Galilean & Special Relativity

விளையாடிக் கற்றுக்கொள்ளுங்கள்

ஆற்றல் சம்பாதிக்க இந்த கேள்விகளுக்குப் பதிலளியுங்கள், பின்னர் மீன் பிடித்து ஆராயுங்கள். கணக்கு தேவையில்லை.

கல்வியாளர்களுக்கு: Galilean & Special Relativity (Physics, HL)-க்கான தயாரான பாட ஸ்லைடுகள், திருப்புதல் குறிப்புகள் — உங்கள் பாடத்தில் அவற்றைப் பயன்படுத்தவும், அல்லது கற்பவர்கள் நேரலை விளையாட்டாக விளையாடும் ஊடாடும் வகுப்பு செயல்பாடாக தலைப்பை இயக்கவும்.

பாட குறிப்புகள்

Reference Frames

  • A reference frame is a set of coordinates used to record the position and time of events.
  • In your own reference frame you are always at rest, even though you may be moving relative to other objects.
  • Different observers in different frames interpret the direction and speed of a moving object differently, and both can be correct.
  • An inertial reference frame is a non-accelerating frame; all inertial frames move at constant velocity relative to each other.
  • There is no absolute reference frame in the Universe — everything is always moving relative to everything else.
  • Exam questions use phrases like 'relative to...' or 'from the reference frame of...' to tell you which frame is measuring the event.

Galilean Relativity

  • Galilean relativity states that Newton's laws of motion are the same in all inertial reference frames.
  • An object moving with constant velocity in one frame will have a constant (but different) velocity in another frame.
  • Galilean transformation equations convert coordinates between frames: x' = x − vt and x = x' + vt.
  • The y and z coordinates and the time t are the same in both frames because relative motion is only along the x direction.
  • The prime notation (') denotes the moving reference frame; v is the velocity of the moving frame.
  • Time is absolute in Galilean relativity: t = t' in all inertial frames.

Galilean Velocity Addition

  • For objects moving in the same direction as the moving frame, the velocities add: u = u' + v.
  • For objects moving in the opposite direction, subtract: u = v − u' (or u = u' + (−v)).
  • To find the velocity measured in the moving frame: u' = u − v.
  • Velocities are vectors, so always account for direction — set a positive direction based on the velocity v of the moving frame.
  • This velocity addition works only for speeds much less than the speed of light.
  • A quick sketch labelling stationary frame S, moving frame S', and the velocities helps avoid sign errors.

Postulates of Special Relativity

  • First postulate: The laws of physics are the same in all inertial frames of reference.
  • Second postulate: The speed of light c in a vacuum is the same in all inertial frames of reference.
  • Both a moving and a stationary observer will always measure the same speed of light, c.
  • Galilean relativity treats space and time as fixed and absolute, but this fails near the speed of light.
  • At speeds close to c, space and time become relative — lengths and time intervals depend on the frame of reference.
  • Galilean velocity addition predicts speeds greater than c (e.g. 0.7c + 0.5c = 1.2c), which is impossible.

Lorentz Transformations

  • The Lorentz factor is γ = 1 / √(1 − v²/c²); since v < c, γ is always greater than 1.
  • Lorentz transformation equations correct Galilean transformations for speeds close to c.
  • From frame S to S': x' = γ(x − vt) and t' = γ(t − vx/c²).
  • From frame S' to S: x = γ(x' + vt') and t = γ(t' + vx'/c²).
  • Unlike Galilean transformations, time is not absolute: t ≠ t' when speeds are close to c.
  • When v is given as a fraction of c, the c cancels in the γ calculation — no need to substitute 3 × 10⁸ m s⁻¹.

Relativistic Velocity Addition

  • For relativistic speeds, use the Lorentz velocity addition equations instead of simple addition.
  • u = (u' + v) / (1 + u'v/c²) gives the velocity measured from the stationary frame.
  • u' = (u − v) / (1 − uv/c²) gives the velocity measured from the moving frame.
  • The signs in the numerator and denominator must match — be careful with direction.
  • Relativistic velocity addition ensures no object can be measured to travel faster than c.
  • Answers for relativistic velocities are often best given in terms of c.

Space-Time Interval

  • Some quantities are invariant — the same in all inertial frames: proper time, proper length, and the space-time interval.
  • The space-time interval is defined as (Δs)² = (cΔt)² − (Δx)².
  • Although Δt and Δx differ between frames, Δs is the same in all inertial reference frames.
  • Space and time are connected as four coordinates (x, y, z, t) for an event.
  • cΔt is a distance in metres, so Δs is also measured in metres.
  • The space-time interval is used in space-time diagrams.

Proper Time and Proper Length

  • Proper time Δt₀ is the time interval between two events measured in the frame where the events occur at the same place.
  • Proper length L₀ is the length measured in the frame where the object is at rest relative to the observer.
  • Proper time and proper length are invariant quantities.
  • An observer at rest relative to an object measures its proper length.
  • An observer moving relative to an event measures a longer time interval than the proper time.
  • Proper quantities can be measured in either the moving or stationary frame — it depends on which frame is at rest relative to the object or event.

Time Dilation and Length Contraction

  • Time dilation: a stationary observer sees clocks in a moving frame run slower.
  • The dilated time is given by Δt = γΔt₀, where Δt₀ is the proper time.
  • Length contraction: a moving object is measured to be shorter in the direction of motion.
  • The contracted length is L = L₀/γ, where L₀ is the proper length.
  • Both effects become significant only at speeds close to the speed of light.
  • The muon experiment demonstrates both effects: muons reach the ground because their lifetime is dilated from Earth's frame and the distance is contracted from the muon's frame.

Light clock and time dilation

Light clock and time dilation

Simultaneity and Space-Time Diagrams

  • Events that are simultaneous in one inertial frame may not be simultaneous in another moving relative to it.
  • This is a direct consequence of the second postulate — the constancy of the speed of light.
  • Space-time diagrams represent events with space on one axis and time (often ct) on the other.
  • The space-time interval between two events is the same for all inertial observers on a space-time diagram.
  • The sign of cΔt' in space-time interval calculations determines the temporal ordering of events.

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பயிற்சி கேள்விகள்

இலவச முன்னோட்டம் — 65-இல் 8 கேள்விகள். அனைத்தையும் பார்க்க பதிவு செய்யவும்.
  1. 1.Which of the following best defines a reference frame?

    Easy
    • AA set of coordinates to record the position and time of events
    • BThe speed of light in a vacuum
    • CA device used to measure time dilation
    • DThe length of an object measured at rest
  2. 2.What is an inertial reference frame?

    Easy
    • AA frame that is accelerating
    • BA non-accelerating reference frame
    • CA frame where the speed of light is zero
    • DA frame that is always stationary
  3. 3.State the two postulates of Special Relativity.

    Easy
    • AThe laws of physics are the same in all inertial frames, and the speed of light in a vacuum is constant in all inertial frames.
    • BThe laws of physics change with velocity, and the speed of light depends on the observer's motion.
    • CTime and space are absolute, and the speed of light is infinite.
    • DThe laws of physics are the same in all frames, and the speed of light varies with the source's velocity.
  4. 4.Proper length is the length of an object measured in a reference frame where the object is at rest.

    Easy

    True or false?

  5. 5.A car travels at 25 m s⁻¹ relative to the road. Another car, B, travels in the opposite direction at 30 m s⁻¹ relative to the road. What is the velocity of Car A relative to Car B?

    Medium
    • A55 m s⁻¹
    • B-5 m s⁻¹
    • C5 m s⁻¹
    • D-55 m s⁻¹
  6. 6.Which of the following quantities are invariant in all inertial reference frames? (Select all that apply)

    Medium
    • AProper time
    • BProper length
    • CSpace-time interval
    • DVelocity of light in vacuum
    • ETime interval between two events
  7. 7.What is the Lorentz factor γ for a speed of 0.5c?

    Easy
    • A1.15
    • B1.20
    • C1.10
    • D1.25
  8. 8.Match each term with its correct definition.

    Medium
    • Proper time
    • Proper length
    • Inertial reference frame
    • Space-time interval
    • The time interval between two events measured in the frame where they occur at the same place
    • The length measured in the frame where the object is at rest
    • A non-accelerating reference frame
    • An invariant quantity in all inertial frames

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இந்த தலைப்பிற்கான ஒவ்வொரு கேள்வியையும், ஸ்லைடுகளையும், ஃப்ளாஷ் கார்டுகளையும் மற்றும் திருப்புதல் குறிப்புகளையும் பார்க்க இலவச கணக்கை உருவாக்கவும்.

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