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Long-Baseline Neutrino Facility (LBNF) and Deep Underground Neutrino Experiment (DUNE)
The Physics Program for the Deep Underground Neutrino Experiment (DUNE) at the Fermilab Long-Baseline Neutrino Facility (LBNF) is described.
Simultaneous single-pulse observations of radio pulsars IV: flux density spectra of individual pulses
In this paper we demonstrate that a large, unexplored reservoir of information about pulsar emission exists, that is directly linked to the radiating particles and their radiation process: We present
NLO QCD corrections to t anti-t H production in hadron collisions
The Higgs boson H of the Standard Model can be searched for in the channels p pbar / pp ->t tbar H + X at the Tevatron and the LHC. The cross sections for these processes and the final-state
Tevatron-for-LHC Report: Top and Electroweak Physics
Author(s): Gerber, CE; Murat, P; Tait, TMP; Wackeroth, D; Arbuzov, A; Bardin, D; Baur, U; Benitez, JA; Berge, S; Bondarenko, S; Boos, EE; Bowen, MT; Brock, R; Bunichev, VE; Campbell, J; Canelli, F;
PSR J1756-2251: a new relativistic double neutron star system
We report the discovery during the Parkes Multibeam Pulsar Survey of PSR J1756-2251, a 28.5 ms pulsar in a relativistic binary system. Subsequent timing observations showed the pulsar to have an
Model-based asymptotically optimal dispersion measure correction for pulsar timing
In order to reach the sensitivity required to detect gravitational waves, pulsar timing array experiments need to mitigate as much noise as possible in timing data. A dominant amount of noise is
Polarized radio emission from a magnetar
We present polarization observations of the radio emitting magnetar AXP J1810-197. Using simultaneous multi-frequency observations performed at 1.4, 4.9 and 8.4 GHz, we obtained polarization
Quantized vortex states of strongly interacting bosons in a rotating optical lattice
Bose gases in rotating optical lattices combine two important topics in quantum physics: superfluid rotation and strong correlations. In this paper, we examine square two-dimensional systems at zero
The binary pulsar PSR J1811-1736: evidence of a low amplitude supernova kick
Aims: The binary pulsar PSR J1811-1736 has been identified, since its discovery, as a member of a double neutron star system. Observations of such binary pulsars allow the measurement of general
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