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