--%>

Define Equivalence principle

Equivalence principle: The fundamental postulate of Sir Einstein’s general theory of relativity that posits that acceleration is basically indistinguishable from the gravitational field. In another words, when you are in an elevator that is utterly sealed and protected from the outside, and hence you can’t "peek outside," then when you feel a force (that is weight), it is basically not possible for you to say whether the elevator is present in a gravitational field, or whether the elevator has rockets joined to it and is accelerating "upward."

However that in practical conditions -- say, sitting in a closed room -- it would be probable to determine whether the acceleration felt was due to the uniform thrust or due to the gravitation (state, by computing the gradient of the field; if non-zero, it would point out a gravitational field instead of thrust); though, these differences could be made randomly small. The idea at the back is the equivalence principle is that it acts about the vicinity of a point, instead of over macroscopic distances. This would be not possible to state whether or not a given (random) acceleration field was caused by the thrust or gravitation by the use of physics by only.

The equivalence principle forecasts interesting general relativistic consequences since not only are the two indistinguishable to human observers, however also to the Universe as well -- any effect which occurs whenever an observer is accelerating must also occur in a gravitational field, and vice-versa.

   Related Questions in Physics

  • Q : Define Pauli Exclusion Principle Pauli

    Pauli Exclusion Principle (W. Pauli; 1925): No two similar fermions in a system, like electrons in an atom, can contain an identical set of the quantum numbers.

  • Q : Define Eddington limit Eddington limit

    Eddington limit (Sir A. Eddington): The hypothetical limit at which the photon pressure would surpass the gravitational attraction of a light-emitting body. That is, a body emanating radiation at bigger than the Eddington limit would

  • Q : Define Faraday constant Faraday

    Faraday constant: F (M. Faraday): The electric charge fetched by one mole of electrons or singly-ionized ions. It is equivalent to the product result of the Avogadro constant and the absolute value of the charge on an electron; this i

  • Q : What is Laplace equation Laplace

    Laplace equation (P. Laplace): For the steady-state heat conduction in 1-dimension, the temperature distribution is the explanation to Laplace's equation, which defines that the second derivative of temperature with respect to displac

  • Q : Explain Event horizon Event horizon:

    Event horizon: The radius which a spherical mass should be compressed to in order to convert it into a black hole, or the radius at which the time and space switch responsibilities. Once within the event horizon, it is basically impossible to escape t

  • Q : Calculate power consumed : A voltage v

    : A voltage v = 150 + j180 is applied across an impedance and the current flowing is I = 5 - j4 find ? A, impedance . B, resistance. C, reactance. D, power consumed. 

  • Q : When the intermolecular forces are

    Describe when the intermolecular forces are strongest? Briefly state it.

  • Q : Define Siemens or SI unit of an

    Siemens: S (after E.W. von Siemens, 1816-1892): The derived SI unit of an electrical conductance equivalent to the conductance of an element which has a resistance of 1 O [ohm]; this has units of O-1.

  • Q : Problem on Adiabatic law When air is

    When air is compressed adiabatically the law connecting the absolute temperature T and the pressure P is of the form T = A.Pn where A and N are constants. Show by drawing a suitable linear graph that the experimental dat

  • Q : Define Newton or SI unit of force

    Newton: N (after Sir I. Newton, 1642-1727): The derived SI unit of force, stated as the force needed to give a mass of 1 kg of an acceleration of 1 m/s2; it therefore has units of kg m/s2.