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Inertial frame of reference
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Everything about Inertial totally explained

An inertial frame of reference, or inertial reference frame, is one in which is valid, the law of inertia.
   Newton viewed the first law as valid in any reference frame moving with uniform velocity relative to the fixed stars; that is, neither rotating nor accelerating relative to the stars. Today the notion of "absolute space" is abandoned, and an inertial frame is defined as:

An inertial frame of reference is one in which the motion of a particle not subject to forces is a straight line.


Hence, with respect to an inertial frame, an object or body accelerates only when a physical force is applied, and (following Newton's first law of motion), in the absence of a net force, a body at rest will remain at rest and a body in motion will continue to move uniformly—that is, in a straight line and at constant speed. It is useful to picture this situation as if we're situated in a zero-gravity condition, but it isn't impossible to establish an inertial frame in which gravity exists. For example, an observer confined in a free-falling lift will assert that he himself is a valid inertial frame, even if he's accelerating under gravity, so long as he's no knowledge about anything outside the lift. So, strictly speaking, inertial frame is a relative concept. With this in mind, we can define inertial frames collectively as a set of frames which are stationary or moving at constant velocity with respect to each other, so that a single inertial frame is defined as an element of this set.

Equivalence of inertial reference frames

The basic principle of relativity states: "Only relative motion is observable; there's no absolute standard of rest". According to this principle, the Laws of Physics are the same in all inertial frames (otherwise the differences would set up an absolute standard). In practical terms, this equivalence of inertial reference frames means that scientists within a box moving uniformly can't determine their absolute velocity by any experiment.
   By contrast, bodies in non-inertial reference frames are subject to so-called fictitious forces (pseudo-forces); that is, forces that result from the acceleration of the reference frame itself and not from any physical force acting on the body. Examples of fictitious forces are the centrifugal force and the Coriolis force in rotating reference frames. Therefore, scientists within a box that's being rotated or otherwise accelerated (except by gravity) can measure their acceleration and angular velocity by observing the motion of an un-restrained body inside the box.

Inertial frames in Newtonian mechanics

Classical mechanics, which includes relativity, assumes the equivalence of all inertial reference frames. Newtonian mechanics makes the additional assumptions of absolute space and absolute time. Given these two assumptions, the coordinates of the same event (a point in space and time) described in two inertial reference frames are related by a Galilean transformation »

mathbf From this perspective, the speed of light is only accidentally a property of light, and is rather a property of spacetime, a conversion factor between conventional time units (such as seconds) and length units (such as meters).

Einstein’s general theory of relativity

Einstein’s general theory modifies the distinction between nominally "inertial" and "noninertial" effects by replacing special relativity's "flat" Euclidean geometry with a curved non-Euclidean metric. In general relativity, the principle of inertia is replaced with the principle of geodesic motion, whereby objects move in a way dictated by the curvature of spacetime. As a consequence of this curvature, it isn't a given in general relativity that inertial objects moving at a particular rate with respect to each other will continue to do so. This phenomenon of geodesic deviation means that inertial frames of reference don't exist globally as they do in Newtonian mechanics and special relativity.
   However, the general theory reduces to the special theory over sufficiently small regions of spacetime, where curvature effects become less important and the earlier inertial frame arguments can come back into play. Consequently, modern special relativity is now sometimes described as only a “local theory”. (However, this refers to the theory’s application rather than to its derivation.)

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