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