Lecture

Time Coordinate in Reference Frame

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Description

This lecture discusses the importance of using a time coordinate associated with reference frames to satisfy Einstein's relativity principle. Two examples are presented: the speed of light and simultaneity, showing the relativity to the reference frame. The lecture explains the composition of velocities and introduces the concept of a time coordinate in the second reference frame. It also explores the concept of simultaneity and how it is relative to the reference frame, highlighting the impossibility of working with a single time coordinate.

In MOOC

Mechanics: Change of Reference Frame and Relativity

This module begins by explaining how to apply Newton's mechanics when the frame of reference is accelerated. Translations and rotations are considered in Lesson 15, in which context the famous "Coriolis force" comes to the fore. The Earth is a natural reference frame for us earthbound observers. However, there are experiments such as the Foucault pendulum, in which the Earth's rotation has a clear effect on the dynamics observed locally on the Earth's surface. Other less sensitive experiments, measured with

Official source

Ontological neighbourhood

Physics

Relativity: Special relativity

Related concepts (23)

Principle of relativity

In physics, the principle of relativity is the requirement that the equations describing the laws of physics have the same form in all admissible frames of reference. For example, in the framework of special relativity the Maxwell equations have the same form in all inertial frames of reference. In the framework of general relativity the Maxwell equations or the Einstein field equations have the same form in arbitrary frames of reference.

Speed of light

The speed of light in vacuum, commonly denoted c, is a universal physical constant that is exactly equal to ). According to the special theory of relativity, c is the upper limit for the speed at which conventional matter or energy (and thus any signal carrying information) can travel through space. All forms of electromagnetic radiation, including visible light, travel at the speed of light. For many practical purposes, light and other electromagnetic waves will appear to propagate instantaneously, but for long distances and very sensitive measurements, their finite speed has noticeable effects.

Special relativity

In physics, the special theory of relativity, or special relativity for short, is a scientific theory of the relationship between space and time. In Albert Einstein's 1905 treatment, the theory is based on two postulates: The laws of physics are invariant (identical) in all inertial frames of reference (that is, frames of reference with no acceleration). The speed of light in vacuum is the same for all observers, regardless of the motion of light source or observer.

Frame of reference

In physics and astronomy, a frame of reference (or reference frame) is an abstract coordinate system whose origin, orientation, and scale are specified by a set of reference points―geometric points whose position is identified both mathematically (with numerical coordinate values) and physically (signaled by conventional markers). For n dimensions, n + 1 reference points are sufficient to fully define a reference frame.

Relativity of simultaneity

In physics, the relativity of simultaneity is the concept that distant simultaneity – whether two spatially separated events occur at the same time – is not absolute, but depends on the observer's reference frame. This possibility was raised by mathematician Henri Poincaré in 1900, and thereafter became a central idea in the special theory of relativity. According to the special theory of relativity introduced by Albert Einstein, it is impossible to say in an absolute sense that two distinct events occur at the same time if those events are separated in space.

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