Showing 1–20 of 97 results
/ Date/ Name
Jun 7, 1999Determination of neutrino incoming direction in the CHOOZ experiment and Supernova explosion location by scintillator detectorsOct 12, 2017Localized and intense energy conversion in the diffusion region of asymmetric magnetic reconnectionJan 13, 2003Search for neutrino oscillations on a long base-line at the CHOOZ nuclear power stationApr 5, 2017Turbulence in Three-Dimensional Simulations of Magnetopause ReconnectionApr 27, 2016The Effects of Turbulence on Three-Dimensional Magnetic Reconnection at the MagnetopauseOct 4, 2019Turbulence and Transport During Guide-Field Reconnection at the MagnetopauseJul 19, 1999Limits on Neutrino Oscillations from the CHOOZ ExperimentJan 5, 2014The NINJA-2 project: Detecting and characterizing gravitational waveforms modelled using numerical binary black hole simulationsJan 22, 2014Hole burning and higher order photon effects in attosecond light-atom interactionNov 13, 1996Measurement of the atmospheric neutrino flavour composition in Soudan 2Nov 7, 2004Generic Lie Color AlgebrasJun 3, 2016Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescenceJun 13, 2016Supplement: The Rate of Binary Black Hole Mergers Inferred from Advanced LIGO Observations Surrounding GW150914Jul 25, 2016Upper limits on the rates of binary neutron star and neutron-star--black-hole mergers from Advanced LIGO's first observing runOct 5, 2017Effects of Data Quality Vetoes on a Search for Compact Binary Coalescences in Advanced LIGO's First Observing RunDec 1, 2014A directed search for gravitational waves from Scorpius X-1 with initial LIGOAug 16, 2011Good Gradings of Generalized Incidence RingsSep 28, 2012Search for Gravitational Waves from Binary Black Hole Inspiral, Merger and Ringdown in LIGO-Virgo Data from 2009-2010May 10, 2012Search for gravitational waves associated with gamma-ray bursts during LIGO science run 6 and Virgo science runs 2 and 3Dec 21, 2011Upper limits on a stochastic gravitational-wave background using LIGO and Virgo interferometers at 600-1000 Hz