50 84 v 4 1 0 Se p 20 01 What is general relativity silent on ?
نویسنده
چکیده
In general relativity the gravitational field is a manifestation of spacetime curvature and unlike the electromagnetic field is not a force field. A body falling toward the Earth is represented by a geodesic worldline which means that no force is acting on it. If a body is on the Earth’s surface, however, its worldline is no longer geodesic and it is subjected to a force. The nature of that force is an open question in general relativity. The aim of this paper is to outline an approach toward resolving it which was initiated by Fermi in 1921. General relativity provides a consistent no-force explanation of gravitational interaction of bodies following geodesic paths. However, it is silent on the nature of the very force we regard as gravitational the force acting upon a body deviated from its geodesic path due to its being at rest in a gravitational field. A non-resistant motion (i.e. motion by inertia) of a body in both special relativity (in flat spacetime) and general relativity (in curved spacetime) is represented by a geodesic worldline whereas a body represented by a non-geodesic worldline is subjected to a force whose nature is inertial in both special and general relativity. It should be specifically stressed that the conclusion of the non-gravitational nature of the force acting on a body at rest in a gravitational field follows from general relativity itself [7]: as a body supported in a gravitational field is deviated from its geodesic path, which means that it is prevented from moving non-resistantly (by inertia), it is subjected to an inertial force (since a body prevented from moving by inertia is subjected to such an inertial force). That is why ”there is no such thing as the force of gravity” in general relativity [8]. What has been traditionally called the gravitational force in the Newtonian gravitational theory (i) the force acting on a body at rest in a gravitational field, and (ii) the force a falling body is subjected to turned out to be (i) an inertial force, and (ii) no force at all in general relativity. That a body falling in a gravitational field is subjected to no force is nicely explained by general relativity in terms of spacetime curvature. However, like the Newtonian physics general relativity provides no insight into the nature of inertial forces. Here it will be shown that a corollary of general relativity that the propagation of electromagnetic signals (for short light) in a gravitational field is anisotropic in conjunction with the classical electromagnetic mass theory [1]-[6] sheds some light on the nature of the force acting on a classical charged particle deviated from its geodesic path. Consider a classical [9] electron at rest in the non-inertial reference frame N of an observer supported in the Earth’s gravitational field. Following Lorentz [4] and Abraham [5] we assume that the electron charge is uniformly distributed on a spherical shell. The repulsion of the charge elements of an electron in uniform motion in flat spacetime cancels out exactly and there is no net force acting on the electron. As we shall see below, however, the anisotropic velocity of light in N (i) gives rise to a self-force acting on an electron deviated from its geodesic path by disturbing the balance of the mutual repulsion of its charge elements, and (ii) makes a free electron fall in N with an acceleration g in order to balance the repulsion of its charge elements. No force is acting upon a falling electron (whose worldline is geodesic) but if it is prevented from falling (i.e. deviated from its geodesic path) the average velocity of light with respect to it becomes anisotropic and disturbs the balance of the mutual repulsion of the elements of its charge which results in a self-force trying to force the electron to fall. This force turns out to be precisely equal to the gravitational force F = mg, where m = U/c represents the passive gravitational mass of the classical electron and U is the energy of its field. As the coefficient m in front of g is precisely equal to U/c
منابع مشابه
ar X iv : g r - qc / 0 10 90 68 v 1 1 9 Se p 20 01 Entropic Dynamics ∗
I explore the possibility that the laws of physics might be laws of inference rather than laws of nature. What sort of dynamics can one derive from well-established rules of inference? Specifically, I ask: Given relevant information codified in the initial and the final states, what trajectory is the system expected to follow? The answer follows from a principle of inference, the principle of m...
متن کاملHousehold food insecurity and diet diversity after the major 2010 landslide disaster in Eastern Uganda: a cross-sectional survey.
In 2010, a landslide in Bududa, Eastern Uganda, killed about 350 people and nearly 1000 affected households were resettled in Kiryandongo, Western Uganda. A cross-sectional survey assessed household food insecurity and diet diversity among 1078 affected and controls. In Bududa, the affected had a lower adjusted mean score of food insecurity than controls - 9·2 (se 0·4) v. 12·3 (se 0·4) (P<0·01)...
متن کاملar X iv : g r - qc / 0 50 90 51 v 1 1 4 Se p 20 05 Gravity and the Quantum : Are they Reconcilable ?
General relativity and quantum mechanics are conflicting theories. The seeds of discord are the fundamental principles on which these theories are grounded. General relativity, on one hand, is based on the equivalence principle, whose strong version establishes the local equivalence between gravitation and inertia. Quantum mechanics, on the other hand, is fundamentally based on the uncertainty ...
متن کامل0 10 50 83 v 2 1 2 Se p 20 01 General relativistic analysis of peculiar velocities
We give a careful general relativistic and (1+3)-covariant analysis of cosmological peculiar velocities induced by matter density perturbations in the presence of a cosmological constant. In our quasi-Newtonian approach, constraint equations arise to maintain zero shear of the non-comoving fundamental worldlines which define a Newtonian-like frame, and these lead to the (1+3)-covariant dynamica...
متن کاملar X iv : g r - qc / 0 41 01 04 v 2 2 8 Se p 20 05 CAUSAL SITES AS QUANTUM GEOMETRY
We propose a structure called a causal site to use as a setting for quantum geometry, replacing the underlying point set. The structure has an interesting categorical form, and a natural " tangent 2-bundle, " analogous to the tangent bundle of a smooth manifold. Examples with reasonable finiteness conditions have an intrinsic geometry, which can approximate classical solutions to general relati...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2008