Upload
prudence-bender
View
23
Download
1
Embed Size (px)
DESCRIPTION
Relativistic (4-vector) Notation. y'. y. x m = ( x 0 , x 1 , x 2 , x 3 ) (c t , x , y , z ). compare: x i = ( x 1 , x 2 , x 3 ) = ( x , y , z ). v. S '. x'. S. x. z'. z. t' = g ( t - vx /c 2 ) x' = g ( x - vt ) y' = y - PowerPoint PPT Presentation
Citation preview
y
x
z
S
y'
x'
z'
S'v
x = (x0, x1, x2, x3) (ct, x, y, z)
Relativistic (4-vector) Notation
compare: xi = (x1, x2, x3) = (x, y, z)
= = v/c 1
12
t' = (t-vx/c2)x' = (x-vt)y' = yz' = z
which can be recast as:
ct' = ctxx' = xv/c)ct
xo = xo x1
x1 = x1xo
which should be compared to the coordinate-mixing of rotations:
x' = xcos ysiny' = xcos ysin
Noticing:
2222 1
1
1
1cos
abba
a
212
1
/
22sin
ab
ab
ba
b
we write:
x0'x1'x2'x3'
compared to rotations about the z-axis:
x0'x1'x2'x3'
x0
x1
x2
x3
0 0
0 0
0 0 1 0
0 0 0 1
=
x0
x1
x2
x3
0 0
0 cos sin 0
0 sin cos 0
0 0 0 1
=
3
0
/
xx
exactly same form!
World line of particlemoving in straight linealong the x-direction
event
ct
xvt1
ct1
ct´
x´
The Lorentz transformation is not exactlya ROTATION, but mechanically like one.We will consider it a generalized rotation.
But now, the old “dot product” will no longer do.It can’t guarantee invariance for many of the
quantities we know should be invariant under suchtransformations. The fix is simple and obvious…
33221100 yxyxyxyxyx
So that under a Lorentz transformation
33221100 yxyxyxyxyx
3322
0101
1010
))((
))((
yxyx
yyxx
yyxx
3322
01012
10102
))((
))((
yxyx
yyxx
yyxx
3322
002100111
1120110002
])(
)([
yxyx
yxyxyxyx
yxyxyxyx
3322
2112002
)]1()1([
yxyx
yxyx
3322
2112002
)]1()1([)()(
yxyx
yxyxyx
21
1
33221100)()( yxyxyxyxyx
To help keep track of the sign conventions, we introduce the
metric tensor: 0 0
0 0
0 0 1 0
0 0 0 = g
Then our “dot product” becomes
yxygxygx
3
0
3
0
),,,( zyxctyy
and a lowered index means the metric tensor has been applied
Notice
yxyx
we argue:
ygx
yx
yxor
contra-variant4-vector
co-variant 4-vector
x
x
xx
xxx
summed over
The lowered index just meansthat is in the appropriateform to “dot” into a vector
Since the is raised, the above multiplication gives
(x´ )
Notice:
g means has been
multiplied by themetric tensor!
And just what does g look like?
1000
0100
00
00
1000
0100
0010
0001
g
1000
0100
00
00
1000
0100
00
00
g
Now notice that
(g) =
1000
0100
00
00
1000
0100
00
00
1000
0100
00)1(
00)1(2222
2222
1000
0100
0010
0001
= g
Also notice:
T = which means
gT =g gg or
but
(g)T = gThis is because:
(g)T = TgT = g = g
1000
0100
00
00
1000
0100
00
00
g
So as an exercise in using this notation let’s look at
)()( yx
)()( ygx
ygx
yxg
The indices indicate very specific matrix or vector components/elements. These are not matrices themselves, but just numbers, which we can reorder as we wish. We still have to respect the summations over repeated indices!
yxg??
(g) = gAnd remember we just showed
xyyx
i.e.
yxyx )()( All dot products are
INVARIANT underLorentz transformations.
yxg
even for ROTATIONS as an example, considerrotations about the z-axis
331212
212100
)sincos)(sincos(
)sincos)(sincos()()(
yxyyxx
yyxxyxyx
332111221222
222122121100
sincossincossincos
sincossincossincosyx
yxyxyxyx
yxyxyxyxyx
33221100 yxxxxxyx yx
The relativistic transformations:
)(c
Epp xx
)( xpc
E
c
E )( xcpEE
suggest a 4-vector
);( pc
Ep
that also transforms by
pp )(
so pp should be an invariant!
22
2
pc
E
Ec
In the particle’s rest frame:
px = ? E = ? pp = ?0 mc2 m2c2
In the “lab” frame:
)(c
Epp xx
)( xpc
E
c
E
)0( mc = mv
= = mc
2222222)()( cmcmpp
so
2222 )1( cm
22cm
Limitations of Schrödinger’s Equation
1-particle equation
),()(),(2
),( 21
22
txxVtxxm
txt
i
),,(),()()(
),,(2
),,(2
),,(
212121
2122
2
2
2
2121
2
2
2
21
txxxxVxVxV
txxxm
txxxm
txxt
i
2-particle equation:
mutual interaction
But in many high energy reactionsthe number of particles is not conserved!
np+e++e
n+p n+p+3
e+ p e+ p + 6 + 3