Response of a Spaceborn Gravitational Wave Antenna to Solar Oscillations
We investigate the possibility of observing very small amplitude low frequency solar oscillations with the proposed laser interferometer space antenna
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Torsional oscillations in the solar convection zone
Recent analysis of the helioseismic observations indicate that the previously observed surface torsional oscillations extend significantly downwards into the solar
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Reaction Front in an A+B -> C Reaction-Subdiffusion Process
We study the reaction front for the process A+B -> C in which the reagents move subdiffusively. Our theoretical description
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Momentum-Resolved Charge Excitations in a Prototype One Dimensional Mott Insulator
We report momentum resolved charge excitations in a one dimensional (1-D) Mott insulator studied using high resolution (~ 325 meV)
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The Capture of Particles by Chaotic Resonances During Orbital Migration
Because a chaotic zone can reduce the long timescale capture probabilities and cause catastrophic events such as close encounters with
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Solar Turbulence and Magnetism Studied Within a Rotating Convective Spherical Shell
We discuss recent advances made in modelling the complex magnetohydrodynamics of the Sun using our anelastic spherical harmonics (ASH) code.
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Timing Effects of Gravitational Waves from Localized Sources
Localized astronomical sources like a double stellar system, rotating neutron star, or a massive black hole at the center of
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On some inverse problems in nuclear physics
Some inverse problems in high-energy physics, neutron diffraction and NMR spectroscopy are discussed. To solve them, the Fourier integrated transformation
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The theoretical calculation of the Rossby number and the `non-local' convective overturn time for pre-main sequence and early post-main sequence stars
This paper provides estimates of convective turnover time scales for Sun-like stars in the pre-main sequence and early post-main sequence
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State Space Computation and Analysis of Time Petri Nets
The theory of Petri Nets provides a general framework to specify the behaviors of real-time reactive systems and Time Petri
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Sub-Microarcsecond Astrometry and New Horizons in Relativistic Gravitational Physics
Attaining the limit of sub-microarcsecond optical resolution will completely revolutionize fundamental astrometry by merging it with relativistic gravitational physics. Beyond
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Exciton-LO-phonon dynamics in InAs/GaAs quantum dots: Effects of zone-edge phonon damping
The dynamics of an exciton-LO-phonon system after an ultrafast optical excitation in an InAs/GaAs quantum dot is studied theoretically. Influence
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Evolution with redshift of the ICM abundances
We predict the behaviour of the abundances of $α$-elements and iron in the intracluster medium as a function of redshift
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Numerical simulations of stellar winds: polytropic models
We discuss steady-state transonic outflows obtained by direct numerical solution of the hydrodynamic and magnetohydrodynamic equations. We make use of
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A possible solution of the G-dwarf problem in the frame-work of closed models with a time-dependent IMF
In this paper we present a method to solve the G-dwarf problem in the frame-work of analytical models (based on
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On the formation of hydrogen-deficient post-AGB stars
We present an evolutionary sequence of a low mass star from the Asymptotic Giant Branch (AGB) through its post-AGB stage,
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Irradiation and mass transfer in low-mass compact binaries
We study the reaction of low-mass stars to anisotropic irradiation and its importance for the long-term evolution of compact binaries
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The Magnetic Field Sign Reversal and Evolution of Rossby and Alfven Waves Induced by Velocity Shear Oscillations on the Sun
The behaviour of the toroidal and meridional components of the solar large-scale magnetic field and linear Alfven and Rossby waves
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Modeling the evolution of Sakurai's object
Sakurai's object is a born again AGB star of the very late thermal pulse flavor. In this contribution I will
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Hadronization in Nuclear Matter
Nuclei are unique analyzers of the space-time development of jets at early stage. We argue that the gluon bremsstrahlung, rather
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Internal Rotation, Mixing and Lithium Abundances
Lithium is an excellent tracer of mixing in stars as it is destroyed (by nuclear reactions) at a temperature around
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Time dependent non-LTE calculations of ionisation in the early universe
We present a new implicit numerical algorithm for the calculation of the time dependent non-Local Thermodynamic Equilibrium of a gas
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The Dynamics of Flux Tubes in a High Beta Plasma
We suggest a new model for the structure of a magnetic field embedded high $β$ turbulent plasma, based on the
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Time dependent models for the interaction of energetic particles in the ISM
We present a general model allowing one to calculate the distribution function of energetic particles in the interstellar medium, and
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