In physics, a particle is called ultrarelativistic when its speed is very close to the speed of light c.
The energy of an ultrarelativistic particle is almost completely due to its momentum (pc ≫ mc2), and thus can be approximated by E = pc. This can result from holding the mass fixed and increasing p to very large values (the usual case); or by holding the energy E fixed and shrinking the mass m to negligible values. The latter is used to derive orbits of massless particles such as the photon from those of massive particles (cf. Kepler problem in general relativity).
In general, the ultrarelativistic limit of an expression is the resulting simplified expression when pc ≫ mc2 is assumed. Or, similarly, in the limit where the Lorentz factor is very large (γ ≫ 1).
Below are some ultrarelativistic approximations in units with c = 1. The rapidity is denoted φ:
- 1 − v ≈ 1⁄2γ2
- E − p = E(1 − v) ≈ m2⁄2E = m⁄2γ
- φ ≈ ln(2γ)
- Motion with constant proper acceleration: d ≈ eaτ/(2a), where d is the distance traveled, a = dφ/dτ is proper acceleration (with aτ ≫ 1), τ is proper time, and travel starts at rest and without changing direction of acceleration (see proper acceleration for more details).
- Fixed target collision with ultrarelativistic motion of the center of mass: ECM ≈ √} where E1 and E2 are energies of the particle and the target respectively (so E1 ≫ E2), and ECM is energy in the center of mass frame.
Accuracy of the approximation
For calculations of the energy of a particle, the relative error of the ultrarelativistic limit for a speed v = 0.95c is about 10%, and for v = 0.99c it is just 2%. For particles such as neutrinos, whose γ (Lorentz factor) are usually above 106 (v very close to c), the approximation is essentially exact.
The opposite case is a so-called classical particle, where its speed is much smaller than c and so its energy can be approximated by E = mc2 + p2⁄2m.