The Special Theory of Relativity Chapter III 1. Relativistic dynamics 2. Momentum and energy 3. E=mc2 4. Relativistic particle scattering Excercise Relativistic Momentum The formula for relativistic momentum can be derived by requiring that the conservation of momentum during collisions remain valid in all inertial reference frames. Note: that does NOT mean that the momentum is equal in different reference frames Go over this and derive ! Result p= mv 1 − v2 / c2 = γm v Relativistic Force Newtons second law remains valid (without proof) dp d d mv F= = γmv = dt dt dt 1 − v 2 / c 2 1) For every physical law it has to be established how they transform in relativity (under Lorentz transformations) 2) Quantities (like F) not the same in reference frames Relativistic acceleration dp d dγ dv = γmv = γm + mv F= dt dt dt dt dγ = γm a + m v dt The force vector does not point in the same direction as the acceleration vector dγ d v = 1 − 2 dt dt c 2 −1 / 2 1 v = − 1 − 2 2 c 2 −3 / 2 v − 2v ⋅ 2 = γ 3 2 c c Note: in case of acceleration γ is not constant Relativistic Mass From the momentum: p= mv 1 − v2 / c2 = γm v Gamma and the rest mass are combined to form the relativistic mass: mrel = m 1 − v2 / c2 Relativistic Energy Work done to increase the speed of a particle from v=0 (i-state) to v=v (f state): f f f f dp dp W = ∫ Fdx = ∫ dx = ∫ vdt = ∫ vdp = ∫ d ( pv ) − ∫ pdv i i dt i dt i i i f f ∫ d ( pv ) = i f f pv i = (γmv )v f v mv i 0 1 − v2 / c2 − ∫ pdv = − ∫ dv = mc vdp = d ( pv) − pdv because 2 1− v / c 2 2 v = mc 2 1 − v 2 / c 2 − mc 2 0 use So: W = γmv + 2 mc 2 γ − mc 2 ( γ 2v 2 + c 2 ) = m − mc 2 = (γ − 1)mc 2 ( ) d v 1 − v 2 / c 2 = − 2 / 1 − v 2 / c 2 dv c γ Kinetic energy of the particle is K = (γ − 1)mc 2 1) Amount of kinetic energy depends on inertial frame 2) Amount of kinetic energy reduces to classical value at low v 3) Note 1 K ≠ mv 2 2 Mass and Energy The kinetic energy K = (γ − 1)mc 2 Can be written as the total energy: Where the difference is the rest energy: E = γmc 2 = mc 2 1 − v2 / c2 E = mc 2 The last equation is Einstein famous equation implying that mass is equivalent to energy The energy of a particle at rest. Note that mc2 is the same as seen from all reference frames; It is an invariant upon frame transformation Mass, Energy, Momentum Energy E = γmc 2 Momentum p = γmv Combining these relations gives E = p c +m c 2 2 2 Hence also the following Is an invariant under Lorentz transformations 2 4 E −p c 2 2 2 Mass, Energy, Momentum for light particles Light particles have no “rest” mass (m=0), but they have energy E = p c +m c 2 2 2 2 4 hence Energy in the quantum picture E h Hence momentum p = = c λ E p= c E = hν = hc λ Compton scattering A photon (is a light particle) collides with an electron and its energy (so its wavelength) must change !! Before collision hc photon E = hf = electron Ee = me c 2 λ p= h λ After collision hc λ' photon E'= electron e Etot = γme c 2 p' = h λ' pe = γme v e Ekin = (γ − 1)me c 2 Write the momentum conservation equations along the x-coordinate and along the y-coordinate. Write the energy conservation equation. Then solve the equations and determine the wavelength λ’ for angle φ. Compton scattering Conservation of energy hc λ = hc + (γ − 1)me c 2 λ' Conservation of momentum h Along x: Along y: Three equations with 3 unknowns, eliminate v and θ Compton scattering: λ = 0= h cos φ + γme v cosθ λ' h sin φ − γme v sin θ λ' h (1 − cosφ ) λ'= λ + me c Compton scattering Arthur Compton ∆λ = h (1 − cosφ ) = λC (1 − cosφ ) me c The Nobel Prize in Physics 1927 "for his discovery of the effect named after him" Note that λC ~ 0.00243 nm So the effects is not so well visible with visible light Compton performed his experiment with x-rays Doppler Shift for Light The Doppler shift for light for c=constant in all inertial frames. λ0 = c∆t0 = c / f 0 Two effects in relativistic Doppler 1) Moving waves + 2) Time dilation!! 1) λ = c∆t − v∆t 2) ∆t = ∆t0 / 1 − v 2 / c 2 λ = (c − v )∆t = (c − v )∆t0 1 − v2 / c2 = λ0 c−v c+v When source moving toward observer Doppler Shift for Light Hence, one can derive the observed frequency and wavelength: If the source and observer are moving away from each other, v changes sign. Remember: higher pitch, blue shift when moving toward each other Doppler Shift for Light Speeding through a red light. A driver claims that he did not go through a red light because the light was Doppler shifted and appeared green. Calculate the speed of a driver in order for a red light to appear green. λ = 500nm ; λ0 =650 nm v = 0.26 c
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