A) Albert Einstein B) Stephen Hawking C) Galileo Galilei D) Isaac Newton
A) 1,000,000,000 meters per second B) 299,792,458 meters per second C) 500,000,000 meters per second D) 100,000,000 meters per second
A) Time B) Speed of light C) Length D) Mass
A) Potential energy B) Momentum conservation C) Force and acceleration D) Mass-energy equivalence
A) Luminiferous aether B) Dark matter C) Quantum vacuum D) Plasma
A) It becomes zero B) It decreases C) It remains constant D) It increases
A) Quantum entanglement B) Alternate dimensions C) Space travel through time D) Integration of space and time into a single continuum
A) Law of conservation of energy B) Principle of relativity C) Quantum entanglement D) Law of inertia
A) Albert Einstein B) Galileo Galilei C) Isaac Newton D) James Clerk Maxwell
A) 1925 B) 1915 C) 1905 D) 1895
A) They depend on acceleration B) They are invariant (identical) C) They vary based on observer's position D) They change with velocity
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) Postgraduate level C) High school level D) University level
A) E=c/m2 B) E=m/c2 C) E=mc2 D) E=mc
A) Newtonian geometry B) Lorentzian geometry C) Galilean geometry D) Euclidean geometry
A) c B) m C) L D) E
A) Galilean transformation B) The Lorentz transformation C) Euclidean transformation D) Newtonian transformation
A) Newtonian mechanics B) Euclidean geometry C) Galilean transformation 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) Time dilation does not occur C) Events appear simultaneous to all observers D) Visual observations always report events that have happened in the past
A) Euclidean geometry B) Lorentzian geometry C) Galilean geometry D) Newtonian geometry
A) 1887 B) 1905 C) 1864 D) 1632
A) FitzGerald-Lorentz experiment B) Michelson–Morley experiment C) Einstein's 1905 paper D) Maxwell's experiment
A) 1887 B) 1907 C) 1864 D) 1915
A) By observing changes in velocity. B) Using a clock with uniform periodicity within a reference frame. C) Through acceleration measurements. D) By using only spatial coordinates.
A) A reference frame. B) An event. C) The speed of light. D) Acceleration.
A) James Clerk Maxwell. B) Henri Poincaré. C) Isaac Newton. D) Albert Einstein.
A) Relativistic aberration of light B) Complete aether-drag C) Light-time correction 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 remains unchanged. C) The received frequency increases. D) The frequency depends on the medium.
A) Δt' = Δt/γ B) Δx = Δx'γ C) Δx' = Δxγ D) Δx' = Δx/γ
A) Lorentz transformation B) Time dilation C) Relativistic velocity addition D) Length contraction
A) Alvager, T.; Farley, F. J. M. B) Darrigol, Olivier C) Wolf, Peter; Petit, Gerard D) Rindler, Wolfgang
A) 3.1 seconds B) 4 seconds C) 1.5 seconds D) 2 seconds
A) Time dilation effects B) The impossibility of faster-than-light travel C) Thomas rotation provides a resolution D) Length contraction only
A) Princeton University Press B) De Gruyter C) TU Delft OPEN Publishing D) Oxford University Press
A) lightspeed B) Real Time Relativity C) Through Einstein's Eyes D) Warp Special Relativity Simulator
A) Wave propagation B) General relativity C) Quantum mechanics D) Thermodynamics
A) Relativity Calculator: Special Relativity B) The Hogg Notes on Special Relativity C) MathPages – Reflections on Relativity D) Bondi K-Calculus
A) Isis B) Physics Letters C) Physical Review A D) Scholarpedia
A) 2005 B) 1964 C) 1923 D) 1905
A) Princeton University Press B) TU Delft OPEN Books C) Nauka, Moscow D) University of California Press
A) Wolfgang Rindler B) Olivier Darrigol C) Peter Wolf; Gerard Petit D) T. Alvager
A) The Schrödinger equation B) The Heisenberg uncertainty principle C) The Klein-Gordon equation D) The Dirac equation
A) Mass-energy equivalence. B) Lorentz contraction. C) Time dilation. D) The Sagnac effect.
A) On the Electrodynamics of Moving Bodies B) Zur Elektrodynamik bewegter Körper C) Relativity: The Special and General Theory D) The Meaning of Relativity
A) The Hogg Notes on Special Relativity B) MathPages – Reflections on Relativity C) SpecialRelativity.net D) Relativity Calculator: Special Relativity
A) cos⁻¹(β) B) sin⁻¹(β) C) sec⁻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) Both axes are vertical B) The x axis C) The ct axis 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) Timelike, spacelike, or null (lightlike). B) Orthogonal, parallel, or perpendicular. C) Only timelike and spacelike. D) Dependent solely on spatial components.
A) 40,000 years B) 80,000 years C) 100,000 years D) 58,000 years
A) Because they communicate in real-time during the journey. B) The stationary twin does not receive any signals. C) Because each twin receives all signals sent by the other, despite differing experiences. D) The traveling twin sends more signals than received.
A) Newtonian potential B) Coulomb potential C) Gravitational potential D) Liénard–Wiechert potential
A) Through Einstein's Eyes B) Warp Special Relativity Simulator 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) Carl Sagan B) Richard Feynman C) Robert Katz D) Stephen Hawking
A) 150,000 years B) 148,000 years C) 200,000 years D) 100,000 years
A) Einstein Light B) The Hogg Notes on Special Relativity C) Audio: Cain/Gay (2006) – Astronomy Cast D) Relativity Calculator: Special Relativity
A) 2005 B) 2026 C) 2018 D) 1977
A) Δx'
eq 0 B) Δt' eq 0 C) Δx = γΔx' D) Δt' = 0
A) Isaac Newton. B) Albert Einstein. C) Niels Bohr. D) Paul Langevin.
A) Lawrence Sklar B) Harvey R. Brown C) Paul Tipler D) Sergey Stepanov
A) Darrigol, Olivier B) Rindler, Wolfgang C) Wolf, Peter; Petit, Gerard D) Alvager, T.; Farley, F. J. M.
A) γ = cosh(φ). B) γ = tanh(φ). C) γ is independent of rapidity. D) γ = sin(φ).
A) The displacement would be due to light-time correction. B) It results from aberration of light. C) There is no displacement predicted. D) The displacement depends on complete aether-drag.
A) Modern Physics (4th ed.) B) Mechanics and Relativity C) Relativistic World D) Classical Mechanics and Special Relativity
A) Newtonian diagrams B) Galilean diagrams C) Einstein diagrams D) Minkowski diagrams
A) 12 years B) 10 years C) 6.5 years D) 5 years |