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