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