Geons, anyone?
Hi again, notknowing,
notknowing said:
Einsteins field equations are nonlinear. One could interpret this to mean that curvature is itself the source of curvature (thus not only mass). Would it be possible to find a stationary (non-zero) solution of the (non-linearised) field equations without a mass being present - a kind of spacetime deformation which has an existence independent of mass ?
It sounds very much like you want to notion of a "geon", which was introduced by Wheeler under the slogan "mass without mass". Try these:
http://arxiv.org/find/gr-qc/1/OR+ti:+geons+ti:+geon/0/1/0/all/0/1
(I should caution that some of these papers make controversial assertions. Note too that there are various ways to define "mass" which may be more or less appropriate in different circumstances.)
pess5 said:
I'm pretty sure there is a soln to Einstein's field eqns for a massless universe which contains only energy.
This probably is not what you want (nothing to do with "inflation"--- by the way, I think you meant "preBB cosmology"), but there are many nontrivial exact vacuum solutions which have zero ADM mass. A large family of them was found by Papapetrou (this is a subfamily of the Ernst vacuums, the family of all stationary axisymmetric vacuum solutions to the EFE), but most of these are not asymptotically flat. A simple AF example has been discussed by Bonnor.
The issue of interpretation is often vexed in gtr, and it is not clear that these solutions are valid. In weak-field gtr, the two halves of the Ernst equation decouple, which means that you can treat sources have independently variable mass-energy density and momentum density. That is, in Newtonian gravitation, a spinning disk and a nonspinning disk (with uniform density and the same mass) give the same gravitational field, but in gtr the fields differ (the differences arise from a zero or nonzero gravitomagnetic field). But you would presmably not want to allow a source which has nonzero angular momentum but zero mass! If I recall correctly, the massless AF Bonnor vacuum does have zero Komar mass but nonzero Komar angular momentum. (I am too lazy to check this right now.)
masudr said:
Well, what if there are no quadropole moments?
masudr, I am coming into this rather late, but I guess that you meant: do systems with constant mass, angular momentum, and quadrupole moment but with time varying octupole moments (next higher order after quadrupole moments) produced gravitational radiation, according to the linearized-EFE? The answer is yes. (More pedantically, we can define moments for mass-energy and momentum of all orders, so that in addition to "mass-quadrupole moment" and so on, we can compute a "current-quadrupole moment" which gives another contribution to the radiation, and so on for higher orders.)
MeJennifer said:
So I take it between all the flowery language that the answer is yes orbits in GR are not stable, while the effect is very smalll, orbits spiral towards the center.?
Oh dear, Jennifer, I can't imagine how you might have been led to that conclusion, but be assured that it is not true! I agree with stingray and pervect that you appear to have confused closed or decaying orbits with stable orbits-- that's unfortunate, but probably not your fault (probably you were reading something which didn't bother to use the correct terms, or to note that these are distinct concepts?)
The standard definition of stable, as used in dynamical systems theory and in applications in gtr, e.g. to test particle orbits, basically means that the orbit is stable under small perturbations in the sense that small changes don't change the orbit drastically. It does NOT contradict either quasi-Keplerian motion (so that the orbits are not closed) or inspiral (aka orbital decay) due to gravitational radiation carrying away energy from the system.
Chris Hillman