--%>

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 : Explain Ideal gas equation Ideal gas

    Ideal gas equation: The equation that sums up the ideal gas laws in one simple equation, P V = n R T, Here V is the volume, P is the pressure, n is the

  • Q : Explain Gauss law for magnetic fields

    Gauss' law for magnetic fields (K.F. Gauss): The magnetic flux via a closed surface is zero (0); no magnetic charges present; in its differential form, div B = 0

  • Q : Explain Stefan-Boltzmann law

    Stefan-Boltzmann law (Stefan, L. Boltzmann): The radiated power P (that is the rate of emission of electromagnetic energy) of a hot body is proportional to the radiating surface area, A, and the 4th power of the thermodynamic temperature, T. The const

  • Q : Magnetism what's the unit of Curie

    what's the unit of Curie constant and how to calculate Bohr magneton from the plot of 1/Khi vs Temperature(K)?

  • Q : Problem on multiplexed channels 4

    4 channels, two with a bit-rate of 200 kbps and two with a bit-rate of 150 Kbps are to be multiplexed employing multiple slots TDM with no sync bits. a. Find out the size of a frame in bits?

    Q : Define Universal constant of gravitation

    Universal constant of gravitation: G The constant of proportionality in the Newton’s law of universal gravitation and that plays a comparable role in Sir Einstein's general relativity. This is equivalent to the 6.672 x 10-1

  • Q : Difference between the electron and a

    Write down the vital difference between the electron and a beta ray?

  • Q : Fundamental principles of the regulation

    Describe the fundamental principles of the regulation? Briefly describe the principles?

  • Q : Explain Tachyon paradox Tachyon

    Tachyon paradox: The argument explaining that tachyons (should they subsist, of course) can’t carry an electric charge. For an imaginary-massed particle travelling faster than c, less energy the tachyon has, the faster it travels, till at zero e

  • Q : What is Universal age paradox Universal

    Universal age paradox: The two most straightforward techniques of computing the age of the Universe -- via red-shift measurements, and via stellar evolution -- outcome incompatible outcomes. Recent (in mid 1990s) measurements of the distances of far-a