In relativity, rapidity is an alternative to speed as a measure of rate of motion. On parallel velocities (say, in one-dimensional space) rapidities are simply additive, unlike speeds at relativistic velocities. For low speeds, rapidity and speed are proportional, but for high speeds, rapidity takes a larger value. The rapidity of light is infinite.
Using the inverse hyperbolic function artanh, the rapidity w corresponding to velocity v is w = artanh(v / c). For low speeds, w is approximately v / c. The speed of light c being finite, any velocity v is constrained to the interval −c < v < c and the ratio v / c satisfies −1 < v / c < 1. Since the inverse hyperbolic tangent has the unit interval (−1, 1) for its domain and the whole real line for its range, the interval −c < v < c maps onto −∞ < w < ∞.
In 1908 Hermann Minkowski explained how the Lorentz transformation could be seen as simply a hyperbolic rotation of the spacetime coordinates, i.e., a rotation through an imaginary angle. This angle therefore represents (in one spatial dimension) a simple additive measure of the velocity between frames. The rapidity was used by Whittaker 1910  and by Varićak 1910. The name "rapidity" is due to Alfred Robb 1911  and this term was adopted by many subsequent authors, such as Varićak 1912, Silberstein (1914), Morley (1936) and Rindler (2001). The development of the theory of rapidity is mainly due to Varićak in writings from 1910 to 1924.
In one spatial dimension
The rapidity φ arises in the linear representation of a Lorentz boost as a vector-matrix product
The matrix Λ(w) is of the type with p and q satisfying p2 − q2 = 1, so that (p, q) lies on the unit hyperbola. Such matrices form the indefinite orthogonal group O(1,1) with one-dimensional Lie algebra spanned by the anti-diagonal unit matrix, showing that the rapidity is the coordinate on this Lie algebra. This action may be depicted in a spacetime diagram. In matrix exponential notation, Λ(w) can be expressed as , where Z is the anti-diagonal unit matrix
It is not hard to prove that
This establishes the useful additive property of rapidity: if A, B and C are frames of reference, then
where wPQ denotes the rapidity of a frame of reference Q relative to a frame of reference P. The simplicity of this formula contrasts with the complexity of the corresponding velocity-addition formula.
As we can see from the Lorentz transformation above, the Lorentz factor identifies with cosh w
Proper acceleration (the acceleration 'felt' by the object being accelerated) is the rate of change of rapidity with respect to proper time (time as measured by the object undergoing acceleration itself). Therefore the rapidity of an object in a given frame can be viewed simply as the velocity of that object as would be calculated non-relativistically by an inertial guidance system on board the object itself if it accelerated from rest in that frame to its given speed.
The product of β and γ appears frequently, and is from the above arguments
Exponential and logarithmic relations
From the above expressions we have
The Doppler-shift factor associated with rapidity w is .
In more than one spatial dimension
In more than one spatial dimension rapidities lie in a hyperbolic space having unit radius of negative curvature and they may be combined by the hyperbolic law of cosines. Rapidities with directions inclined at an angle have a resultant rapidity given by
This was one of the first results to be proved in the hyperbolic theory of special relativity. Note that the two rapidities must be added sequentially "head to tail"; it is not possible to combine rapidities starting from a common origin as can be done with velocity vectors in Euclidean space. This is the failure of equipollence in hyperbolic space.
Directed values of rapidity form a hyperbolic space) of unit radius of negative curvature and can be represented by geodesics on the hyperboloid model. The metric tensor corresponds to the proper acceleration (see above).
Rapidity in two dimensions can be usefully visualized using the Poincaré disk. Points at the edge of the disk correspond to infinite rapidity. Geodesics correspond to steady accelerations. The Thomas precession is equal to minus the angular deficit of a triangle, or to minus the area of the triangle.
In experimental particle physics
The energy E and scalar momentum |p| of a particle of non-zero (rest) mass m are given by:
With the definition of φ
and thus with
the energy and scalar momentum can be written as:
So rapidity can be calculated from measured energy and momentum by
However, experimental particle physicists often use a modified definition of rapidity relative to a beam axis
where pz is the component of momentum along the beam axis. This is the rapidity of the boost along the beam axis which takes an observer from the lab frame to a frame in which the particle moves only perpendicular to the beam. Related to this is the concept of pseudorapidity.
Notes and references
- Minkowski, H., Fundamental Equations for Electromagnetic Processes in Moving Bodies" 1908
- Sommerfeld, Phys. Z 1909
- "A History of the Theories of the Aether and Electricity" 1910. In a later edition of this book in 1953 the rapidity is used consistently for the theory
- "Optical Geometry of Motion" p.9
- See his papers, available in translation in Wikisource
- Robb 1910, Varićak 1910, Borel 1913
- Silberstein L:The Theory of Relativity 1914 pp.178,179
- John A. Rhodes & Mark D. Semon (2003) "Relativistic velocity space, Wigner rotation, and Thomas precession", American Journal of Physics 72(7):943–961
- Amsler, C. et al., "The Review of Particle Physics", Physics Letters B 667 (2008) 1, Section 38.5.2
- Whittaker, E. T. (1910). "A history of the theories of aether and electricity": 441. Retrieved 22 January 2016.
- Robb, Alfred (1911). Optical geometry of motion, a new view of the theory of relativity. Cambridge: Heffner & Sons.
- Borel E (1913) La théorie de la relativité et la cinématique, Comptes Rendus Acad Sci Paris 156 215-218; 157 703-705
- Silberstein, Ludwik (1914). The Theory of Relativity. London: Macmillan & Co.
- Vladimir Karapetoff (1936) "Restricted relativity in terms of hyperbolic functions of rapidities", American Mathematical Monthly 43:70.
- Frank Morley (1936) "When and Where", The Criterion, edited by T.S. Eliot, 15:200-2009.
- Wolfgang Rindler (2001) Relativity: Special, General, and Cosmological, page 53, Oxford University Press.
- Shaw, Ronald (1982) Linear Algebra and Group Representations, v. 1, page 229, Academic Press ISBN 0-12-639201-3.
- Walter, Scott (1999). "The non-Euclidean style of Minkowskian relativity" (PDF). In J. Gray. The Symbolic Universe: Geometry and Physics. Oxford University Press. pp. 91–127.(see page 17 of e-link)
- Varićak V (1910), (1912), (1924) See Vladimir Varićak#Publications