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We report on the multi-epoch observations of H2O maser emission in star forming region OH 43.8-0.1 carried out with VLBI
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arxiv
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We prove the no-go theorem that the gravivector $(h_{5μ})$ and graviscalar $(h_{55})$ cannot have any on-shell propagation on the Randall-Sundrum
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arxiv
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We discuss the junction conditions in the context of the Randall-Sundrum model with the Gauss-Bonnet interaction. We consider the $Z_2$
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arxiv
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As it was recently shown by Derishev etal (1999), initial GRB ejecta are likely to contain comparable number of protons
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arxiv
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We investigate the evolution of initially metal-free, low-mass Red Giant stars through the He core flash at the tip of
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arxiv
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Using quantum electrodynamics as an example, a dependence of physical predictions of quantum field theory in a finite perturbation theory
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arxiv
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We develop a method for constructing asymptotic solutions of finite-difference equations and implement it to a relativistic Schroedinger equation which
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arxiv
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We present non-perturbative results for the constants needed for on-shell $O(a)$ improvement of bilinear operators composed of Wilson fermions. We
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arxiv
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It is shown that in presence of URCA shell pulsational energy losses due to neutrino emission and nonequilibrium beta heating
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arxiv
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The Local Bubble (LB) is an X-ray emitting region extending 100 pc in radius in the Galactic plane and 300
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arxiv
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The so-called Unitary Gauge Puzzle is re-examined in the light of a set of gauge dependence identities discovered by Kobes,
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arxiv
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We derive the stellar and circumstellar parameters of the Galactic compact planetary nebula Hen 2-90 with two models: the classical
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arxiv
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In the spirit of general relativity, spacetime should become curved due to the presence of a particle of a given
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arxiv
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We discuss decay of unstable particles and pair annihilation of stable heavy particles that occur in the cosmic medium, from
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arxiv
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Recently, I showed that the "standard model" of solar system formation is wrong,yielding the contradiction of terrestrial planets having insufficiently
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arxiv
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The quantum black hole model with a self-gravitating spherically symmetric thin dust shell as a source is considered. The shell
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arxiv
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It is shown that conventional mass renormalization, when applied to photonic or gluonic corrections to unstable particle propagators, leads to
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arxiv
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Accretion disks and nuclear shell burning are present in some symbiotic stars (SS) and probably all supersoft X-ray binaries (SSXBs).
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arxiv
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We implement the dynamical renormalization group (DRG) using the hard thermal loop (HTL) approximation for the real-time nonequilibrium dynamics in
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arxiv
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We reconsider the rejuvenation mechanism as proposed by Shull, Fesen, & Saken (1989). These authors suggest that an active pulsar
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arxiv
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Pair annihilation of heavy stable particles that occurs in the early universe is reconsidered including the off-shell effect not properly
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arxiv
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A semiclassical approach for calculating shell effects, that has been used in atomic and plasma physics, is applied to describe
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arxiv