1,061 research outputs found
Pionic Degrees of Freedom in Atomic Nuclei and Quasielastic Knockout of Pions by High-Energy Electrons
The nonlinear model of pionic condensate in nuclei by G. Preparata can be
efficiently verified by investigation of the quasielastic knockout process of
pions out of nuclei by high energy electrons. First, a momentum distribution
(MD) of the collective pions has a bright maximum at q=0.3 Gev.Second the
excitation spectrum of a recoil nucleus is concentrated at low energies E
lesser than 1MeV. The results for the pion knockout from mesonic clouds of
individual nucleons are absolutely different. The latter results are presented
both for pion and rho-meson clouds localized on nucleons.Comment: 13 pages, 3 figure
Some properties of convection in hybrid stars
It is shown that the unusual thermodynamic properties of matter within the
region of two-phase coexistence in hybrid stars result in a change of the
standard condition for beginning of convection. In particular, the thermal flux
transported by convection may be directed towards the stellar center. We
discuss favorable circumstances leading to such an effect of "inverse
convection" and its possible influence on the thermal evolution of hybrid
stars.Comment: 13 pages, 3 figures. The discussion is extended according to referees
suggestions. New references added. Accepted to MNRA
Photoelectron spectra in strong-field ionization by a high frequency field
We analyze atomic photoelectron momentum distributions induced by bichromatic
and monochromatic laser fields within the strong field approximation (SFA),
separable Coulomb-Volkov approximation (SCVA), and ab initio treatment. We
focus on the high frequency regime -- the smallest frequency used is larger
than the ionization potential of the atom. We observe a remarkable agreement
between the ab initio and velocity gauge SFA results while the velocity gauge
SCVA fails to agree. Reasons of such a failure are discussed.Comment: Completely rewritten paper. Ionization by a two-color field is adde
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