Modelling SN Type II: microphysics
HALO - a Helium and Lead Observatory
Spin dependent limits on WIMP-proton scattering cross-section from PICASSO
Lecture 11 Neutrino Losses and Advanced Stages of Stellar Evolution - I
Does WMAP data constrain the lepton asymmetry of the Universe to be zero? M. Lattanzi*, R. Ruffini, G.V. Vereshchagin Dip. di Fisica - Università di Roma.
E 3
Some Open Problems in Nuclear Large Amplitude Collective Motion Aurel Bulgac University of Washington Funding: DOE grants No. DE-FG02-97ER41014 (UW NT.
© A. Nitzan, TAU PART B: Main results and phenomenology A. Nitzan.
Study QGP in different Centrality Most Central events (highest multiplicity), e.g. top 5% central, i.e. 5% of the events with largest multiplicity Mid.
FERMI LEVEL AND EFFECT OF TEMPERATURE ON SC. At absolute zero all the electronic states of the valence band are full and those of conduction band are.
Railway Project
“Characterizing many-body systems by observing density fluctuations” Wolfgang Ketterle
