batozskaya, V. Battista, V. Bay, A. Beaucourt, L. Beddow, J. Bedeschi, F. Bediaga, I. Beiter, A. Bel, L.J. Beliy, N. Bellee, V. Belloli, N. Belous, K. Belyaev, I. Ben-Haim, E. Bencivenni, G. Benson, S. Beranek, S. Berezhnoy, A. Bernet, R. Berninghoff, D. Bertholet, E. Bertolin, A. Betancourt, C. Betti, F. Bettler, M.-O. van Beuzekom, M. Bezshyiko, Ia. Bifani, S. Billoir, P. Birnkraut, A. Bitadze, A. Bizzeti, A. Bjoern, M.B. Blake, T. Blanc, F. Blouw, J. Blusk, S. Bocci, V. Boettcher, T. Bondar, A. Bondar, N. Bonivento, W. Bordyuzhin, I. Borgheresi, A. Borghi, S. Borisyak, M. Borsato, M. Borysova, M. Bossu, F. Boubdir, M. Bowcock, T.J.V. Bowen, E. Bozzi, C. Braun, S. Britton, T. Brodzicka, J. Brundu, D. Buchanan, E. Burr, C. Bursche, A. Buytaert, J. Byczynski, W. Cadeddu, S. Cai, H. Calabrese, R. Calladine, R. Calvi, M. Calvo Gomez, M. Camboni, A. Campana, P. Campora Perez, D.H. Capriotti, L. Carbone, A. Carboni, G. Cardinale, R. Cardini, A. Carniti, P. Carson, L. Carvalho Akiba, K. Casse, G. Cassina, L. Castillo Garcia, L. Cattaneo, M. Cavallero, G. Cenci, R. Chamont, D. Charles, M. Charpentier, Ph. Chatzikonstantinidis, G. Chefdeville, M. Chen, S. Cheung, S.F. Chitic, S.-G. Chobanova, V. Chrzaszcz, M. Chubykin, A. Ciambrone, P. Cid Vidal, X. Ciezarek, G. Clarke, P.E.L. Clemencic, M. Cliff, H.V. Closier, J. Cogan, J. Cogneras, E. Cogoni, V. Cojocariu, L. Collins, P. Colombo, T. Rio de Janeiro Brazil Rio de Janeiro Brazil Center for High Energy Physics Tsinghua University Beijing China LAPP Université Savoie Mont-Blanc CNRS/IN2P3 Annecy-Le-Vieux France Clermont Université Université Blaise Pascal CNRS/IN2P3 LPC Clermont-Ferrand France CPPM Aix-Marseille Université CNRS/IN2P3 Marseille France LAL Université Paris-Sud CNRS/IN2P3 Orsay France LPNHE Université Pierre et Marie Curie Université Paris Diderot CNRS/IN2P3 Paris France I. Physikalisches Institut RWTH Aachen University Aachen Germany Fakultät Physik Technische Universität Dortmund Dortmund Germany Heidelberg Germany Physikalisches Institut Ruprecht-Karls-Universität Heidelberg Heidelberg Germany School of Physics University College Dublin Dublin Ireland Sezione INFN di Bari Bari Italy Sezione INFN di Bologna Bologna Italy Sezione INFN di Cagliari Cagliari Italy Universita e INFN Ferrara Ferrara Italy Sezione INFN di Firenze Firenze Italy Laboratori Nazionali dell'INFN di Frascati Frascati Italy Sezione INFN di Genova Genova Italy Universita e INFN Milano-Bicocca Milano Italy Sezione di Milano Milano Italy Sezione INFN di Padova Padova Italy Sezione INFN di Pisa Pisa Italy Sezione INFN di Roma Tor Vergata Roma Italy Sezione INFN di Roma La Sapienza Roma Italy Henryk Niewodniczanski Institute of Nuclear Physics Polish Academy of Sciences Kraków Poland AGH - University of Science and Technology Faculty of Physics and Applied Computer Science Kraków Poland Warsaw Poland Horia Hulubei National Institute of Physics and Nuclear Engineering Bucharest-Magurele Romania Gatchina Russia Moscow Russia Moscow Russia Moscow Russia Yandex School of Data Analysis Moscow Russia Novosibirsk Russia Protvino Russia ICCUB Universitat de Barcelona Barcelona Spain Universidad de Santiago de Compostela Santiago de Compostela Spain Geneva Switzerland Lausanne Switzerland Physik-Institut Universität Zürich Zürich Switzerland Nikhef National I

A highly significant structure is observed in the Λ+c K−π+π+ mass spectrum, where the Λ+c baryon is reconstructed in the decay mode pK−π+. The structure is consistent with originating from a weakly decaying particle, identified as the doubly charmed baryon Ξcc++. The difference between the masses of the Ξcc++ and Λ+c states is measured to be 1334.94 ± 0.72 (stat) ± 0.27 (syst) MeV/c2, and the Ξcc++ mass is then determined to be 3621.40 ± 0.72 (stat) ± 0.27 (syst) ± 0.14 (Λ+c ) MeV/c2, where the last uncertainty is due to the limited knowledge of the Λ+c mass. The state is observed in a sample of proton-proton collision data collected by the LHCb experiment at a center-of-mass energy of 13 TeV, corresponding to an integrated luminosity of 1.7 fb−1, and confirmed in an additional sample of data collected at 8 TeV. Copyright © 2017, The Authors. All rights reserved.

关键词： Hadrons

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χc1 and χc2 resonance parameters with the decays χc1,c2 → J/ψµ+µ−

arXiv

引用

arXiv 2017年

作者： Aaij, R. Adeva, B. Adinolfi, M. Ajaltouni, Z. Akar, S. Albrecht, J. Alessio, F. Alexander, M. Alfonso Albero, A. Ali, S. Alkhazov, G. Alvarez Cartelle, P. Alves, A.A. Amato, S. Amerio, S. Amhis, Y. An, L. Anderlini, L. Andreassi, G. Andreotti, M. Andrews, J.E. Appleby, R.B. Archilli, F. d'Argent, P. Arnau Romeu, J. Artamonov, A. Artuso, M. Aslanides, E. Atzeni, M. Auriemma, G. Baalouch, M. Babuschkin, I. Bachmann, S. Back, J.J. Badalov, A. Baesso, C. Baker, S. Balagura, V. Baldini, W. Baranov, A. Barlow, R.J. Barschel, C. Barsuk, S. Barter, W. Baryshnikov, F. Batozskaya, V. Battista, V. Bay, A. Beaucourt, L. Beddow, J. Bedeschi, F. Bediaga, I. Beiter, A. Bel, L.J. Beliy, N. Bellee, V. Belloli, N. Belous, K. Belyaev, I. Ben-Haim, E. Bencivenni, G. Benson, S. Beranek, S. Berezhnoy, A. Bernet, R. Berninghoff, D. Bertholet, E. Bertolin, A. Betancourt, C. Betti, F. Bettler, M.-O. van Beuzekom, M. Bezshyiko, Ia. Bifani, S. Billoir, P. Birnkraut, A. Bizzeti, A. Bjørn, M. Blake, T. Blanc, F. Blusk, S. Bocci, V. Boettcher, T. Bondar, A. Bondar, N. Bordyuzhin, I. Borghi, S. Borisyak, M. Borsato, M. Bossu, F. Boubdir, M. Bowcock, T.J.V. Bowen, E. Bozzi, C. Braun, S. Britton, T. Brodzicka, J. Brundu, D. Buchanan, E. Burr, C. Bursche, A. Buytaert, J. Byczynski, W. Cadeddu, S. Cai, H. Calabrese, R. Calladine, R. Calvi, M. Calvo Gomez, M. Camboni, A. Campana, P. Campora Perez, D.H. Capriotti, L. Carbone, A. Carboni, G. Cardinale, R. Cardini, A. Carniti, P. Carson, L. Carvalho Akiba, K. Casse, G. Cassina, L. Cattaneo, M. Cavallero, G. Cenci, R. Chamont, D. Chapman, M.G. Charles, M. Charpentier, Ph. Chatzikonstantinidis, G. Chefdeville, M. Chen, S. Cheung, S.F. Chitic, S.-G. Chobanova, V. Chrzaszcz, M. Chubykin, A. Ciambrone, P. Cid Vidal, X. Ciezarek, G. Clarke, P.E.L. Clemencic, M. Cliff, H.V. Closier, J. Cogan, J. Cogneras, E. Cogoni, V. Cojocariu, L. Collins, P. Colombo, T. Comerma-Montells, A. Contu, A. Cook, A. Coombs, G. Coquereau, S. Rio de Janeiro Brazil Rio de Janeiro Brazil Center for High Energy Physics Tsinghua University Beijing China LAPP Université Savoie Mont-Blanc CNRS/IN2P3 Annecy-Le-Vieux France Clermont Université Université Blaise Pascal CNRS/IN2P3 LPC Clermont-Ferrand France Aix Marseille Univ CNRS/IN2P3 CPPM Marseille France LAL Université Paris-Sud CNRS/IN2P3 Orsay France LPNHE Université Pierre et Marie Curie Université Paris Diderot CNRS/IN2P3 Paris France I. Physikalisches Institut RWTH Aachen University Aachen Germany Fakultät Physik Technische Universität Dortmund Dortmund Germany Heidelberg Germany Physikalisches Institut Ruprecht-Karls-Universität Heidelberg Heidelberg Germany School of Physics University College Dublin Dublin Ireland Sezione INFN di Bari Bari Italy Sezione INFN di Bologna Bologna Italy Sezione INFN di Cagliari Cagliari Italy Universita e INFN Ferrara Ferrara Italy Sezione INFN di Firenze Firenze Italy Laboratori Nazionali dell'INFN di Frascati Frascati Italy Sezione INFN di Genova Genova Italy Universita & INFN Milano-Bicocca Milano Italy Sezione di Milano Milano Italy Sezione INFN di Padova Padova Italy Sezione INFN di Pisa Pisa Italy Sezione INFN di Roma Tor Vergata Roma Italy Sezione INFN di Roma La Sapienza Roma Italy Henryk Niewodniczanski Institute of Nuclear Physics Polish Academy of Sciences Kraków Poland AGH - University of Science and Technology Faculty of Physics and Applied Computer Science Kraków Poland Warsaw Poland Horia Hulubei National Institute of Physics and Nuclear Engineering Bucharest-Magurele Romania Gatchina Russia Moscow Russia Moscow Russia Moscow Russia Yandex School of Data Analysis Moscow Russia Novosibirsk Russia Protvino Russia ICCUB Universitat de Barcelona Barcelona Spain Universidad de Santiago de Compostela Santiago de Compostela Spain Geneva Switzerland Lausanne Switzerland Physik-Institut Universität Zürich Zürich Switzerland Nikhef National Institu

The decays χc1 → J/ψµ+µ− and χc2 → J/ψµ+µ− are observed and used to study the resonance parameters of the χc1 and χc2 mesons. The masses of these states are measured to be m(χc1) = 3510.71 ± 0.04 (stat) ± 0.09 (syst) MeV, m(χc2) = 3556.10 ± 0.06 (stat) ± 0.11 (syst) MeV, where the knowledge of the momentum scale for charged particles dominates the systematic uncertainty. The momentum-scale uncertainties largely cancel in the mass difference m(χc2) − m(χc1) = 45.39 ± 0.07 (stat) ± 0.03 (syst) MeV. The natural width of the χc2 meson is measured to be Γ(χc2) = 2.10 ± 0.20 (stat) ± 0.02 (syst) MeV. These results are in good agreement with and have comparable precision to the current world averages. Copyright © 2017, The Authors. All rights reserved.

关键词： Hadrons

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Search for astrophysical tau neutrinos in three years of IceCube data

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Physical Review D 2016年第2期93卷 022001-022001页

作者： M. G. Aartsen K. Abraham M. Ackermann J. Adams J. A. Aguilar M. Ahlers M. Ahrens D. Altmann T. Anderson I. Ansseau M. Archinger C. Arguelles T. C. Arlen J. Auffenberg X. Bai S. W. Barwick V. Baum R. Bay J. J. Beatty J. Becker Tjus K.-H. Becker E. Beiser S. BenZvi P. Berghaus D. Berley E. Bernardini A. Bernhard D. Z. Besson G. Binder D. Bindig M. Bissok E. Blaufuss J. Blumenthal D. J. Boersma C. Bohm M. Börner F. Bos D. Bose S. Böser O. Botner J. Braun L. Brayeur H.-P. Bretz N. Buzinsky J. Casey M. Casier E. Cheung D. Chirkin A. Christov K. Clark L. Classen S. Coenders D. F. Cowen A. H. Cruz Silva J. Daughhetee J. C. Davis M. Day J. P. A. M. de André C. De Clercq E. del Pino Rosendo H. Dembinski S. De Ridder P. Desiati K. D. de Vries G. de Wasseige M. de With T. DeYoung J. C. Díaz-Vélez V. di Lorenzo J. P. Dumm M. Dunkman R. Eagan B. Eberhardt T. Ehrhardt B. Eichmann S. Euler P. A. Evenson O. Fadiran S. Fahey A. R. Fazely A. Fedynitch J. Feintzeig J. Felde K. Filimonov C. Finley T. Fischer-Wasels S. Flis C.-C. Fösig T. Fuchs T. K. Gaisser R. Gaior J. Gallagher L. Gerhardt K. Ghorbani D. Gier L. Gladstone M. Glagla T. Glüsenkamp A. Goldschmidt G. Golup J. G. Gonzalez D. Góra D. Grant J. C. Groh A. Groß C. Ha C. Haack A. Haj Ismail A. Hallgren F. Halzen E. Hansen B. Hansmann K. Hanson D. Hebecker D. Heereman K. Helbing R. Hellauer S. Hickford J. Hignight G. C. Hill K. D. Hoffman R. Hoffmann K. Holzapfel A. Homeier K. Hoshina F. Huang M. Huber W. Huelsnitz P. O. Hulth K. Hultqvist S. In A. Ishihara E. Jacobi G. S. Japaridze K. Jero M. Jurkovic A. Kappes T. Karg A. Karle M. Kauer A. Keivani J. L. Kelley J. Kemp A. Kheirandish J. Kiryluk J. Kläs S. R. Klein G. Kohnen R. Koirala H. Kolanoski R. Konietz L. Köpke C. Kopper S. Kopper D. J. Koskinen M. Kowalski K. Krings G. Kroll M. Kroll J. Kunnen N. Kurahashi T. Kuwabara M. Labare J. L. Lanfranchi M. J. Larson M. Lesiak-Bzdak M. Leuermann J. Leuner L. Lu J. Lünemann J. Madsen G. Maggi K. B. M. Mahn R. Maruyama K. Mase H. S. Matis R. Maunu F. McNally K. Meagher M. Medici A Department of Physics University of Adelaide Adelaide 5005 Australia Technische Universität München D-85748 Garching Germany DESY D-15735 Zeuthen Germany Department of Physics and Astronomy University of Canterbury Private Bag 4800 Christchurch New Zealand Université Libre de Bruxelles Science Faculty CP230 B-1050 Brussels Belgium Department of Physics and Wisconsin IceCube Particle Astrophysics Center University of Wisconsin Madison Wisconsin 53706 USA Oskar Klein Centre and Department of Physics Stockholm University SE-10691 Stockholm Sweden Erlangen Centre for Astroparticle Physics Friedrich-Alexander-Universität Erlangen-Nürnberg D-91058 Erlangen Germany Department of Physics Pennsylvania State University University Park Pennsylvania 16802 USA Institute of Physics University of Mainz Staudinger Weg 7 D-55099 Mainz Germany III. Physikalisches Institut RWTH Aachen University D-52056 Aachen Germany Physics Department South Dakota School of Mines and Technology Rapid City South Dakota 57701 USA Department of Physics and Astronomy University of California Irvine California 92697 USA Department of Physics University of California Berkeley California 94720 USA Department of Physics and Center for Cosmology and Astro-Particle Physics Ohio State University Columbus Ohio 43210 USA Department of Astronomy Ohio State University Columbus Ohio 43210 USA Fakultät für Physik & Astronomie Ruhr-Universität Bochum D-44780 Bochum Germany Department of Physics University of Wuppertal D-42119 Wuppertal Germany Department of Physics University of Maryland College Park Maryland 20742 USA Department of Physics and Astronomy University of Kansas Lawrence Kansas 66045 USA Lawrence Berkeley National Laboratory Berkeley California 94720 USA Department of Physics and Astronomy Uppsala University Box 516 S-75120 Uppsala Sweden Department of Physics TU Dortmund University D-44221 Dortmund Germany Department of Physics Sungkyunkwan University Suwon 440-746 Korea

The IceCube Neutrino Observatory has observed a diffuse flux of TeV-PeV astrophysical neutrinos at 5.7σ significance from an all-flavor search. The direct detection of tau neutrinos in this flux has yet to occur. Tau neutrinos become distinguishable from other flavors in IceCube at energies above a few hundred TeV, when the cascade from the tau neutrino charged current interaction becomes resolvable from the cascade from the tau lepton decay. This paper presents results from the first dedicated search for tau neutrinos with energies between 214 TeV and 72 PeV in the full IceCube detector. The analysis searches for IceCube optical sensors that observe two separate pulses in a single event—one from the tau neutrino interaction and a second from the tau decay. No candidate events were observed in three years of IceCube data. For the first time, a differential upper limit on astrophysical tau neutrinos is derived around the PeV energy region, which is nearly 3 orders of magnitude lower in energy than previous limits from dedicated tau neutrino searches.

关键词： Cosmic ray composition & spectra Extrasolar neutrino astronomy Neutrino interactions Cosmic ray & astroparticle detectors

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Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger

arXiv

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arXiv 2017年

作者： Pian, E. D’Avanzo, P. Benetti, S. Branchesi, M. Brocato, E. Campana, S. Cappellaro, E. Covino, S. D’Elia, V. Fynbo, J.P.U. Getman, F. Ghirlanda, G. Ghisellini, G. Grado, A. Greco, G. Hjorth, J. Kouveliotou, C. Levan, A. Limatola, L. Malesani, D. Mazzali, P.A. Melandri, A. Møller, P. Nicastro, L. Palazzi, E. Piranomonte, S. Rossi, A. Salafia, O.S. Selsing, J. Stratta, G. Tanaka, M. Tanvir, N.R. Tomasella, L. Watson, D. Yang, S. Amati, L. Antonelli, L.A. Ascenzi, S. Bernardini, M.G. Boër, M. Bufano, F. Bulgarelli, A. Capaccioli, M. Casella, P.G. Castro-Tirado, A.J. Chassande-Mottin, E. Ciolfi, R. Copperwheat, C.M. Dadina, M. de Cesare, G. Di Paola, A. Fan, Y.Z. Gendre, B. Giuffrida, G. Giunta, A. Hunt, L.K. Israel, G. Jin, Z.-P. Kasliwal, M. Klose, S. Lisi, M. Longo, F. Maiorano, E. Mapelli, M. Masetti, N. Nava, L. Patricelli, B. Perley, D. Pescalli, A. Piran, T. Possenti, A. Pulone, L. Razzano, M. Salvaterra, R. Schipani, P. Spera, M. Stamerra, A. Stella, L. Tagliaferri, G. Testa, V. Troja, E. Turatto, M. Vergani, S.D. Vergani, D. INAF Institute of Space Astrophysics and Cosmic Physics Via Gobetti 101 BolognaI-40129 Italy I-23807 Italy INAF Osservatorio Astronomico di Padova Vicolo dell’Osservatorio 5 PadovaI-35122 Italy Gran Sasso Science Institute Viale F. Crispi 7 L’Aquila Italy INFN Laboratori Nazionali del Gran Sasso L’AquilaI-67100 Italy Space Science Data Center ASI Via del Politecnico s.n.c. Roma00133 Italy INAF Osservatorio Astronomico di Roma Via di Frascati 33 Monteporzio CatoneI-00078 Italy Dark Cosmology Centre Niels Bohr Institute University of Copenhagen Juliane Maries Vej 30 Copenhagen ØDK-2100 Denmark INAF Osservatorio Astronomico di Capodimonte salita Moiariello 16 NapoliI-80131 Italy Università degli Studi di Urbino ‘Carlo Bo’ Dipartimento di Scienze Pure e Applicate P.za Repubblica 13 UrbinoI-61029 Italy INFN Sezione di Firenze Sesto Fiorentino FirenzeI-50019 Italy Department of Physics George Washington University Corcoran Hall WashingtonDC20052 United States Department of Physics University of Warwick Gibbet Hill Road CoventryCV4 7AL United Kingdom Astrophysics Research Institute Liverpool John Moores University Liverpool Science Park IC2 146 Brownlow Hill LiverpoolL3 5RF United Kingdom Max-Planck-Institut für Astrophysik Karl-Schwarzschild-Str. 1 Garching bei München85748 Germany European Southern Observatory Karl-Schwarzschild-Strasse 2 Garching bei MünchenD-85748 Germany Dipartimento di Fisica’G. Occhialini’ Università degli Studi di Milano-Bicocca P.za della Scienza 3 MilanoI-20126 Italy National Astronomical Observatory of Japan MitakaTokyo Japan Department of Physics and Astronomy University of Leicester University Road LeicesterLE1 7RH United Kingdom Department of Astronomy and Physics Padova University Italy Department of Astronomy University of California Davis United States Dip. di Fisica Universita‘di Roma La Sapienza P.le A. Moro 2 RomeI-00185 Italy Università di Roma Tor Vergata Via della Ricerca Scient

The merger of two neutron stars is predicted to give rise to three major detectable phenomena: a short burst of γ-rays, a gravitational wave signal, and a transient optical/near-infrared source powered by the synthesis of large amounts of very heavy elements via rapid neutron capture (the r-process)1–3. Such transients, named "macronovae" or "kilonovae" (refs 4-7), are believed to be centres of production of rare elements such as gold and platinum8. The most compelling evidence so far for a kilonova was a very faint near-infrared rebrightening in the afterglow of a short γ-ray burst9, 10 at z = 0.356, although findings indicating bluer events have been reported11. Here we report the spectral identification and describe the physical properties of a bright kilonova associated with the gravitational wave source GW 17081712 and γ-ray burst GRB 170817A13, 14 associated with a galaxy at a distance of 40 Mpc from Earth. Using a series of spectra from ground-based observatories covering the wavelength range from the ultraviolet to the near-infrared, we find that the kilonova is characterized by rapidly expanding ejecta with spectral features similar to those predicted by current models15, 16. The ejecta is optically thick early on, with a velocity of about 0.2 times light speed, and reaches a radius of ∼ 50 astronomical units in only 1.5 days. As the ejecta expands, broad absorption-like lines appear on the spectral continuum indicating atomic species produced by nucleosynthesis that occurs in the post-merger fast-moving dynamical ejecta and in two slower (0.05 times light speed) wind regions. Comparison with spectral models suggests that the merger ejected 0.03–0.05 solar masses of material, including high-opacity lanthanides. Copyright © 2017, The Authors. All rights reserved.

关键词： Merging

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Fermi-lat observations of high-energy behind-the-limb solar flares

arXiv

引用

arXiv 2017年

作者： Ackermann, M. Allafort, A. Baldini, L. Barbiellini, G. Bastieri, D. Bellazzini, R. Bissaldi, E. Bonino, R. Bottacini, E. Bregeon, J. Bruel, P. Buehler, R. Cameron, R.A. Caragiulo, M. Caraveo, P.A. Cavazzuti, E. Cecchi, C. Charles, E. Ciprini, S. Costanza, F. Cutini, S. D'Ammando, F. de Palma, F. Desiante, R. Digel, S.W. Di Lalla, N. Di Mauro, M. Di Venere, L. Drell, P.S. Favuzzi, C. Fukazawa, Y. Fusco, P. Gargano, F. Giglietto, N. Giordano, F. Giroletti, M. Grenier, I.A. Guillemot, L. Guiriec, S. Jogler, T. Jóhannesson, G. Kashapova, L. Krucker, S. Kuss, M. la Mura, G. Larsson, S. Latronico, L. Li, J. Liu, W. Longo, F. Loparco, F. Lubrano, P. Magill, J.D. Maldera, S. Manfreda, A. Mazziotta, M.N. Mitthumsiri, W. Mizuno, T. Monzani, M.E. Morselli, A. Moskalenko, I.V. Negro, M. Nuss, E. Ohsugi, T. Omodei, N. Orlando, E. Pal'shin, V. Paneque, D. Perkins, J.S. Pesce-Rollins, M. Petrosian, V. Piron, F. Principe, G. Rainò, S. Rando, R. Razzano, M. Reimer, O. Rubio da Costa, F. Sgrò, C. Simone, D. Siskind, E.J. Spada, F. Spandre, G. Spinelli, P. Tajima, H. Thayer, J.B. Torres, D.F. Troja, E. Vianello, G. Deutsches Elektronen Synchrotron DESY ZeuthenD-15738 Germany W. W. Hansen Experimental Physics Laboratory Kavli Institute for Particle Astrophysics and Cosmology Department of Physics SLAC National Accelerator Laboratory Stanford University StanfordCA94305 United States Università di Pisa Istituto Nazionale di Fisica Nucleare Sezione di Pisa PisaI-56127 Italy Istituto Nazionale di Fisica Nucleare Sezione di Trieste TriesteI-34127 Italy Dipartimento di Fisica Università di Trieste TriesteI-34127 Italy Istituto Nazionale di Fisica Nucleare Sezione di Padova PadovaI-35131 Italy Dipartimento di Fisica e Astronomia "G. Galilei" Università di Padova PadovaI-35131 Italy Istituto Nazionale di Fisica Nucleare Sezione di Pisa PisaI-56127 Italy Istituto Nazionale di Fisica Nucleare Sezione di Bari BariI-70126 Italy Istituto Nazionale di Fisica Nucleare Sezione di Torino TorinoI-10125 Italy Dipartimento di Fisica Università degli Studi di Torino TorinoI-10125 Italy Laboratoire Univers et Particules de Montpellier Université Montpellier CNRS IN2P3 MontpellierF-34095 France Laboratoire Leprince-Ringuet École polytechnique CNRS IN2P3 PalaiseauF-91128 France Dipartimento di Fisica "M. Merlin" dell'Università e del Politecnico di Bari BariI-70126 Italy INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica Milano via E. Bassini 15 MilanoI-20133 Italy Science Data Center RomaI-00133 Italy Istituto Nazionale di Fisica Nucleare Sezione di Perugia PerugiaI-06123 Italy Dipartimento di Fisica Università degli Studi di Perugia PerugiaI-06123 Italy INAF Istituto di Radioastronomia BolognaI-40129 Italy Dipartimento di Astronomia Università di Bologna BolognaI-40127 Italy Università Telematica Pegaso Piazza Trieste e Trento 48 NapoliI-80132 Italy Università di Udine UdineI-33100 Italy Department of Physical Sciences Hiroshima University Higashi-Hiroshima Hiroshima739-8526 Japan Laboratoire AIM CEA IRFU CNRS Université Paris Diderot Servic

We report on the Fermi-LAT detection of high-energy emission from the behind-the-limb solar flares that occurred on 2013 October 11, 2014 January 6 and 2014 September 1. The Fermi-LAT observations are associated with flares from active regions originating behind both the eastern and western limbs, as determined by STEREO. All three flares are associated with very fast Coronal Mass Ejections (CMEs) and strong Solar Energetic particle events. We present updated localizations of the > 100 MeV photon emission, hard X-ray (HXR) and EUV images and broad-band spectra from 10 keV to 10 GeV as well as microwave spectra. We also provide a comparison of the behind-the-limb flares detected by the Fermi-LAT with three on-disk flares and present a study of some of the significant quantities of these flares as an attempt to better understand the acceleration mechanisms at work during these occulted flares. We interpret the HXR emission to be due to electron bremsstrahlung from a coronal thin-target loop-top with the accelerated electron spectra steepening at semirelativistic energies. The > 100 MeV gamma-rays are best described by a pion decay model resulting from interaction of protons (and other ions) in a thick target photospheric source. The protons are believed to have been accelerated (to energies > 10 GeV) in the CME environment and precipitate down to the photosphere from the down-stream side of the CME shock and landed on the front side of the Sun, away from the original flare site and the HXR emission. Copyright © 2017, The Authors. All rights reserved.

关键词： Gamma rays

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Erratum to: Study of the spin and parity of the Higgs boson in diboson decays with the ATLAS detector

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The European Physical Journal C 2016年第3期76卷 1-14页

作者： Aad, G. Abbott, B. Abdallah, J. Abdinov, O. Aben, R. Abolins, M. AbouZeid, O. S. Abramowicz, H. Abreu, H. Abreu, R. Abulaiti, Y. Acharya, B. S. Adamczyk, L. Adams, D. L. Adelman, J. Adomeit, S. Adye, T. Affolder, A. A. Agatonovic-Jovin, T. Agricola, J. Aguilar-Saavedra, J. A. Ahlen, S. P. Ahmadov, F. Aielli, G. Akerstedt, H. Åkesson, T. P. A. Akimov, A. V. Alberghi, G. L. Albert, J. Albrand, S. Alconada Verzini, M. J. Aleksa, M. Aleksandrov, I. N. Alexa, C. Alexander, G. Alexopoulos, T. Alhroob, M. Alimonti, G. Alio, L. Alison, J. Alkire, S. P. Allbrooke, B. M. M. Allport, P. P. Aloisio, A. Alonso, A. Alonso, F. Alpigiani, C. Altheimer, A. Alvarez Gonzalez, B. Álvarez Piqueras, D. Alviggi, M. G. Amadio, B. T. Amako, K. Amaral Coutinho, Y. Amelung, C. Amidei, D. Amor Dos Santos, S. P. Amorim, A. Amoroso, S. Amram, N. Amundsen, G. Anastopoulos, C. Ancu, L. S. Andari, N. Andeen, T. Anders, C. F. Anders, G. Anders, J. K. Anderson, K. J. Andreazza, A. Andrei, V. Angelidakis, S. Angelozzi, I. Anger, P. Angerami, A. Anghinolfi, F. Anisenkov, A. V. Anjos, N. Annovi, A. Antonelli, M. Antonov, A. Antos, J. Anulli, F. Aoki, M. Aperio Bella, L. Arabidze, G. Arai, Y. Araque, J. P. Arce, A. T. H. Arduh, F. A. Arguin, J.-F. Argyropoulos, S. Arik, M. Armbruster, A. J. Arnaez, O. Arnal, V. Arnold, H. Arratia, M. Arslan, O. Artamonov, A. Artoni, G. Asai, S. Asbah, N. Ashkenazi, A. Åsman, B. Asquith, L. Assamagan, K. Astalos, R. Atkinson, M. Atlay, N. B. Auerbach, B. Augsten, K. Aurousseau, M. Avolio, G. Axen, B. Ayoub, M. K. Azuelos, G. Baak, M. A. Baas, A. E. Bacci, C. Bachacou, H. Bachas, K. Backes, M. Backhaus, M. Bagiacchi, P. Bagnaia, P. Bai, Y. Bain, T. Baines, J. T. Baker, O. K. Baldin, E. M. Balek, P. Balestri, T. Balli, F. Banas, E. Banerjee, Sw. Bannoura, A. A. E. Bansil, H. S. Barak, L. Barberio, E. L. Barberis, D. Barbero, M. Barillari, T. Barisonzi, M. Barklow, T. Barlow, N. Barnes, S. L. Barnett, B. M. Barnett, R. M. Barnovska, Z. Baroncelli, A. Barone, G. Barr, A. J. Barreiro, F. Barreiro Guimarães da Costa, J. Bart CPPM Aix-Marseille Université and CNRS/IN2P3 Marseille France Homer L. Dodge Department of Physics and Astronomy University of Oklahoma Norman USA Institute of Physics Academia Sinica Taipei Taiwan Institute of Physics Azerbaijan Academy of Sciences Baku Azerbaijan Nikhef National Institute for Subatomic Physics and University of Amsterdam Amsterdam The Netherlands Department of Physics and Astronomy Michigan State University East Lansing USA Department of Physics University of Toronto Toronto Canada Raymond and Beverly Sackler School of Physics and Astronomy Tel Aviv University Tel Aviv Israel Department of Physics Technion: Israel Institute of Technology Haifa Israel Center for High Energy Physics University of Oregon Eugene USA Department of Physics Stockholm University Stockholm Sweden The Oskar Klein Centre Stockholm Sweden INFN Gruppo Collegato di Udine Udine Italy ICTP Trieste Italy AGH University of Science and Technology Faculty of Physics and Applied Computer Science Kraków Poland Physics Department Brookhaven National Laboratory Upton USA Department of Physics Northern Illinois University De Kalb USA Fakultät für Physik Ludwig-Maximilians-Universität München Munich Germany Particle Physics Department Rutherford Appleton Laboratory Didcot UK Oliver Lodge Laboratory University of Liverpool Liverpool UK Institute of Physics University of Belgrade Belgrade Serbia II Physikalisches Institut Georg-August-Universität Göttingen Germany Laboratório de Instrumentação e Física Experimental de Partículas-LIP Lisbon Portugal Departamento de Fisica Teorica y del Cosmos and CAFPE Universidad de Granada Granada Spain Department of Physics Boston University Boston USA Joint Institute for Nuclear Research JINR Dubna Dubna Russia INFN Sezione di Roma Tor Vergata Rome Italy Dipartimento di Fisica Università di Roma Tor Vergata Rome Italy Fysiska institutionen Lunds universitet Lund Sweden P.N. Lebedev Institute of Physics Academy of Sciences

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Chiral phase transition with a chiral chemical potential in the framework of Dyson-Schwinger equations

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Physical Review D 2015年第5期91卷 056003-056003页

作者： Shu-Sheng Xu Zhu-Fang Cui Bin Wang Yuan-Mei Shi You-Chang Yang Hong-Shi Zong Key Laboratory of Modern Acoustics MOE Institute of Acoustics and Department of Physics Nanjing University Nanjing 210093 China State Key Laboratory of Theoretical Physics Institute of Theoretical Physics CAS Beijing 100190 China Department of Physics Nanjing University Nanjing 210093 China Department of Physics Huazhong University of Science and Technology Wuhan 430074 China Department of Physics and Electronic Engineering Nanjing Xiaozhuang University Nanjing 211171 China School of Physics and Mechanical-Electrical Engineering Zunyi Normal College Zunyi 563002 China Joint Center for Particle Nuclear Physics and Cosmology Nanjing 210093 China

Within the framework of Dyson-Schwinger equations , we discuss the chiral phase transition of QCD with a chiral chemical potential μ5 as an additional scale. We focus especially on the issues related to the widely accepted as well as interesting critical end point (CEP). With the help of a scalar susceptibility, we find that there might be no CEP5 in the T−μ5 plane, and the phase transition in the T−μ5 plane might be totally crossover when μ<50 MeV, which has apparent consistency with the lattice QCD calculation. Our study may also provide some useful hints to some other studies related to μ5.

关键词： CHIRALITY THERMODYNAMIC functions CHEMICAL potential GIBBS-Duhem equation NUMERICAL analysis

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Erratum to: ATLAS Run 1 searches for direct pair production of third-generation squarks at the Large Hadron Collider ATLAS Collaboration

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The European Physical Journal C 2016年第3期76卷 1-14页

作者： Aad, G. Abbott, B. Abdallah, J. Abdinov, O. Aben, R. Abolins, M. AbouZeid, O. S. Abramowicz, H. Abreu, H. Abreu, R. Abulaiti, Y. Acharya, B. S. Adamczyk, L. Adams, D. L. Adelman, J. Adomeit, S. Adye, T. Affolder, A. A. Agatonovic-Jovin, T. Agricola, J. Aguilar-Saavedra, J. A. Ahlen, S. P. Ahmadov, F. Aielli, G. Akerstedt, H. Åkesson, T. P. A. Akimov, A. V. Alberghi, G. L. Albert, J. Albrand, S. Alconada Verzini, M. J. Aleksa, M. Aleksandrov, I. N. Alexa, C. Alexander, G. Alexopoulos, T. Alhroob, M. Alimonti, G. Alio, L. Alison, J. Alkire, S. P. Allbrooke, B. M. M. Allport, P. P. Aloisio, A. Alonso, A. Alonso, F. Alpigiani, C. Altheimer, A. Alvarez Gonzalez, B. Álvarez Piqueras, D. Alviggi, M. G. Amadio, B. T. Amako, K. Amaral Coutinho, Y. Amelung, C. Amidei, D. Amor Dos Santos, S. P. Amorim, A. Amoroso, S. Amram, N. Amundsen, G. Anastopoulos, C. Ancu, L. S. Andari, N. Andeen, T. Anders, C. F. Anders, G. Anders, J. K. Anderson, K. J. Andreazza, A. Andrei, V. Angelidakis, S. Angelozzi, I. Anger, P. Angerami, A. Anghinolfi, F. Anisenkov, A. V. Anjos, N. Annovi, A. Antonelli, M. Antonov, A. Antos, J. Anulli, F. Aoki, M. Aperio Bella, L. Arabidze, G. Arai, Y. Araque, J. P. Arce, A. T. H. Arduh, F. A. Arguin, J.-F. Argyropoulos, S. Arik, M. Armbruster, A. J. Arnaez, O. Arnal, V. Arnold, H. Arratia, M. Arslan, O. Artamonov, A. Artoni, G. Asai, S. Asbah, N. Ashkenazi, A. Åsman, B. Asquith, L. Assamagan, K. Astalos, R. Atkinson, M. Atlay, N. B. Auerbach, B. Augsten, K. Aurousseau, M. Avolio, G. Axen, B. Ayoub, M. K. Azuelos, G. Baak, M. A. Baas, A. E. Baca, M. J. Bacci, C. Bachacou, H. Bachas, K. Backes, M. Backhaus, M. Bagiacchi, P. Bagnaia, P. Bai, Y. Bain, T. Baines, J. T. Baker, O. K. Baldin, E. M. Balek, P. Balestri, T. Balli, F. Banas, E. Banerjee, Sw. Bannoura, A. A. E. Bansil, H. S. Barak, L. Barberio, E. L. Barberis, D. Barbero, M. Barillari, T. Barisonzi, M. Barklow, T. Barlow, N. Barnes, S. L. Barnett, B. M. Barnett, R. M. Barnovska, Z. Baroncelli, A. Barone, G. Barr, A. J. Barreiro, F. Barreiro Guimarães da Co CPPM Aix-Marseille Université and CNRS/IN2P3 Marseille France Homer L. Dodge Department of Physics and Astronomy University of Oklahoma Norman USA Institute of Physics Academia Sinica Taipei Taiwan Institute of Physics Azerbaijan Academy of Sciences Baku Azerbaijan Nikhef National Institute for Subatomic Physics and University of Amsterdam Amsterdam The Netherlands Department of Physics and Astronomy Michigan State University East Lansing USA Department of Physics University of Toronto Toronto Canada Raymond and Beverly Sackler School of Physics and Astronomy Tel Aviv University Tel Aviv Israel Department of Physics Technion: Israel Institute of Technology Haifa Israel Center for High Energy Physics University of Oregon Eugene USA Department of Physics Stockholm University Stockholm Sweden The Oskar Klein Centre Stockholm Sweden INFN Gruppo Collegato di Udine Udine Italy ICTP Trieste Italy AGH University of Science and Technology Faculty of Physics and Applied Computer Science Kraków Poland Physics Department Brookhaven National Laboratory Upton USA Department of Physics Northern Illinois University De Kalb USA Fakultät für Physik Ludwig-Maximilians-Universität München Munich Germany Particle Physics Department Rutherford Appleton Laboratory Didcot UK Oliver Lodge Laboratory University of Liverpool Liverpool UK Institute of Physics University of Belgrade Belgrade Serbia II Physikalisches Institut Georg-August-Universität Göttingen Germany Laboratório de Instrumentação e Física Experimental de Partículas-LIP Lisbon Portugal Departamento de Fisica Teorica y del Cosmos and CAFPE Universidad de Granada Granada Spain Department of Physics Boston University Boston USA Joint Institute for Nuclear Research JINR Dubna Dubna Russia INFN Sezione di Roma Tor Vergata Rome Italy Dipartimento di Fisica Università di Roma Tor Vergata Rome Italy Fysiska institutionen Lunds universitet Lund Sweden P.N. Lebedev Institute of Physics Academy of Sciences

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