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
Index