Newtonian Relativity ¾A reference frame in which Newton’s laws are valid is called an inertial frame ¾Newtonian principle of relativity or Galilean invariance
If Newton’s laws are valid in one reference frame, then they are also valid in a reference frame moving at uniform velocity relative to the first system
Thus this moving frame is also an inertial frame
1 Newtonian Relativity ¾Consider
2 Newtonian Relativity ¾Galilean transformation
¾Note time is the same in both systems
3 Newtonian Relativity ¾Note Newton’s laws are valid in both frames
The force and acceleration are the same in both frames
There is no way to detect which frame is moving and which is at rest
d 2 y′ d 2 y F′ = ma′ = m = m = ma = F y y dt′2 dt2 y y d 2 x′ d 2 (x − vt) d 2 x F′ = ma′ = m = m = m = F x x dt′2 dt2 dt2 x
4 Lorentz Transformation ¾We immediately see the Galilean transformation is inconsistent with Einstein’s postulates If the velocity of light = c in frame K, the velocity of light = c – V in frame K’ ¾The Lorentz transformation satisfies Einstein’s postulates and also reduces to the Galilean transformation at low velocities ¾A derivation is given in Thornton and Rex p30-31
5 Lorentz Transformation x′ = γ (x − vt) x = γ (x′ + vt′) y′ = y y = y′ z′ = z z = z′ t′ = γ (t − vx / c2 ) t = γ (t′ + vx′/ c2 )
γ 1 1 where = = 1− β 2 v2 1− c2 6 Lorentz Transformation ¾Time dilation revisited ’ ’ ’ Let Δt = t2 –t1 be the proper time interval ’ ’ measured by a clock fixed at x0 in K γ x′V x′V ′ 2 ′ 0 t2 = (t2 + 2 γ) = (t2 + 2 ) γ c c x′V x′V t = (t′ + 1 ) = (t′ + 0 ) 1 1 c2 γ 1 c2
Δt = t2 − t1 = γΔt′
¾The clocks in S read a time longer than the proper time. The moving clock in S’ runs slow. 7 x Lorentz Transformation ¾Length contraction revisited ’ Consider a measuring rod with proper length Δx = ’ ’ 2 -x1 . The interval Δx as viewed in S must have the positions measured at the same time t0 in S. x′ = γ (x −Vt ) = γ (x −Vt ) 2 γ 2 2 2 0 x′ = (x −Vt ) = (x −Vt ) 1 1 1 γ 1 0 Δx = Δx′/γ
¾The length of the moving object as measured in S is shorter than the proper length
8 Lorentz Transformation ¾Clock synchronization revisited
Consider two clocks synchronized in S’. Clock B’ at ’ ’ x2 and clock A’ at x1 . What times do they read at time t0 in S? γ ⎛ x2V ⎞ tB′ = ⎜t0 − ⎟ ⎝ c2 ⎠ γ ⎛ x1V ⎞ t′A = ⎜t0 − ⎟ ⎝ c2 ⎠ V V L V t′ − t′ = −γ ()x − x = −()x′ − x′ = − 0 B A 2 1 c2 2 1 c2 c2
Agrees with results from the homework 9 Beta and Gamma
β =
10 Invariants ¾Invariant quantities have the same value in all inertial frames
In the next homework, you’ll show s2 = x2 + y2 + z2 − (ct)2 s′2 = x′2 + y′2 + z′2 − (ct′)2 s2 = s′2 2 s is the same for all inertial frames
11 Invariants ¾Consider two events 1 and 2 ¾We define the spacetime interval as 2 2 2 Δs = Δx -(cΔt) ¾Three cases 2 Lightlike (Δs =0) The two events can be connected only by a light signal 2 Spacelike (Δs >0) The two events are not causally connected. We can find an inertial frame where the events occur at the same time but at different positions in space 2 Timelike (Δs <0) The two events are causally connected. We can find an inertial frame where the events occur at the same position in space but at different times
12 Addition of Velocities ¾Recall the Galilean transformation between two frames K and K’ where K’ moves with velocity v with respect to K
Consider an object moving with velocity u in K and u’ in K’ x′ = x − vt dx′ d(x − vt) dx = = − v dt′ dt dt u′ = u − v
13 Galilean Transformation
x′ = x − vt x = x′ + vt y′ = y y = y′ z′ = z z = z′ t′ = t t = t′
¾Note time is the same in both systems
14 Addition of Velocities ¾We know the Lorentz transformation should be used instead so
dx γ (dx′ + vdt′) u′x + v ux = = = dt ⎡ ⎛ v ⎞ ⎤ ⎛ v ⎞ γ dt′ + dx′ 1+ u′ ⎢ ⎜ 2 ⎟ ⎥ ⎜ 2 ⎟ x ⎣ ⎝ c ⎠ ⎦ ⎝ c ⎠ similarly
u′y uy = ⎡ ⎛ v ⎞ ⎤ γ 1+ u′ ⎢ ⎜ 2 ⎟ x ⎥ ⎣ ⎝ c ⎠ ⎦
u′z uz = ⎡ ⎛ v ⎞ ⎤ γ 1+ u′ ⎢ ⎜ 2 ⎟ x ⎥ ⎝ c ⎠ ⎣ ⎦ 15 Lorentz Transformation x′ = γ (x − vt) x = γ (x′ + vt′) y′ = y y = y′ z′ = z z = z′ t′ = γ (t − vx / c2 ) t = γ (t′ + vx′/ c2 )
γ 1 1 where = = 1− β 2 v2 1− c2 16 Addition of Velocities ¾Swapping primed and unprimed variables and letting v go to –v u − v u′ = x x ⎛ v ⎞ 1− ⎜ ⎟ux ⎝ c2 ⎠
uy u′y = ⎡ ⎛ v ⎞ ⎤ γ 1− u ⎢ ⎜ 2 ⎟ x ⎥ ⎣ ⎝ c ⎠ ⎦
uz u′z = ⎡ ⎛ v ⎞ ⎤ γ 1− ⎜ ⎟u ⎢ c2 x ⎥ ⎣ ⎝ ⎠ ⎦ 17 Addition of Velocities
¾Example - let u’x=c, u’y=0, u’z=0 (c +V ) u = = c, u = 0, u = 0 x ⎛ cV ⎞ y z ⎜1+ ⎟ ⎝ c2 ⎠
¾Example - let u’x=0, u’y=c, u’z=0 c u = V , u = , u = 0 x y γ z θ u γV tan = x = uy c 18 Addition of Velocities ¾A rocket blasts off from the earth at v=0.90c ¾A second rocket follows in the same direction at velocity 0.98c ¾What is the relative velocity of the rockets using a Galilean transformation ¾What is the relative velocity of the rockets using a Lorentz transformation?
19 Lorentz Transformation ¾Last time we argued that y = y′ and z = z′ γ ¾The most general linearα transformation for x=f(x’,t’) is γ ⎛ α ⎞ x = x′ + t′ = ⎜ x′ + t′⎟ ⎝ γ ⎠ ¾At low velocities, γ→1 and α/γ→V x = γ (x′ +Vt′) ¾The inverse transformation is the same except for the sign of relative motion x′ = γ (x −Vt)
20 Lorentz Transformation ¾For a light pulse in S we have x=ct ¾For a light pulse in S’ we have x’=ct’ ¾Then x = ct = γ (ct′ +Vt′)= γ (c +V )t′ x′ = c()()t′ = ct −Vt = c −V t γ () ct′ = c −V ()cγ+V t′ γ γ c 1 γ = V 2 1− c2 21 Lorentz Transformation ¾For the t transformation x′ = γ (x −Vt) γx′γ= []()x′ +Vt′ −Vt γ ⎛ 1 ⎞ x′ t = t′ +γ ⎜ − ⎟ ⎝ ⎠ V γ ⎛ Vx′⎞ t = γ ⎜t′ + ⎟ ⎝ c2 ⎠
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