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