Date post: | 21-Dec-2015 |
Category: |
Documents |
View: | 213 times |
Download: | 0 times |
/18/18
Introduction Paths through time Interference Direction of time Early universe
Unidirectionality of time induced by T violation
Joan VaccaroCentre for Quantum Dynamics
Griffith UniversityAustralia
BU FUBU FU
BU FU
BU FU BU FU
BU FUBU FU BU FU
BU FU BU FU
( )N
11
/18/18
Introduction Paths through time Interference Direction of time Early universe
22
Direction of time arrows of time (Eddington)
thermodynamic (entropy doesn’t decrease)
cosmological (expanding universe)
electromagnetic (spontaneous emission not absorption)
psychological (remember past not future)
matter-antimatter, … (CP violation favours matter)
description of dynamical systems is time-symmetric
Introduction
[The Nature Of The Physical World, 1928]
unidirectionality of time problem
2
2
d x F
dt m ˆd i
Hdt
BUT why do we experience only one direction of time?
This is the
?
time
/18/18
Introduction Paths through time Interference Direction of time Early universe
Time reversal operator
)(t )(ˆ tT
p
p
L
L
[Wigner, Group theory (1959]
ˆ ˆ ˆT U K
unitary operator
anti-unitary operator- action is complex conjugation
* *ˆ ˆ ˆ0 1 0 1K a b a K b K † † ˆˆ ˆ ˆ ˆ 1K K K K
Typical Schrodinger equation Backwards evolution is simply backtracking the forwards evolution
ˆi Ht
ˆ ˆHT
1ˆ ˆ ˆ ˆ ˆi T T HT Tt
1ˆ ˆ ˆ ˆT HT H
33
t
y
forwards
“backwards”H H
mirror symmetry
/18/18
Introduction Paths through time Interference Direction of time Early universe
But kaons don’t behave this way
1ˆ ˆ ˆ ˆT HT H
Violation of time reversal invariance- a small (0.2%) violation of CP & T invariance in neutral kaon decay- discovered in 1964 by Cronin & Fitch (Nobel Prize 1980)- partially accounts for observed dominance of matter over antimatter
gives time asymmetric dynamics
What effect does this have on the direction of time?
u s_
boson,neutral, ½ mp
lifetime 108s
44
Conventional answer: nothing!!!
1ˆ ˆ ˆT HT
t
y
forwards
“backwards”
H
broken mirror
a fundamental time asymmetry
/18/18
Introduction Paths through time Interference Direction of time Early universe
where
and = Hamiltonian for forward time evolution.
Model of the universe:▀ it is closed in the sense
that it does not interact with any other physical system
▀ it has no external clocks and so analysis needs to be unbiased with respect to the direction of time
▀ both versions of the Hamiltonian shouldappear in the dynamical equation of motion
Forwards and Backwards evolutionEvolution of state over time interval in the forward direction
0
0ˆ( ) ( )F FU
ˆ ˆ( ) expF FU iH ˆ
FH
( 1)
Preprint arXiv:0911.4528
55
Paths through time
/18/18
Introduction Paths through time Interference Direction of time Early universe
66
Evolution of state over time interval in the backward direction
where
and = Hamiltonian for backward time evolution.
0
0ˆ( ) ( )B BU
ˆ ˆ( ) expB BU iH 1ˆ ˆ ˆ ˆ
B FH T H T
( 1)
▀ and are probability
amplitudes for the system to evolve from to
via two paths in time
▀ we have no basis for favouring one path over the other
so assign an equal statistical weighting to each
using Feynman’s sum over histories
[Feynman Rev. Mod. Phys. 20, 367 (1948)]
0ˆ ( )FU 0
ˆ ( )BU
0 0
BU FU
Constructing paths:
/18/18
Introduction Paths through time Interference Direction of time Early universe
which we call time-symmetric
evolution.
0 0
0
ˆ ˆ( ) ( )
ˆ ˆ ( ) ( )
F B
F B
U U
U U
0
0ˆ ˆ( ) ( ) ( )F BU + U
0(2 ) ( )2ˆ ˆ ˆ ˆ ( ) ( ) ( ) ( )F B F BU + U U + U
0
BU FU
0
77
c.f. double slit:The total amplitude for is proportional to
This is true for all states , so
Time-symmetric evolution over an additional time interval of is given by
0
BU FU
( )t
/18/18
Introduction Paths through time Interference Direction of time Early universe
Repeating this N times yields
0ˆ ˆ( )N ( ) ( )F B
NU + U
00
ˆ( )N
m
N
( )S N,m
▀ is a sum containing different terms
▀ is a sum over a set of paths each
comprising
forwards steps and backwards steps
Let
ˆ( )S N,m )(Nm
0ˆ ( )S N,m
m N m
88
0
BU FU
BU FU BU FU
BU FUBU FU BU FU
BU FU BU FU BU FUBU FU
( )Nt
ˆ(4,1)S
/18/18
Introduction Paths through time Interference Direction of time Early universe
The limit 0 ?
tott tott
N N
2
tot
1 1ˆ ˆ ˆ ˆ( ) ( ) exp[ ( ) ] ( )2 2
1 ˆ ˆexp[ ( ) ] as 2
NN
F B F BN
F B
U U i H H O
i H H t N
effective Hamiltonian=0 for conventional clock device no time in conventional sense▀ Set to be a small physical time interval,
Planck time
445 10 s
99
0
BU FU
BU FU BU FU
BU FUBU FU BU FU
BU FU BU FU BU FUBU FU
( )N t
▀ fix total time and set . Take limit as .
▀ we find
/18/18
Introduction Paths through time Interference Direction of time Early universe
Interference
Multiple paths
ˆ(4,1)S
4 terms
interfere
ˆ(4,0)S ˆ(4,4)S
Example:
1010
0
BU FU
BU FU BU FU
BU FUBU FU BU FU
BU FU BU FU BU FUBU FU
( )N
t
/18/18
Introduction Paths through time Interference Direction of time Early universe
1111
The Zassenhaus (Baker-Campbell-Hausdorff ) formula
gives
Simplifying ˆ( )S N,m
ˆˆ ˆB FU N m U m ( )S N,m
Eigenvalue equation for
commutatorˆ ˆi [ , ]F BH H
degeneracytrace 1 projection op.
ˆ ( ) 1d ( )
eigenvalue
i
ˆ ˆ iA iB e e
2 3ˆ ˆˆ ˆ [ , ] ( )iB iA A B O e e e
2 3
0 0 0 0
exp ( ) (ˆ ˆ )N m v k
v u k j
v u k j O
[ , ]
F BH H
0 0ˆ
0
ˆˆN
n
( ) ( ) ( )F B
NU + U S N,m
/18/18
Introduction Paths through time Interference Direction of time Early universe
1 2
0
2
1
{exp[ ( ) ] 1}
[exp( ) 1]
m
km
k
i N k
ik
( , , )I N m where
ˆ ˆ ˆ ˆ( , ) [( ) ] ( ) ( )B FS N m U N m U m d (( , , ) )I N m
degeneracy
eigenvalue
trace 1 projection op.
1212
Eigenvalues for j th kaon 17 210 sj
Eigenvalues for M kaons
Estimating eigenvalues
0
0( ) ,
a Kdi i
bdt K
ψM Γ ψ ψ
ˆ ˆi [ , ]F BH Hphenomenological model [Lee, PR 138, B1490 (1965)].
17 2SD 10 sM
0
8010M f
57 2SD 10 sf
Let
fraction
total # of particles
/18/18
Introduction Paths through time Interference Direction of time Early universe
Comparison of with ( , , )I N m ( )
( , , )I N n n ( , , )I N n n
1dˆ (0)d
ˆ ˆ ˆ ˆ( , ) [( ) ] ( ) ( )B FS N n n U N n U n d (( ) ), ,I N m
destructive interference
constructive interference
2 24
( )m N m N
1313
( )
( , , )I N m
width
( , , )I N m
8000, 400N m 500, 100N m
/18/18
Introduction Paths through time Interference Direction of time Early universe
1/2 13 10 sN f
total time
0ˆ ˆ( ) ( ) ( )F BN U N U N
Bi-evolution equation of motion
Only two paths survive if
1414
8010M f
fraction
total # of particles
#
kaons
0
BU FU
BU FU
BU FU
FUBU
( )N
t
Destructive interference
/18/18
Introduction Paths through time Interference Direction of time Early universe
0
BU FU
BU FU
BU FU
FUBU
( )N
t
0ˆ ˆ( ) ( ) ( )F BN U N U N
ˆBH
only observe evidence of in this branch
we observe only one of these terms
phenomenological unidirectionality of time
ˆFH
only observe evidence of in this branch
1515
Direction of time
/18/18
Introduction Paths through time Interference Direction of time Early universe
Shortest path through time
1616
BU FU
BU FU BU FU
BU FUBU FU BU FU
BU FU BU FU BU FUBU FU
BU FU
FU
shortest path
same time
/18/18
Introduction Paths through time Interference Direction of time Early universe
1717
Early universeT violation would be relatively rare, so no interference:
0
0
0
ˆ ˆ( ) ( ) ( ) ,
ˆ ˆexp( ) exp( )
ˆco
ˆ
s ( )
ˆcos( )
ˆF BN U U
iH iH
H
N
N
N
H
=F BH H
eigenstate of
with largest eigenvalue (i.e. 1)
= zero eigenvalue of
H
max max maxˆ NNA
Power method
ˆ ( ) 0H N ~ Hamiltonian constraint of the Wheeler-DeWitt eqn.
Hence
BU FU
BU FU BU FU
BU FUBU FU BU FU
BU FU BU FU BU FUBU FU
( )N t
largest eigenvalue
= history
/18/18
Introduction Paths through time Interference Direction of time Early universe
Summary
▀ must use Feynman’s sum over histories to account for both directions
▀ destructive interference leaves only 2 paths▀ physical evidence shows which path we experience▀ quantum algorithm for the shortest path to the
“future”...
1818
the unidirectionality of time
BU FU
BU FU BU FU
BU FUBU FU BU FU
BU FU BU FU BU FUBU FU
BU FU
FU
T invarianceT violation
0
BU FU
BU FU BU FU
BU FUBU FU BU FU
BU FU BU FU BU FUBU FU
( )N t
Universe has no reference for direction of time