Astrophysics (Index)About

relativistic speed

(a substantial fraction of the speed of light)

Relativistic speed is a speed at which the laws of relativity become significant, i.e., a speed that is more than an insignificant fraction of the speed of light (c). Non-relativistic speed refers to speeds too slow to qualify. Ultrarelativistic speed means very close to c. For example, 0.25c could be considered relativistic and 0.999c, ultrarelativistic. (Such speeds are often expressed as fractions of c.) Some of the theorizing of astrophysical phenomena consists of figuring out means by which particles observed to be moving at relativistic or ultrarelativistic speed might have achieved that velocity. Speeds close to c are also cited by giving their Lorentz factor, a number which is roughly 1 for non-relativistic speeds, and rises without bound the closer a speed is to c.

(The term relativistic velocity means roughly the same thing as relativistic speed, but a velocity is a vector that additionally indicates the direction of motion, and the relativistic speed is more precisely the vector magnitude of the relativistic velocity.)


(physics,EMR)
Further reading:
https://en.wikipedia.org/wiki/Relativistic_speed
https://en.wikipedia.org/wiki/Ultrarelativistic_limit
https://en.wiktionary.org/wiki/ultrarelativistic
https://www.oxfordreference.com/display/10.1093/oi/authority.20110803100412735
https://dictionary.obspm.fr/index.php?formSearchTextfield=relativistic+speed&showAll=1
https://dictionary.obspm.fr/index.php?formSearchTextfield=ultrarelativistic&showAll=1

Referenced by pages:
active galactic nucleus (AGN)
active galaxy
blue shift
Cherenkov detector
cosmic neutrino background (CNB)
cosmological time dilation
curvature radiation
cyclotron radiation
dark matter (DM)
GW170817
HZE ion
jet
Kepler's laws
kinetic energy (KE)
Lorentz transformation
M87
maser
Penrose Compton scattering (PCS)
Poynting vector (S)
redshift (z)
relativistic astrophysics
relativistic beaming
relativistic energy
relativistic invariance
relativistic momentum
relativity
shock wave
Solar and Heliospheric Observatory (SOHO)
solar energetic particle (SEP)
Sunyaev-Zel'dovich effect (SZ effect)
superluminal motion
supernova remnant (SNR)
suprathermal
synchrotron radiation
synchrotron self-Compton (SSC)
Van Allen belts

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