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On The Evolution Of The Spectral Break In The Afterglow Of Gamma Ray Bursts
Shlomo Dado, Arnon Dar
The temporal evolution of the spectral break in the time resolved spectral energy density of the broad band afterglow of gamma ray bursts (GRBs) 091127 and 080319B was shown recent…
Possible Origin Of The Neutrino Speed Anomaly Reported By OPERA
Shlomo Dado, Arnon Dar
Recently the OPERA collaboration reported a measurement of a superluminal speed of muon neutrinos travelling through the Earth's crust between their production site at CERN and the…
Misaligned And Alien Planets From Explosive Death Of Stars
Shlomo Dado, Arnon Dar, Erez Ribak
Exoplanets whose orbit is misaligned with the spin of their host star could have originated from high-speed gas blobs, which are observed in multitudes in nearby supernova remnants…
Have the missing cosmic baryons been found?
Ehud Behar, Shlomo Dado, Arnon Dar +1
The angular power spectrum and polarization of the cosmic microwave background radiation (CMB), the relative abundances of primordial hydrogen, deuterium and helium isotopes, and t…
Can the soft X-ray opacity towards high redshift sources probe the missing baryons?
Ehud Behar, Shlomo Dado, Arnon Dar +1
Observations with the Swift satellite of X-ray afterglows of more than a hundred gamma ray bursts (GRBs) with known redshift reveal ubiquitous soft X-ray absorption. The directly m…
Determination of αS using OPAL hadronic event shapes at sqrt(s) = 91 - 209 GeV and resummed NNLO calculations
The OPAL Collaboration
Hadronic event shape distributions from e+e- annihilation measured by the OPAL experiment at centre-of-mass energies between 91 GeV and 209 GeV are used to determine the strong cou…