71 research outputs found
Thermal distributions in stellar plasmas, nuclear reactions and solar neutrinos
The physics of nuclear reactions in stellar plasma is reviewed with special
emphasis on the importance of the velocity distribution of ions. Then the
properties (density and temperature) of the weak-coupled solar plasma are
analysed, showing that the ion velocities should deviate from the Maxwellian
distribution and could be better described by a weakly-nonexstensive
(|q-1|<0.02) Tsallis' distribution. We discuss concrete physical frameworks for
calculating this deviation: the introduction of higher-order corrections to the
diffusion and friction coefficients in the Fokker-Plank equation, the influence
of the electric-microfield stochastic distribution on the particle dynamics, a
velocity correlation function with long-time memory arising from the coupling
of the collective and individual degrees of freedom. Finally, we study the
effects of such deviations on stellar nuclear rates, on the solar neutrino
fluxes, and on the pp neutrino energy spectrum, and analyse the consequences
for the solar neutrino problem.Comment: ReVTeX, 23 pages, 3 figures, to appear in the special issue
(Nonextensive statistical mechanics and thermodynamics) of the Brazilian
Journal of Physic
Numerical modelling of the quantum-tail effect on fusion rates at low energy
Results of numerical simulations of fusion rate d(d,p)t, for low-energy
deuteron beam, colliding with deuterated metallic matrix (Raiola et al. Phys.
Lett.B 547 (2002) 193 and Eur. Phys J. A 13 (2002) 377) confirm analytical
estimate given in Coraddu et al. nucl-th/0401043, taking into account quantum
tails in the momentum distribution function of target particles, and predict an
enhanced astrophysical factor in the 1 keV region in qualitative agreement with
experiments.Comment: 6 pages, without figure
Deuterium burning in Jupiter interior
We show that moderate deviations from the Maxwell-Boltzmann energy
distribution can increase deuterium reaction rates enough to contribute to the
heating of Jupiter. These deviations are compatible with the violation of
extensivity expected from temperature and density conditions inside Jupiter.Comment: 6 pages, use elsart + 1 encaspulated postscript figure. Submitted to
Physica
Weak insensitivity to initial conditions at the edge of chaos in the logistic map
We extend existing studies of weakly sensitive points within the framework of
Tsallis non-extensive thermodynamics to include weakly insensitive points at
the edge of chaos. Analyzing tangent points of the logistic map we have
verified that the generalized entropy with suitable entropic index q correctly
describes the approach to the attractor.Comment: 6 pages, 3 figure
The LUNA project: Status and first results
LUNA is a pilot project initially focused on the ^3He(^3He,^2p)^4He cross section measurement within the thermal energy region of the Sun (15–27 KeV). A compact high current 50 KV ion accelerator facility including a windowless gas target system, a beam calorimeter, and four detector telescopes has been built, tested, and installed underground at the Laboratori Nazionali del Gran Sasso. The sensitivity has been improved by more than four orders of magnitude, as compared to the previous experiment. In particular, thanks to the cosmic ray suppression, we could attain a background level of less than 1 event per week, a rate similar to the one expected from ^3He(^3He,^2p)^4He at the lower edge of the Sun thermal energy region
Fusion reactions in plasmas as probe of the high-momentum tail of particle distributions
In fusion reactions, the Coulomb barrier selects particles from the high-momentum part of the distribution. Therefore, small variations of the high-momentum tail of the velocity distribution can produce strong effects on fusion rates. In plasmas several potential mechanisms exist that can produce deviations from the standard Maxwell-Boltzmann distribution. Quantum broadening of the energy-momentum dispersion relation of the plasma quasi-particles modifies the high-momentum tail and could explain the fusion-rate enhancement observed in low-energy nuclear reaction experiments
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