Pop (physics)

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In physics, pop is the sixth derivative of the position vector with respect to time, with the first, second, third, fourth, and fifth derivatives being velocity, acceleration, jerk, snap, and crackle, respectively; pop is thus the rate of change of the crackle with respect to time. [1] [2] Pop is defined by any of the following equivalent expressions:

The following equations are used for constant pop:

where

 : constant pop,
 : initial crackle,
 : final crackle,
 : initial snap,
 : final snap,
 : initial jerk,
 : final jerk,
 : initial acceleration,
 : final acceleration,
 : initial velocity,
 : final velocity,
 : initial position,
 : final position,
 : time between initial and final states.

The terms snap (also referred to as jounce ), crackle , and popfor the fourth, fifth, and sixth derivatives of positionwere inspired by the advertising mascots Snap, Crackle, and Pop. [2]

Unit and dimension

The dimensions of pop are LT−6. In SI units, this is m/s6, and in CGS units, 100 gal per quartic second.

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Jerk (physics) Rate of change of acceleration

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Guiding center

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Jounce fourth derivative of the position vector with respect to time, or the rate of change of the jerk with respect to time

In physics, jounce, also known as snap, is the fourth derivative of the position vector with respect to time, or the rate of change of the jerk with respect to time. Equivalently, it is the second derivative of acceleration or the third derivative of velocity. Jounce is defined by any of the following equivalent expressions:

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Proper acceleration

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The Einstein–Infeld–Hoffmann equations of motion, jointly derived by Albert Einstein, Leopold Infeld and Banesh Hoffmann, are the differential equations of motion describing the approximate dynamics of a system of point-like masses due to their mutual gravitational interactions, including general relativistic effects. It uses a first-order post-Newtonian expansion and thus is valid in the limit where the velocities of the bodies are small compared to the speed of light and where the gravitational fields affecting them are correspondingly weak.

The magnetic radiation reaction force is a force on an electromagnet when its magnetic moment changes. One can derive an electric radiation reaction force for an accelerating charged particle caused by the particle emitting electromagnetic radiation. Likewise, a magnetic radiation reaction force can be derived for an accelerating magnetic moment emitting electromagnetic radiation.

References

  1. Thompson, Peter M. (March 2011). "Snap, Crackle, and Pop" (PDF). Proc of AIAA Southern California Aerospace Systems and Technology Conference. p. 1. Archived from the original (PDF) on 2017-03-04. Retrieved 29 February 2020. The common names for the first three derivatives are velocity, acceleration, and jerk. The not so common names for the next three derivatives are snap, crackle, and pop.
  2. 1 2 Visser, Matt (31 March 2004). "Jerk, snap and the cosmological equation of state" (PDF). Classical and Quantum Gravity . 21 (11): 2603–2616. arXiv: gr-qc/0309109 . Bibcode:2004CQGra..21.2603V. doi:10.1088/0264-9381/21/11/006. ISSN   0264-9381 . Retrieved 17 May 2015. Snap [the fourth time derivative] is also sometimes called jounce. The fifth and sixth time derivatives are sometimes somewhat facetiously referred to as crackle and pop.