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19922026
most citedExperimental and Theoretical Challenges in the Search for the Quark Gluon Plasma: The STAR Collaboration's Critical Assessment of the Evidence from RHIC Collisions

3.4k citations

Showing 2002 · astro-phShow all

10 papers · 2 filters

astro-ph2002★ 15 cited

Extraction of cluster parameters with future Sunyaev-Zel'dovich observations

Nabila Aghanim, Steen H. Hansen, Sergio Pastor +1

The Sunyaev-Zel'dovich (SZ) effect of galaxy clusters is characterized by three parameters: Compton parameter, electron temperature and cluster peculiar velocity. In the present st…

astro-ph2002★ 46 cited

A search for TeV gamma-ray emission from SNRs, pulsars and unidentified GeV sources in the Galactic plane in the longitude range between -2 deg and 85 deg

HEGRA-Collaboration, F. A. Aharonian

Using the HEGRA system of imaging atmospheric Cherenkov telescopes, one quarter of the Galactic plane (-2 deg < l < 85 deg) was surveyed for TeV gamma-ray emission from point sourc…

astro-ph2002★ 20 cited

Neutrino Masses in Astroparticle Physics

G. G. Raffelt

The case for small neutrino mass differences from atmospheric and solar neutrino oscillation experiments has become compelling, but leaves the overall neutrino mass scale m_nu unde…

astro-ph2002★ 587 cited

Monte Carlo Study of Supernova Neutrino Spectra Formation

Mathias Th. Keil, Georg G. Raffelt, Hans-Thomas Janka

The neutrino flux and spectra formation in a supernova core is studied by using a Monte Carlo code. The dominant opacity contribution for nu_mu and nu_tau is elastic scattering on…

astro-ph2002★ 184 cited

An unidentified TeV source in the vicinity of Cygnus OB2

F. A. Aharonian, A. Akhperjanian, M. Beilicke +2

Deep observation (~113 hrs) of the Cygnus region at TeV energies using the HEGRA stereoscopic system of air Cerenkov telescopes has serendipitously revealed a signal positionally i…

astro-ph2002★ 151 cited

Flavor oscillations in the supernova hot bubble region: Nonlinear effects of neutrino background

Sergio Pastor, Georg Raffelt

The neutrino flux close to a supernova core contributes substantially to neutrino refraction so that flavor oscillations become a nonlinear phenomenon. One unexpected consequence i…