Physics 2D Lecture Slides Jan 15 Vivek Sharma UCSD Physics Watching an Inelastic Collision between two putty balls Relativistic Momentum and Revised Newton’s Laws Need to generalize the laws of Mechanics & Newton to confirm to Lorentz Transform G G and the Special theory of relativity: Example : p = mu S P = mv –mv = 0 P=0 Before v 1 v V=0 2 1 2 After v1 − v v2 − v −2v V −v ' = −v = 0, v2 = = , V '= v = 2 v1v v1v V v 1− 2 1− 2 1 − 2 1 + v2 c c c c −2mv ' ' , pafter = 2mV ' = −2mv pbefore = mv1' + mv2' = 2 v 1+ 2 S’ c ' p'before ≠ pafter ' 1 1 v1’=0 Before v2’ 2 V’ 1 2 After Definition (without proof) of Relativistic Momentum G mu G G With the new definition relativistic = γ mu momentum is conserved in all frames p= 1 − (u / c) 2 of references : Do the exercise New Concepts Rest mass = mass of object measured In a frame of ref. where object is at rest γ= 1 1 − (u / c) 2 u is velocity of the object NOT of a reference frame ! Nature of Relativistic Momentum m u G p= G mu 1 − (u / c) 2 G = γ mu With the new definition of Relativistic momentum Momentum is conserved in all frames of references Good old Newton Relativistic Force & Acceleration G p= G mu 1 − (u / c) 2 G = γ mu Relativistic Force And Acceleration Reason why you cant quite get up to the speed of light no matter how hard you try! G G dpG d mu F = = dt dt 1 − (u / c ) 2 use d du d = dt dt du m mu u 1 2 − − du F = ( )( ) + × 1 − (u / c ) 2 (1 − (u / c ) 2 )3 / 2 c 2 dt 2 2 2 2 mc mu mu − + du F = c 2 (1 − (u / c ) 2 )3 / 2 dt m du : Relativistic Force F = (1 − (u / c ) 2 )3 / 2 dt G G du Since A ccele ra tion a = , dt G G F 2 3/ 2 1 − (u / c ) ⇒ a= m G Note: As u / c → 1, a → 0 !!!! Its harder to accelerate when you get closer to speed of light A Linear Particle Accelerator - F q E d + E= V/d F=eE V Charged particle q moves in straight line G G Under force, work is done in a uniform electric field E with speed u on the particle, it gains G G Kinetic energy accelarates under force F=qE G G G 2 3/ 2 2 3/ 2 New Unit of Energy G du F u qE u a = = 1 − 2 = 1 − 2 dt m c m c 1 eV = 1.6x 10-19 Joules larger the potential difference V across plates, larger the force on particle A Linear Particle Accelerator G G eE 2 3/ 2 1 − (u / c) a= m PEPPEP-II accelerator schematic and tunnel view Magnetic Confinement & Circular Particle Accelerator G V G Classically B v2 F =m r v2 qvB = m r dp d (γ mu ) du F= = =γm = quB dt dt dt du u 2 (Centripetal accelaration) = dt r u2 γ m = quB ⇒ γ mu = qBr ⇒ p = qBr r G FB r Charged Form of Matter & Anti-Matter in a B Field Circular Particle Accelerator: LEP @ CERN, Geneve Magnets Keep Circular Orbit of Particles Inside A Circular Particle Accelerator @ CERN Accelerating Electrons Thru RF Cavities Test of Relativistic Momentum In Circular Accelerator G mu G G p= = γ mu 1 − (u / c ) 2 γ mu = qBr qBr γ = mu Relativistic Work Done & Change in Energy W = X2 , u=u x2 ∫ G G F .dx = x1 x1 , u=0 u ∫ 0 u W = ∫ G dp G .dx dt du G m dp dt ∴ = , substitute i n W , 2 3/2 dt u 1 − c 2 u2 1− 2 c ∴W = ∫ x1 mu p= x2 du udt dt 2 3/2 u − 1 2 c m m udu 3/2 = (change in var x → u ) mc2 1/ 2 − mc2 = γ mc2 − mc2 u u2 0 1 − c 2 1 − c 2 W o rk d one is change in Kinetic energy K 2 K = γ m c 2 − m c 2 or Total Ener gy E= γ m c 2 = K + mc 2 Why Can’s Anything go faster than light ? Lets accelerate a particle from rest, particle gains velocity & kinetic energy K= mc 2 1/ 2 u 1 − c 2 2 − mc ⇒ 2 ( K + mc ) 2 2 u2 ⇒ 1 − 2 = m 2c 4 K + mc 2 c ⇒ u = c 1− ( 2 mc = u 2 1/ 2 1 − 2 c −2 K K −2 1) (Parabolic in u Vs ) + 2 2 mc mc Non-relativistic case: K = 1 2 2K mu ⇒ u = 2 m 2 Relativistic Kinetic Energy When Electron Goes Fast it Gets “Fat” E = γ mc 2 v As → 1, γ → ∞ c Apparent Mass approaches ∞ Relativistic Kinetic Energy & Newtonian Physics Relativistic KE = γ mc 2 − mc 2 − 1 2 2 u2 1u When u << c, 1- 2 ≅ 1 − + ...smaller terms 2 2c c 2 1 1 u 2 2 2 so K ≅ mc [1 − ] − mc = mu (classical form recovered) 2 2c 2 Total Energy of a Particle E = γ mc = KE + mc 2 2 For a particle at rest, u = 0 ⇒ Total Energy E= mc 2 E = γ mc 2 ⇒ E 2 = γ 2 m 2 c 4 Relationship between P and E p = γ mu ⇒ p 2 c 2 = γ 2 m 2 u 2 c 2 ⇒ E 2 − p 2 c 2 = γ 2 m 2 c 4 − γ 2 m 2u 2 c 2 = γ 2 m 2 (c 2 − u 2 ) 2 4 m 2c 2 2 m c 2 2 2 4 2 = ( ) ( ) − = − = c u c u m c 2 2 2 u c −u 1− 2 c E 2 = p 2 c 2 + ( mc 2 ) 2 ........important relati on For p articles with zero rest mass like photon (EM waves) E E= pc or p = c (light has momentum!) Re lativistic Invariance : E 2 − p 2 c 2 = m 2 c 4 : In all Ref Frames Rest M ass is a "finger print" of the particle Mass Can “Morph” into Energy & Vice Verca • Unlike in Newtonian mechanics • In relativistic physics : Mass and Energy are the same thing • New word/concept : Mass-Energy • It is the mass-energy that is always conserved in every reaction : Before & After a reaction has happened • Like squeezing a balloon : – If you squeeze mass, it becomes (kinetic) energy & vice verca ! • CONVERSION FACTOR = C2 Mass is Energy, Energy is Mass : Mass-Energy Conservation Examine Kinetic energy Before and After Inelastic Collision: Conserved? S K=0 K = mu2 Before v 1 v V=0 2 1 2 After Mass-Energy Conservation: sum of mass-energy of a system of particles before interaction must equal sum of mass-energy after interaction E before mc 2 2 + mc 2 2 = E after = 2 Mc ⇒ M = 2m 2 > 2m u u u 1− 2 1− 2 1− 2 Kinetic energy is not lost, c c c Kinetic energy has been transformed into mass increase its transformed into more mass in final state 2 K 2 mc 2 − mc 2 ∆M = M - 2m = 2 = 2 c c u2 1− 2 c Conservation of Mass-Energy: Nuclear Fission M1 M Mc 2 = M 1c 2 u12 1− 2 c <1 + + M 2c 2 u22 1− 2 c M2 + <1 + M 3c 2 u32 1− 2 c M3 Nuclear Fission ⇒ M > M1 + M 2 + M 3 <1 Loss of mass shows up as kinetic energy of final state particles Disintegration energy per fission Q=(M – (M1+M2+M3))c2 =∆Mc2 236 92 1 U → 14553 Cs+ 90 R b +3 92 0n ∆m=0.177537u=2.9471× 10-28 kg = 165.4 MeV What makes it explosive is 1 mole U = 6.023 x 1023 Nuclei !! Relativistic Kinematics of Subatomic Particles Reconstructing Decay of a π Meson