Stellar cooling bounds on new light particles: plasma mixing effects

Journal of High Energy Physics Springer Nature 2017:2 (2017) 33

Authors:

Edward Hardy, Robert Lasenby

Holomorphic Yukawa couplings for complete intersection Calabi-Yau manifolds

JOURNAL OF HIGH ENERGY PHYSICS (2017) ARTN 119

Authors:

S Blesneag, EI Buchbinder, A Lukas

First measurement of the muon neutrino charged current single pion production cross section on water with the T2K near detector

Physical Review D American Physical Society 95:1 (2017)

Authors:

K Abe, C Andreopoulos, M Antonova, S Aoki, A Ariga, S Assylbekov, D Autiero, S Ban, M Barbi, GJ Barker, Giles Barr, P Bartet-Friburg, M Batkiewicz, F Bay, V Berardi, S Berkman, S Bhadra, S Bienstock, A Blondel, S Bolognesi, S Bordoni, SB Boyd, D Brailsford, A Bravar, C Bronner, M Buizza Avanzini, RG Calland, T Campbell, S Cao, J Caravaca Rodríguez, SL Cartwright, R Castillo, A Cervera, D Cherdack, N Chikuma, G Christodoulou, A Clifton, J Coleman, G Collazuol, David Coplowe, L Cremonesi, A Dabrowska, G De Rosa, T Dealtry, PF Denner, C Densham, D Dewhurst, F Di Lodovico

Abstract:

The T2K off-axis near detector, ND280, is used to make the first differential cross section measurements of muon neutrino charged current single positive pion production on a water target at energies ∼0.8 GeV. The differential measurements are presented as a function of the muon and pion kinematics, in the restricted phase space defined by pπ+>200 MeV/c, pμ>200 MeV/c, cos(θπ+)>0.3 and cos(θμ)>0.3. The total flux integrated νμ charged current single positive pion production cross section on water in the restricted phase space is measured to be σ

Can black hole superradiance be induced by galactic plasmas?

(2017)

Authors:

Joseph P Conlon, Carlos AR Herdeiro

All-sky search for time-integrated neutrino emission from astrophysical sources with 7 yr of IceCube data

Astrophysical Journal Institute of Physics 835:2 (2017) 151

Authors:

K Abraham, M Ackermann, Subir Sarkar

Abstract:

Since the recent detection of an astrophysical flux of high-energy neutrinos, the question of its origin has not yet fully been answered. Much of what is known about this flux comes from a small event sample of high neutrino purity, good energy resolution, but large angular uncertainties. In searches for point-like sources, on the other hand, the best performance is given by using large statistics and good angular reconstructions. Track-like muon events produced in neutrino interactions satisfy these requirements. We present here the results of searches for point-like sources with neutrinos using data acquired by the IceCube detector over 7 yr from 2008 to 2015. The discovery potential of the analysis in the northern sky is now significantly below E 2 v doφ/dE v = 10 -12 TeV cm -2 s -1 , on average 38% lower than the sensitivity of the previously published analysis of 4 yr exposure. No significant clustering of neutrinos above background expectation was observed, and implications for prominent neutrino source candidates are discussed.