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Uniform low-speed expansion of the observer energy, momentum and kinetic energy of a massive four-momentum
Statement
Let be the oriented time-oriented affine Minkowski model (Oriented time-oriented affine Minkowski space (the spacetime primitives)), , let be future unit with , and let with and future timelike, . Let , , and be the observer energy, spatial momentum, kinetic energy and invariant mass of Observer energy, spatial momentum, invariant mass, rest energy and kinetic energy of a four-momentum, put as in Norms of four-velocity and four-acceleration, and the observer rest-space decomposition,(c), and let and be the Lorentz factor and relative velocity of Norms of four-velocity and four-acceleration, and the observer rest-space decomposition,(d); then satisfies , and , and Positivity, mass shell and kinetic energy of the observer quantities of a four-momentum,(b) gives , , and .
Let , suppose , put , and let be as in The uniform second-order Taylor remainder of on , so that and with . Then:
(a) and for the common real number , and
(b) with , and moreover and .
(c) Every constant above depends only on , so the estimates are uniform over all future unit , all and all with ; if (equivalently , ) then , , and . The lemma is a statement about the mathematical model only; it asserts no measured quantity, no approximation of a physical theory and no error estimate for any experiment.
Facts & Assumptions
Given: The affine Minkowski model , , a future unit , with and future timelike with , the projection , the numbers and , a bound with , and .
The observer quantities: , , for nonzero future causal , and after the constant is fixed; is the unique decomposition of along and (Observer energy, spatial momentum, invariant mass, rest energy and kinetic energy of a four-momentum).
Projection and relative velocity: is linear with image , kernel , , and the restriction of to is positive definite with norm ; for future unit one has , , , , , and if and only if (Norms of four-velocity and four-acceleration, and the observer rest-space decomposition,(c),(d)).
Observer identities: for with constant and future timelike, , and as above, one has , , , and (Positivity, mass shell and kinetic energy of the observer quantities of a four-momentum,(b)).
Uniform Taylor remainder: for and , with ; in particular and (The uniform second-order Taylor remainder of on ).
Model and powers: the model data are those of Oriented time-oriented affine Minkowski space (the spacetime primitives); on and ; rational powers such as are those of Rational powers of a positive base and integer powers those of Integer powers .
Scalar absolute values satisfy , , and for (Absolute value in an ordered field, Basic properties of the absolute value). The rest-space norm supplied by [L2] (Norms of four-velocity and four-acceleration, and the observer rest-space decomposition,(c)) satisfies for .
Proof
Relative velocity and the Taylor form of . The map is linear by [L2], so and ; the vector is future unit and , so [L2],(d) gives , , and . By [L4] applied to we have with ; define .
The observer identities. By [L3] at these data, , , , and ; define .
Translating into norms. Since , we have , and also . Both expressions are nonnegative because , and .
Part (a), the expansions. By steps 1.1 and 1.2, using from step 1.3, and by the definition of in [L1].
Part (a), the bounds. By step 1.1, using step 1.3; the second displayed bound is .
Part (b). By step 1.2, with . Norm homogeneity [L6] gives ; since , the bound on of The uniform second-order Taylor remainder of on ,(b) gives where the final inequality uses and . The norm identity and are those of step 1.2.
Uniformity and the case . The remainders and and the bounds of steps 2.2 and 2.3 depend on the state only through , and , and their constants depend on alone, so the estimates hold uniformly over all future unit , all and all with . If then by step 1.1, so and by [L2],(d), whence by [L4], , , and steps 1.2 and 2.1 give , , ; conversely gives , and is the same case.
Conclusion. Steps 2.1 and 2.2 are clauses (a), step 2.3 is clause (b) including the norm identity and , and step 3.1 is clause (c) with the uniformity statement and the case; no step used more than the stated hypotheses , and the model's normalization, and the statement concerns the mathematical model only.
Depends on
The uniform second-order Taylor remainder of on
Positivity, mass shell and kinetic energy of the observer quantities of a four-momentum
Norms of four-velocity and four-acceleration, and the observer rest-space decomposition
Observer energy, spatial momentum, invariant mass, rest energy and kinetic energy of a four-momentum
Oriented time-oriented affine Minkowski space (the spacetime primitives)
Rational powers of a positive base
Integer powers
Absolute value in an ordered field
Basic properties of the absolute value
Dependency tree · 2 levels
Sources
- B. Crowell, Special Relativity, revision 2020-12-10 (author-published undergraduate textbook, 246 PDF pages); signature (+---) converted to (-+++) and c = 1 formulas restored to x^0 = c t; Section 4.2 pp. 82-86 (relativistic kinetic energy; Example 5 p. 86, the Newtonian prediction eV = (1/2)mv^2), Section 4.3.3 Example 8 p. 91 (the Newtonian limit v = p/m), Section 4.3.4 p. 96 (p = m gamma v; the momentum of a material particle approaches infinity as its speed approaches c) and problems 11-12 p. 116 (expand K = m(gamma-1) and p = m gamma v in Taylor series; show the first terms are the nonrelativistic expressions)
- S. M. Carroll, Lecture Notes on General Relativity, arXiv:gr-qc/9712019v1 (1997); signature (-+++) with c = 1. Chapter 1 printed p. 27, equations (1.98)-(1.101) (PDF p. 34): for small v, p^0 = m + (1/2)mv^2 (rest energy plus kinetic energy) and p^1 = mv (Newtonian momentum); Chapter 4 printed pp. 105-106 (PDF pp. 112-113): the Newtonian limit, the slow-motion condition (4.10) and the weak static field
- D. Tong, General Relativity (Cambridge Part III lecture notes, 2019), Section 1.2.2 pp. 14-16 (relativistic free-particle action and the Lorentz factor gamma = (1-|xdot|^2/c^2)^(-1/2)) and Section 1.2.3 pp. 16-19, in particular the Taylor expansion (1.22) on printed p. 17 (-mc^2 + (m/2)|xdot|^2 - m Phi(x) + ... obtained by expanding the square root) (author-hosted copy of the official Cambridge PDF)