94,247 research outputs found
Theoretical planetary mass spectra - a predition for COROT
The satellite COROT will search for close-in exo-planets around a few
thousand stars using the transit search method. The COROT mission holds the
promise of detecting numerous exo-planets. Together with radial velocity
follow-up observations, the masses of the detected planets will be known.
We have devised a method for predicting the expected planetary populations
and compared it to the already known exo-planets. Our method works by looking
at all hydrostatic envelope solutions of giant gas planets that could possibly
exist in arbitrary planetary nebulae and comparing the relative abundance of
different masses. We have completed the first such survey of hydrostatic
equilibria in an orbital range covering periods of 1 to 50 days.
Statistical analysis of the calculated envelopes suggests division into three
classes of giant planets that are distinguished by orbital separation. We term
them classes G (close-in), H, and J (large separation). Each class has distinct
properties such as a typical mass range.
Furthermore, the division between class H and J appears to mark important
changes in the formation: For close-in planets (classes G and H) the concept of
a critical core-mass is meaningless while it is important for class J. This
result needs confirmation by future dynamical analysis.Comment: 6 pages, 3 figures, MNRAS letter, accepted 2007 February
Relativistic quantum motion of spin-0 particles under the influence of non-inertial effects in the cosmic string space-time
We study solutions for the Klein-Gordon equation with vector and scalar
potentials of the Coulomb types under the influence of non-inertial effects in
the space-time of topological defects. We also investigate a quantum particle
described by the Klein-Gordon oscillator in the background space-time generated
by a string. An important result obtained is that the non-inertial effects
restrict the physical region of the space-time where the particle can be
placed. In addition, we show that these potentials can form bound states for
the relativistic wave equation equation in this kind of background.Comment: arXiv admin note: text overlap with arXiv:1608.0669
Dynamical instabilities in density-dependent hadronic relativistic models
Unstable modes in asymmetric nuclear matter (ANM) at subsaturation densities
are studied in the framework of relativistic mean-field density-dependent
hadron models. The size of the instabilities that drive the system are
calculated and a comparison with results obtained within the non-linear Walecka
model is presented. The distillation and anti-distillation effects are
discussed.Comment: 8 pages, 8 Postscript figures. Submitted for publication in Phys.
Rev.
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