Classical general relativity effects to second order in mass, spin, and quadrupole moment
نویسندگان
چکیده
منابع مشابه
Spin half in classical general relativity
It is shown that models of elementary particles in classical general relativity will naturally have the transformation properties of a spinor if the spacetime manifold is not time orientable. From a purely pragmatic interpretation of quantum theory this explains why spinors are needed to represent particles. The models are based entirely on classical general relativity and are motivated by the ...
متن کاملSecular dynamics of coplanar, non-resonant planetary system under the general relativity and quadrupole moment perturbations
We construct a secular theory of a coplanar system of N-planets not involved in strong mean motion resonances, and which are far from collision zones. Besides the point-to-point Newtonian mutual interactions, we consider the general relativity corrections to the gravitational potential of the star and the innermost planet, and also a modification of this potential by the quadrupole moment and t...
متن کاملFrom General Relativity to Classical Dynamics
It was a project for a book, but, as my interests shifted towards a different project, I decided to stop this, and start writing my Elements for Physics. The occasional reader is invited to have a look at the Preface and Table of Contents. It may well be that she/he finds useful some parts of this text. Preface The theory of continuous media is not of universal validity but it is applicable in ...
متن کاملProposed new test of spin effects in general relativity.
The recent discovery of a double-pulsar PSR J0737-3039A/B provides an opportunity of unequivocally observing, for the first time, spin effects in general relativity. Existing efforts involve detection of the precession of the spinning body itself. However, for a close binary system, spin effects on the orbit may also be discernible. Not only do they add to the advance of the periastron (by an a...
متن کاملQuasilocal mass in general relativity.
There have been many attempts to define the notion of quasilocal mass for a spacelike two surface in spacetime by the Hamilton-Jacobi analysis. The essential difficulty in this approach is to identify the right choice of the background configuration to be subtracted from the physical Hamiltonian. Quasilocal mass should be non-negative for surfaces in general spacetime and zero for surfaces in f...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Journal of Physics Communications
سال: 2019
ISSN: 2399-6528
DOI: 10.1088/2399-6528/ab3b78