196,132 research outputs found
Simplicial minisuperspace models in the presence of a massive scalar field with arbitrary scalar coupling
We extend previous simplicial minisuperspace models to account for arbitrary
scalar coupling \eta R\phi^2.Comment: 24 pages and 9 figures. Accepted for publication by Classical and
Quantum Gravit
Anisotropic simplicial minisuperspace model
The computation of the simplicial minisuperspace wavefunction in the case of
anisotropic universes with a scalar matter field predicts the existence of a
large classical Lorentzian universe like our own at late timesComment: 19 pages, Latex, 6 figure
Intra-group diffuse light in compact groups of galaxies. HCG 79, HCG 88 and HCG 95
Deep and images of three Hickson Compact Groups, HCG 79, HCG 88 and
HCG 95, were analyzed using a new wavelet technic to measure possible
intra-group diffuse light present in these systems. The method used, OV\_WAV,
is a wavelet technic particularly suitable to detect low-surface brightness
extended structures, down to a per pixel, which corresponds to a
5--detection level in wavelet space. The three groups studied are in
different evolutionary stages, as can be judged by their very different
fractions of the total light contained in their intra-group halos: %
for HCG 79 and % for HCG 95, in the band, and HCG 88 had no
component detected down to a limiting surface brightness of . For HCG 95 the intra-group light is red, similar to the mean
colors of the group galaxies themselves, suggesting that it is formed by an old
population with no significant on-going star formation. For HCG 79, however,
the intra-group material has significantly bluer color than the mean color of
the group galaxies, suggesting that the diffuse light may, at least in part,
come from stripping of dwarf galaxies which dissolved into the group potential
well.Comment: Two suggested references added to the introductio
Irreversible processes and the accelerated-decelerated phases of the Universe
A model for the Universe is proposed where it is considered as a mixture of
scalar and matter fields. The particle production is due to an irreversible
transfer of energy from the gravitational field to the matter field and
represented by a non-equilibrium pressure. This model can simulate three
distinct periods of the Universe: (a) an accelerated epoch where the energy
density of the scalar field prevails over the matter field, (b) a past
decelerated period where the energy density of the matter field becomes more
predominant than the scalar energy density, and (c) a present acceleration
phase where the scalar energy density overcomes the energy density of the
matter field.Comment: 6 pages, 2 figures, to be published in Brazilian Journal of Physic
Questing for Algebraic Mass Dimension One Spinor Fields
This work deals with new classes of spinors of mass dimension one in
Minkowski spacetime. In order to accomplish it, the Lounesto classification
scheme and the inversion theorem are going to be used. The algebraic framework
shall be revisited by explicating the central point performed by the Fierz
aggregate. Then the spinor classification is generalized in order to encompass
the new mass dimension one spinors. The spinor operator is shown to play a
prominent role to engender the new mass dimension one spinors, accordingly.Comment: 7 pages, final version to appear in Eur. Phys. J.
Collision-Dependent Atom Tunnelling Rate in Bose-Einstein Condensates
We show that the interaction (cross-collision) between atoms trapped in
distinct sites of a double-well potential can significantly increase the atom
tunneling rate for special trap configurations leading to an effective linear
Rabi regime of population oscillation between the trap wells. The inclusion of
cross-collisional effects significantly extends the validity of the two-mode
model approach allowing it to be alternatively employed to explain the recently
observed increase of tunneling rates due to nonlinear interactions.Comment: 4 pages, 2 figures. Replaced with improved versio
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