7 research outputs found
Single parameter quasi-particle model for QGP
We discuss a new single parameter quasi-particle model and study the
thermodynamics of (2+1)-flavor quark gluon plasma (QGP). Our model with a
single parameter explains remarkably well the lattice simulation results of
Fodor et. al. Phys. Lett. B568, 73 (2003).Comment: 9 pages, 3 figures, articl
A solution of the coincidence problem based on the recent galactic core black hole mass density increase
A mechanism capable to provide a natural solution to two major cosmological
problems, i.e. the cosmic acceleration and the coincidence problem, is
proposed. A specific brane-bulk energy exchange mechanism produces a total dark
pressure, arising when adding all normal to the brane negative pressures in the
interior of galactic core black holes. This astrophysically produced negative
dark pressure explains cosmic acceleration and why the dark energy today is of
the same order to the matter density for a wide range of the involved
parameters. An exciting result of the analysis is that the recent rise of the
galactic core black hole mass density causes the recent passage from cosmic
deceleration to acceleration. Finally, it is worth mentioning that this work
corrects a wide spread fallacy among brane cosmologists, i.e. that escaping
gravitons result to positive dark pressure.Comment: 14 pages, 3 figure
A unified scheme for flavoured mesons and baryons
The masses of mesons and baryons with various flavour combinations
for , , , , , , etc. are
computed using a confinement scheme based on harmonic approximation
with Lorentz scalar plus vector character. The residual two body coulombic
interactions and the spin-hyperfine interactions of the confined one gluon
exchange effects are perturbatively calculated and added to the confinement
energy to get the mass of the hadron. With all the parameters fixed to get ground state
masses of hadrons containing like flavour combinations, a parameter free
prediction of the leptonic decaywidths of vector mesons and their sizes are
being made. Our results on the baryonic and mesonic masses with open
flavours and the predictions on the leptonic decay widths are in good
agreement with the respective experimental values