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Boosted objects and jet substructure at the LHC. Report of BOOST2012, held at IFIC Valencia, 23rd–27th of July 2012

European Physical Journal C Springer Nature 74:3 (2014) 2792

Authors:

A Altheimer, A Arce, L Asquith, J Backus Mayes, E Bergeaas Kuutmann, J Berger, D Bjergaard, L Bryngemark, A Buckley, J Butterworth, M Cacciari, M Campanelli, T Carli, M Chala, B Chapleau, C Chen, JP Chou, Th Cornelissen, D Curtin, M Dasgupta, A Davison, F de Almeida Dias, A de Cosa, A de Roeck, C Debenedetti, C Doglioni, SD Ellis, F Fassi, J Ferrando, S Fleischmann, M Freytsis, ML Gonzalez Silva, S Gonzalez de la Hoz, F Guescini, Z Han, A Hook, A Hornig, E Izaguirre, M Jankowiak, J Juknevich, M Kaci, D Kar, G Kasieczka, R Kogler, A Larkoski, P Loch, D Lopez Mateos, S Marzani, L Masetti, V Mateu, DW Miller, K Mishra, P Nef, K Nordstrom, E Oliver Garcia, J Penwell, J Pilot, T Plehn, S Rappoccio, A Rizzi, G Rodrigo, A Safonov, GP Salam, J Salt, S Schaetzel, M Schioppa, A Schmidt, J Scholtz, A Schwartzman, MD Schwartz, M Segala, M Son, G Soyez, M Spannowsky, I Stewart, D Strom, M Swiatlowski, V Sanchez Martinez, M Takeuchi, J Thaler, EN Thompson, NV Tran, C Vermilion, M Villaplana, M Vos, J Wacker, J Walsh
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Heavy superpartners with less tuning from hidden sector renormalisation

Journal of High Energy Physics Springer Nature 2014:3 (2014) 69
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The moduli space of heterotic line bundle models: a case study for the tetra-quadric

Journal of High Energy Physics Springer Nature 2014:3 (2014) 25

Authors:

Evgeny I Buchbinder, Andrei Constantin, Andre Lukas
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Annihilation Signals from Asymmetric Dark Matter

(2014)

Authors:

Edward Hardy, Robert Lasenby, James Unwin
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AMS-02 data confronts acceleration of cosmic ray secondaries in nearby sources

ArXiv 1402.0855 (2014)

Authors:

Philipp Mertsch, Subir Sarkar

Abstract:

We revisit the model proposed earlier to account for the observed increase in the positron fraction in cosmic rays with increasing energy, in the light of new data from the Alpha Magnetic Spectrometer (AMS-02) experiment. The model accounts for the production and acceleration of secondary electrons and positrons in nearby supernova remnants which results in an additional, harder component that becomes dominant at high energies. By fitting this to AMS-02 data we can calculate the expected concomitant rise of the boron-to-carbon ratio, as well as of the fraction of antiprotons. If these predictions are confirmed by the forthcoming AMS-02 data it would conclusively rule out all other proposed explanations, in particular dark matter annihilations or decays.
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