The dipole anisotropy of AllWISE galaxies

(2017)

Authors:

M Rameez, R Mohayaee, S Sarkar, J Colin

Precise predictions for V+ jets dark matter backgrounds

European Physical Journal C Springer Berlin Heidelberg 77:12 (2017) 829

Authors:

JM Lindert, S Pozzorini, R Boughezal, JM Campbell, A Denner, S Dittmaier, A Gehrmann-De Ridder, T Gehrmann, N Glover, A Huss, S Kallweit, P Maierhöfer, ML Mangano, TA Morgan, A Mück, F Petriello, Gavin Salam, M Schönherr, C Williams

Abstract:

High-energy jets recoiling against missing transverse energy (MET) are powerful probes of dark matter at the LHC. Searches based on large MET signatures require a precise control of the Z(νν)¯ +jet background in the signal region. This can be achieved by taking accurate data in control regions dominated by Z(+−)+jet, W(ν)+jet and γ +jet production, and extrapolating to the Z(νν)¯ +jet background by means of precise theoretical predictions. In this context, recent advances in perturbative calculations open the door to significant sensitivity improvements in dark matter searches. In this spirit, we present a combination of state-of-the-art calculations for all relevant V+jets processes, including throughout NNLO QCD corrections and NLO electroweak corrections supplemented by Sudakov logarithms at two loops. Predictions at parton level are provided together with detailed recommendations for their usage in experimental analyses based on the reweighting of Monte Carlo samples. Particular attention is devoted to the estimate of theoretical uncertainties in the framework of dark matter searches, where subtle aspects such as correlations across different V+jet processes play a key role. The anticipated theoretical uncertainty in the Z(νν)¯ +jet background is at the few percent level up to the TeV range.

Magneto-optic probe measurements in low density-supersonic jets

Journal of Instrumentation IOP Publishing 12:December (2017) P12001

Authors:

Matthew Oliver, T White, P Mabey, M Kuhn-Kauffeldt, L Dohl, R Bingham, R Clarke, P Graham, R Heathcote, M Koenig, Y Kuramitsu, DQ Lamb, J Meinecke, T Michel, F Miniati, M Notley, B Reville, S Sarkar, Y Sakawa, A Schekochihin, P Tzeferacos, N Woolsey, Gianluca Gregori

Abstract:

A magneto-optic probe was used to make time-resolved measurements of the magnetic field in both a single supersonic jet and in a collision between two supersonic turbulent jets, with an electron density ⇡ 1018 cm3 and electron temperature ⇡ 4 eV. The magneto-optic data indicated the magnetic field reaches B ⇡ 200 G. The measured values are compared against those obtained with a magnetic induction probe. Good agreement of the time-dependent magnetic field measured using the two techniques is found.

Point sources from dissipative dark matter

Journal of Cosmology and Astroparticle Physics IOP Publishing 2017:12 (2017) 019-019

Authors:

Prateek Agrawal, Lisa Randall

Erratum: Constraints on Ultrahigh-Energy Cosmic-Ray Sources from a Search for Neutrinos Above 10 PeV with IceCube [Phys. Rev. Lett. 117, 241101 (2016)].

Physical review letters 119:25 (2017) 259902

Authors:

MG Aartsen, Anonymous

Abstract:

This corrects the article DOI: 10.1103/PhysRevLett.117.241101.