A) Isaac Newton B) Albert Einstein C) Galileo Galilei D) Stephen Hawking
A) 299,792,458 meters per second B) 100,000,000 meters per second C) 1,000,000,000 meters per second D) 500,000,000 meters per second
A) Mass B) Length C) Time D) Speed of light
A) Potential energy B) Force and acceleration C) Momentum conservation D) Mass-energy equivalence
A) Plasma B) Luminiferous aether C) Quantum vacuum D) Dark matter
A) It becomes zero B) It decreases C) It remains constant D) It increases
A) Quantum entanglement B) Alternate dimensions C) Space travel through time D) Integration of space and time into a single continuum
A) Law of conservation of energy B) Principle of relativity C) Law of inertia D) Quantum entanglement
A) James Clerk Maxwell B) Albert Einstein C) Galileo Galilei D) Isaac Newton
A) 1905 B) 1925 C) 1915 D) 1895
A) They vary based on observer's position B) They change with velocity C) They are invariant (identical) D) They depend on acceleration
A) Stay the same B) Moving clocks run slower C) Stop D) Move faster
A) They disappear B) They occur at different times C) They remain simultaneous D) Their order is reversed
A) University level B) Elementary school level C) Postgraduate level D) High school level
A) E=m/c2 B) E=mc C) E=c/m2 D) E=mc2
A) Newtonian geometry B) Euclidean geometry C) Galilean geometry D) Lorentzian geometry
A) E B) m C) L D) c
A) Galilean transformation B) The Lorentz transformation C) Euclidean transformation D) Newtonian transformation
A) Relativistic corrections B) Newtonian mechanics C) Euclidean geometry D) Galilean transformation
A) Velocities no longer simply add B) Events that appear simultaneous to one observer may not be simultaneous to another C) Time measured between two events by observers in motion differ D) Distances between two events by observers in motion differ
A) Events appear simultaneous to all observers B) Length contraction is negated C) Time dilation does not occur D) Visual observations always report events that have happened in the past
A) Newtonian geometry B) Galilean geometry C) Lorentzian geometry D) Euclidean geometry
A) 1887 B) 1864 C) 1905 D) 1632
A) Maxwell's experiment B) Einstein's 1905 paper C) Michelson–Morley experiment D) FitzGerald-Lorentz experiment
A) 1915 B) 1864 C) 1887 D) 1907
A) By using only spatial coordinates. B) Using a clock with uniform periodicity within a reference frame. C) Through acceleration measurements. D) By observing changes in velocity.
A) Acceleration. B) An event. C) The speed of light. D) A reference frame.
A) Albert Einstein. B) Isaac Newton. C) Henri Poincaré. D) James Clerk Maxwell.
A) Complete aether-drag B) Partial aether-drag C) Relativistic aberration of light D) Light-time correction
A) A⋅B = A0B0 - (A→ ⋅ B→). B) A⋅B = A0B0 + (A→ ⋅ B→). C) A⋅B = A0B0 + A1B1 + A2B2 + A3B3. D) A⋅B = A0B0 - A1B1 - A2B2 - A3B3.
A) The received frequency increases. B) The received frequency decreases. C) The frequency depends on the medium. D) The received frequency remains unchanged.
A) Δx' = Δx/γ B) Δx = Δx'γ C) Δt' = Δt/γ D) Δx' = Δxγ
A) Relativistic velocity addition B) Length contraction C) Lorentz transformation D) Time dilation
A) Alvager, T.; Farley, F. J. M. B) Rindler, Wolfgang C) Darrigol, Olivier D) Wolf, Peter; Petit, Gerard
A) 3.1 seconds B) 4 seconds C) 1.5 seconds D) 2 seconds
A) Length contraction only B) Time dilation effects C) The impossibility of faster-than-light travel D) Thomas rotation provides a resolution
A) TU Delft OPEN Publishing B) De Gruyter C) Oxford University Press D) Princeton University Press
A) Through Einstein's Eyes B) lightspeed C) Real Time Relativity D) Warp Special Relativity Simulator
A) Wave propagation B) Thermodynamics C) General relativity D) Quantum mechanics
A) Bondi K-Calculus B) Relativity Calculator: Special Relativity C) The Hogg Notes on Special Relativity D) MathPages – Reflections on Relativity
A) Physical Review A B) Isis C) Physics Letters D) Scholarpedia
A) 1964 B) 1905 C) 2005 D) 1923
A) TU Delft OPEN Books B) University of California Press C) Princeton University Press D) Nauka, Moscow
A) T. Alvager B) Peter Wolf; Gerard Petit C) Olivier Darrigol D) Wolfgang Rindler
A) The Dirac equation B) The Schrödinger equation C) The Klein-Gordon equation D) The Heisenberg uncertainty principle
A) The Sagnac effect. B) Lorentz contraction. C) Mass-energy equivalence. D) Time dilation.
A) The Meaning of Relativity B) Zur Elektrodynamik bewegter Körper C) Relativity: The Special and General Theory D) On the Electrodynamics of Moving Bodies
A) MathPages – Reflections on Relativity B) The Hogg Notes on Special Relativity C) SpecialRelativity.net D) Relativity Calculator: Special Relativity
A) sec⁻¹(β) B) cos⁻¹(β) C) tan⁻¹(β) D) sin⁻¹(β)
A) Rindler, Wolfgang B) Wolf, Peter; Petit, Gerard C) Darrigol, Olivier D) Alvager, T.; Farley, F. J. M.; Kjellman, J.; Wallin, L.
A) Neither axis is vertical B) The x axis C) The ct axis D) Both axes are vertical
A) As stationary within his frame. B) As traveling along a zig-zag path. C) In a straight line up and down. D) As moving slower than c.
A) Orthogonal, parallel, or perpendicular. B) Only timelike and spacelike. C) Timelike, spacelike, or null (lightlike). D) Dependent solely on spatial components.
A) 40,000 years B) 100,000 years C) 80,000 years D) 58,000 years
A) The traveling twin sends more signals than received. B) Because they communicate in real-time during the journey. C) Because each twin receives all signals sent by the other, despite differing experiences. D) The stationary twin does not receive any signals.
A) Coulomb potential B) Gravitational potential C) Newtonian potential D) Liénard–Wiechert potential
A) Warp Special Relativity Simulator B) Through Einstein's Eyes C) lightspeed D) Real Time Relativity
A) Einstein Online B) Relativity Calculator: Special Relativity C) Greg Egan's Foundations D) Audio: Cain/Gay (2006) – Astronomy Cast
A) Richard Feynman B) Stephen Hawking C) Robert Katz D) Carl Sagan
A) 148,000 years B) 200,000 years C) 100,000 years D) 150,000 years
A) The Hogg Notes on Special Relativity B) Audio: Cain/Gay (2006) – Astronomy Cast C) Einstein Light D) Relativity Calculator: Special Relativity
A) 2026 B) 2005 C) 1977 D) 2018
A) Δx = γΔx' B) Δt' = 0 C) Δt' eq 0 D) Δx' eq 0
A) Niels Bohr. B) Paul Langevin. C) Isaac Newton. D) Albert Einstein.
A) Lawrence Sklar B) Harvey R. Brown C) Paul Tipler D) Sergey Stepanov
A) Rindler, Wolfgang B) Alvager, T.; Farley, F. J. M. C) Darrigol, Olivier D) Wolf, Peter; Petit, Gerard
A) γ = cosh(φ). B) γ = tanh(φ). C) γ = sin(φ). D) γ is independent of rapidity.
A) The displacement depends on complete aether-drag. B) The displacement would be due to light-time correction. C) There is no displacement predicted. D) It results from aberration of light.
A) Classical Mechanics and Special Relativity B) Mechanics and Relativity C) Relativistic World D) Modern Physics (4th ed.)
A) Einstein diagrams B) Newtonian diagrams C) Galilean diagrams D) Minkowski diagrams
A) 12 years B) 5 years C) 6.5 years D) 10 years |