1,261 research outputs found
Final State Interactions in Decays of the Exotic Meson
We analyze the role of final state interactions in decay of the lighest
exotic meson, with \pi b_{1}\pi\rho\pi_{1}\pi_1(1600)\omega\pi_{1}\pi\rho$ mode cannot be generated through level
mixing.Comment: 7 pages, 11 figure
Variational formulation of Eisenhart's unified theory
Eisenhart's classical unified field theory is based on a non-Riemannian
affine connection related to the covariant derivative of the electromagnetic
field tensor. The sourceless field equations of this theory arise from
vanishing of the torsion trace and the symmetrized Ricci tensor. We formulate
Eisenhart's theory from the metric-affine variational principle. In this
formulation, a Lagrange multiplier constraining the torsion becomes the source
for the Maxwell equations.Comment: 7 pages; published versio
Towards a Relativistic Description of Exotic Meson Decays
This work analyses hadronic decays of exotic mesons, with a focus on the
lightest one, the , in a fully relativistic formalism,
and makes comparisons with non-relativistic results. We also discuss Coulomb
gauge decays of normal mesons that proceed through their hybrid components. The
relativistic spin wave functions of mesons and hybrids are constructed based on
unitary representations of the Lorentz group. The radial wave functions are
obtained from phenomenological considerations of the mass operator. Fully
relativistic results (with Wigner rotations) differ significantly from
non-relativistic ones. We also find that the decay channels are favored, in agreement with results obtained using
other models.Comment: 14 pages, 7 figure
The present universe in the Einstein frame, metric-affine R+1/R gravity
We study the present, flat isotropic universe in 1/R-modified gravity. We use
the Palatini (metric-affine) variational principle and the Einstein
(metric-compatible connected) conformal frame. We show that the energy density
scaling deviates from the usual scaling for nonrelativistic matter, and the
largest deviation occurs in the present epoch. We find that the current
deceleration parameter derived from the apparent matter density parameter is
consistent with observations. There is also a small overlap between the
predicted and observed values for the redshift derivative of the deceleration
parameter. The predicted redshift of the deceleration-to-acceleration
transition agrees with that in the \Lambda-CDM model but it is larger than the
value estimated from SNIa observations.Comment: 11 pages; published versio
Asymptotic stability of the Cauchy and Jensen functional equations
The aim of this note is to investigate the asymptotic stability behaviour of
the Cauchy and Jensen functional equations. Our main results show that if these
equations hold for large arguments with small error, then they are also valid
everywhere with a new error term which is a constant multiple of the original
error term. As consequences, we also obtain results of hyperstability character
for these two functional equations
Acceleration of the universe in the Einstein frame of a metric-affine f(R) gravity
We show that inflation and current cosmic acceleration can be generated by a
metric-affine f(R) gravity formulated in the Einstein conformal frame, if the
gravitational Lagrangian L(R) contains both positive and negative powers of the
curvature scalar R. In this frame, we give the equations for the expansion of
the homogeneous and isotropic matter-dominated universe in the case
L(R)=R+{R^3}/{\beta^2}-{\alpha^2}/{3R}, where \alpha and \beta are constants.
We also show that gravitational effects of matter in such a universe at very
late stages of its expansion are weakened by a factor that tends to 3/4, and
the energy density of matter \epsilon scales the same way as in the \Lambda-CDM
model only when \kappa*\epsilon<<\alpha.Comment: 12 pages; published versio
The cosmic snap parameter in f(R) gravity
We derive the expression for the snap parameter in f(R) gravity. We use the
Palatini variational principle to obtain the field equations and regard the
Einstein conformal frame as physical. We predict the present-day value of the
snap parameter for the particular case f(R)=R-const/R, which is the simplest
f(R) model explaining the current acceleration of the universe.Comment: 9 pages; published versio
Four-fermion interaction from torsion as dark energy
The observed small, positive cosmological constant may originate from a
four-fermion interaction generated by the spin-torsion coupling in the
Einstein-Cartan-Sciama-Kibble gravity if the fermions are condensing. In
particular, such a condensation occurs for quark fields during the
quark-gluon/hadron phase transition in the early Universe. We study how the
torsion-induced four-fermion interaction is affected by adding two terms to the
Dirac Lagrangian density: the parity-violating pseudoscalar density dual to the
curvature tensor and a spinor-bilinear scalar density which measures the
nonminimal coupling of fermions to torsion.Comment: 6 pages; published versio
On the nonsymmetric purely affine gravity
We review the vacuum purely affine gravity with the nonsymmetric connection
and metric. We also examine dynamical effects of the second Ricci tensor and
covariant second-rank tensors constructed from the torsion tensor in the
gravitational Lagrangian.Comment: 15 pages; published versio
Gravitational Field Equations and Theory of Dark Matter and Dark Energy
The main objective of this article is to derive a new set of gravitational
field equations and to establish a new unified theory for dark energy and dark
matter. The new gravitational field equations with scalar potential
are derived using the Einstein-Hilbert functional, and the scalar potential
is a natural outcome of the divergence-free constraint of the
variational elements. Gravitation is now described by the Riemannian metric
, the scalar potential and their interactions, unified by the
new gravitational field equations. Associated with the scalar potential
is the scalar potential energy density , which represents a new type of
energy caused by the non-uniform distribution of matter in the universe. The
negative part of this potential energy density produces attraction, and the
positive part produces repelling force. This potential energy density is
conserved with mean zero: . The sum of this new potential
energy density and the coupling energy between the
energy-momentum tensor and the scalar potential field gives
rise to a new unified theory for dark matter and dark energy: The negative part
of this sum represents the dark matter, which produces attraction, and the
positive part represents the dark energy, which drives the acceleration of
expanding galaxies. In addition, the scalar curvature of space-time obeys
. Furthermore, the new field equations resolve a
few difficulties encountered by the classical Einstein field equations.Comment: Some statements are made more precise and a conclusion section is
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