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