149 research outputs found
On the Lie symmetries of a class of generalized Ermakov systems
The symmetry analysis of Ermakov systems is extended to the generalized case
where the frequency depends on the dynamical variables besides time. In this
extended framework, a whole class of nonlinearly coupled oscillators are viewed
as Hamiltonian Ermakov system and exactly solved in closed form
Lie Point Symmetries for Reduced Ermakov Systems
Reduced Ermakov systems are defined as Ermakov systems restricted to the
level surfaces of the Ermakov invariant. The condition for Lie point symmetries
for reduced Ermakov systems is solved yielding four infinite families of
systems. It is shown that SL(2,R) always is a group of point symmetries for the
reduced Ermakov systems. The theory is applied to a model example and to the
equations of motion of an ion under a generalized Paul trap
Thermal Behaviour of Euclidean Stars
A recent study of dissipative collapse considered a contracting sphere in
which the areal and proper radii are equal throughout its evolution. The
interior spacetime was matched to the exterior Vaidya spacetime which generated
a temporal evolution equation at the boundary of the collapsing sphere. We
present a solution of the boundary condition which allows the study of the
gravitational and thermodynamical behaviour of this particular radiating model.Comment: 10 pages, 3 figure
A group theoretic approach to shear-free radiating stars
A systematic analysis of the junction condition, relating the radial pressure
with the heat flow in a shear-free relativistic radiating star, is undertaken.
This is a highly nonlinear partial differential equation in general. We obtain
the Lie point symmetries that leave the boundary condition invariant. Using a
linear combination of the symmetries, we transform the junction condition into
ordinary differential equations. We present several new exact solutions to the
junction condition. In each case we can identify the exact solution with a Lie
point generator. Some of the solutions obtained satisfy the linear barotropic
equation of state. As a special case we regain conformally flat models which
were found previously. Our analysis highlights the interplay between Lie
algebras, nonlinear differential equations and application to relativistic
astrophysics.Comment: 11 pages, Submitted for publication, minor revision
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