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Constraints on Dissipative Processes Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: [email protected] 2. LPTMC, University of Paris VI, France 3. DAMTP, Cambridge University , UK email: [email protected] [email protected] DGMTP XXIII, Nankai Institute, Tianjin: 25 August 2005
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Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: [email protected].

Dec 14, 2015

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Page 1: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Constraints on Dissipative ProcessesConstraints on Dissipative Processes Constraints on Dissipative ProcessesConstraints on Dissipative Processes Allan Solomon1,2 and Sonia Schirmer3

1 Dept. of Physics & Astronomy. Open University, UK email: [email protected]

2. LPTMC, University of Paris VI, France

3. DAMTP, Cambridge University , UK email: [email protected] [email protected]

DGMTP XXIII, Nankai Institute, Tianjin: 25 August 2005

Page 2: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

AbstractAbstractAbstractAbstractA state in quantum mechanics is defined as a positive A state in quantum mechanics is defined as a positive operator of norm 1. For operator of norm 1. For finitefinite systems, this may be systems, this may be thought of as a positive matrix of trace 1. This thought of as a positive matrix of trace 1. This constraint of positivity imposes severe restrictions on constraint of positivity imposes severe restrictions on the allowed evolution of such a state. From the the allowed evolution of such a state. From the mathematical viewpoint, we describe the two forms of mathematical viewpoint, we describe the two forms of standard dynamical equations - global (Kraus) and local standard dynamical equations - global (Kraus) and local (Lindblad) - and show how each of these gives rise to a (Lindblad) - and show how each of these gives rise to a semi-group description of the evolution. We then look at semi-group description of the evolution. We then look at specific examples from atomic systems, involving 3-level specific examples from atomic systems, involving 3-level systems for simplicity, and show how these systems for simplicity, and show how these mathematical constraints give rise to non-intuitive mathematical constraints give rise to non-intuitive physical phenomena, reminiscent of Bohm-Aharonov physical phenomena, reminiscent of Bohm-Aharonov effects.effects.

Page 3: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

ContentsContentsContentsContentsPure StatesPure StatesMixed StatesMixed StatesN-level SystemsN-level SystemsHamiltonian DynamicsHamiltonian DynamicsDissipative DynamicsDissipative DynamicsSemi-GroupsSemi-GroupsDissipation and Semi-GroupsDissipation and Semi-GroupsDissipation - General TheoryDissipation - General TheoryTwo-level ExampleTwo-level ExampleRelaxation ParametersRelaxation ParametersBohm-Aharonov EffectsBohm-Aharonov EffectsThree-levels systemsThree-levels systems

Page 4: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

StatesStatesStatesStatesFinite SystemsFinite Systems(1) Pure States(1) Pure States

Ignore overall phase; depends on 22 real parameters Represent by point on SphereSphere

N-levelN-level

E.g. 2-levelE.g. 2-level qubit1|||| 22

Ci

N

i

N

1||1

2

1

Page 5: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

StatesStatesStatesStates(2) Mixed States(2) Mixed States

PurePure state can be represented by operator

projecting onto

For example (N=2) as matrix

is Hermitian Trace = 1 eigenvalues 0

This is taken as definition of a STATESTATE (mixedmixed or purepure)

(For purepure state only one non-zero eigenvalue, =1)

is the Density Matrixis the Density Matrix

This is taken as definition of a STATESTATE (mixedmixed or purepure)

(For purepure state only one non-zero eigenvalue, =1)

is the Density Matrixis the Density Matrix

|

**

***]*[

Page 6: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

N - level systemsN - level systemsN - level systemsN - level systems

Density MatrixDensity Matrix is N x N matrix, elements ij

Notation: Notation: [i,j] = index from 1 to N2; [i,j]=(i-1)N+j

Define Complex NDefine Complex N22-vector V-vector V(()) V[i,j]

() = ij

Ex: N=2:

22

21

12

11

2221

1211

V

Page 7: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Dissipative Dynamics (Non-Hamiltonian)

Ex 1: How to cool a system, & change a mixed state to a pure state

Ex 2: How to change pure state to a mixed state

is a Population Relaxation Coefficient

00

01

4/30

0)3/41(4/1

4/30

04/1

t

tt

e

et

is a Dephasing Coefficient

4/30

04/1

4/34/3

)4/34/1

4/34/3

4/34/1

t

tt

e

et

Page 8: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Ex 3: Can we do both together ?

1121

2212

21

122212

1121

ρ)tγ1(ρtγρt

ρtρ)tγ1(ρtγ

)(eee

eeet

Is this a STATE? (i)Hermiticity? (ii) Trace = 1?

(iii) Positivity?

..)ρρρρ( Det 2112t2

2211t)γγ( 1221 ee

Constraint relations between and ’s.

)21γ12γ(2/1

Page 9: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Hamiltonian Dynamics Hamiltonian Dynamics

(Non-dissipative)(Non-dissipative)

Hamiltonian Dynamics Hamiltonian Dynamics

(Non-dissipative)(Non-dissipative) [[Schroedinger Equation]Schroedinger Equation]

Global Form: (t) = U(t) (0) U(t)†

Local Form: i t (t) =[H, (t) ]

We may now add dissipative terms to this equation.

Page 10: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Dissipation Dynamics - GeneralDissipation Dynamics - GeneralDissipation Dynamics - GeneralDissipation Dynamics - General

Global Form* KRAUS Formalism

†ii ww

iii Iww †

Maintains Positivity and Trace Properties

†U U Analogue of Global Evolution

*K.Kraus, Ann.Phys.64, 311(1971)

Page 11: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Dissipation Dynamics - Dissipation Dynamics - GeneralGeneral

Dissipation Dynamics - Dissipation Dynamics - GeneralGeneral

Local Form* Lindblad Equations

Maintains Positivity and Trace Properties

]},[],{[21

],[)/( ††iiii VVVVHi

Analogue of Schroedinger Equation

*V.Gorini, A.Kossakowski and ECG Sudarshan, Rep.Math.Phys.13, 149 (1976)G. Lindblad, Comm.Math.Phys.48,119 (1976)

Page 12: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Dissipation and Semigroups

I. Sets of Bounded Operators

Dissipation and Semigroups

I. Sets of Bounded Operators

B(H) is the set of boundedbounded operators on H.

Def: Norm of an operator AA:

||AA|| = sup {|| AA || / || ||, H}

Def: Bounded operator The operator AA in H is a bounded operator if ||AA|| < K for some real K.

Examples: X ( x ) = x( x) is NOT a bounded operator on H; but exp (iX) IS a bounded operator.

Page 13: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Dissipation and Semigroups

II. Bounded Sets of operators:

Dissipation and Semigroups

II. Bounded Sets of operators:

Consider S-(A) = {exp(-t) A; A bounded, t 0 }.

Clearly S-(A) B(H).

There exists K such that ||X|| < K for all X S-(A)

Clearly S+(A) = {exp(t) A; A bounded, t 0 } does notnot have this (uniformly bounded) property.

S-(A) is a Bounded SetBounded Set of operators

Page 14: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Dissipation and Semigroups

III. Semigroups

Dissipation and Semigroups

III. Semigroups

Example: The set { exp(-t): t>0 } forms a semigroup.

Example: The set { exp(-t): 0 } forms a semigroup with identity.

Def: A semigroup G is a set of elements which is closed under composition.

Note: The composition is associative, as for groups.

G may or may not have an identity element I, and some of its elements may or may not have inverses.

Page 15: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Dissipation and SemigroupsDissipation and Semigroups

Important Example: If L is a (finite) matrix with negative eigenvalues, and T(t) = exp(Lt).

Then {T(t), t 0 } is a one-parameter semigroup, with Identity, and is a Bounded Set of Operators.

One-parameter semigroups

T(t1)*T(t2)=T(t1 + t1)

with identity, T(0)=I.

Page 16: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Dissipation Dynamics - Semi-GroupDissipation Dynamics - Semi-GroupDissipation Dynamics - Semi-GroupDissipation Dynamics - Semi-Group

Global (Kraus) Form: SEMI - GROUP G

†ii ww

iii Iww †

� Semi-Group G: g={wi} g ’={w ’i }

then g g ’ G

� Identity {I}

� Some elements have inverses:

{U} where UU+=I

Page 17: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Dissipation Dynamics - Semi-GroupDissipation Dynamics - Semi-GroupDissipation Dynamics - Semi-GroupDissipation Dynamics - Semi-Group

Local Form ]},[],{[2

1],[)/( ††

iiii VVVVHi

Superoperator Form VLLV DH )(

Pure Hamiltonian (Formal)

)0()exp( VtLVVLV HH

Pure Dissipation (Formal)

)0()exp( VtLVVLV DD

LH generates Group

LD generates Semi-group

Page 18: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Example: Two-level System (a)

Dissipation Part:V-matrices

)(~

21122

1

:= H w

1 0

0 -1fx

0 1

1 0fy

0 I

I 0

Hamiltonian Part: (fx and fy controls)

with

†† ,,],[ jjjj VVVVHi

1

21

0 0

0V

122

0

0 0V

3

2 0

0 0V

Page 19: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

:= LD

,2 1 0 0

,1 2

0 0 0

0 0 0

,2 1 0 0

,1 2

Example: Two-level System (b)

(1) In Liouville form (4-vector V)

:= V [ ], , ,,1 1

,1 2

,2 1

,2 2

VLLV DH )(.

Where LH has pure imaginary eigenvalues and LD real negative eigenvalues.

Page 20: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

:= LD

,2 1 0 0

,1 2

0 0 0

0 0 0

,2 1 0 0

,1 2

0 0 0

0 0 0

0 0 ,2 1

,1 2

,2 1

,1 2

0 0 0 0

,2 1

,1 2

0 0 0

0 0 0

0 0 2 0

0 0 0 0

2-Level Dissipation Matrix

2-Level Dissipation Matrix (Bloch Form)

2-Level Dissipation Matrix (Bloch Form, Spin System)

4X4 Matrix Form

Page 21: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Solution to Relaxation/Dephasing Solution to Relaxation/Dephasing ProblemProblem

Solution to Relaxation/Dephasing Solution to Relaxation/Dephasing ProblemProblem

Choose Eij a basis of Elementary Matrices, i,,j = 1…N

ijjiji EaV ],[],[

2

],[ || jiij a

)|||(|~

)|||(|

2],[

2],[2

1

2],[

2

,,1],[2

1

jjiiij

jk

N

jikikij

aa

aa

V-matrices

s

s

Page 22: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Solution to Relaxation/Dephasing Problem (contd)Solution to Relaxation/Dephasing Problem (contd)Solution to Relaxation/Dephasing Problem (contd)Solution to Relaxation/Dephasing Problem (contd)

( N2 x’s may be chosen real,positive)

ijjiijjiji ExEaV ],[],[],[

)( ji[i,j]ij x

)(~

)(~

12

1

],[],[2

1

kj

N

kkiijij

jjiiij xx

Determine V-matrices in terms of physical dissipation parameters

N(N-1) s

N(N-1)/2 s

Page 23: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Solution to Relaxation/Dephasing Problem (contd)Solution to Relaxation/Dephasing Problem (contd)Solution to Relaxation/Dephasing Problem (contd)Solution to Relaxation/Dephasing Problem (contd)

ijjiijjiji ExEaV ],[],[],[

)(],[ jiijjix

)(~

],[],[2

1

jjiiij xx

N(N-1) s

N(N-1)/2 s

Problem: Determine N2 x’s in terms of the N(N-1) relaxation coefficients and theN(N-1)/2 pure dephasing parameters Γ

~

There are (N2-3N)/2 conditions on the relaxation parameters; they are not independent!

Page 24: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Bohm-Aharanov–type EffectsBohm-Aharanov–type Effects

“ “ Changes in a system A, which is Changes in a system A, which is apparently physically isolated from a apparently physically isolated from a system B, nevertheless produce phase system B, nevertheless produce phase changes in the system B.”changes in the system B.”

We shall show how changes in A – a subset We shall show how changes in A – a subset of energy levels of an N-level atomic of energy levels of an N-level atomic system, produce phase changes in energy system, produce phase changes in energy levels belonging to a different subset B , levels belonging to a different subset B , and quantify these effects.and quantify these effects.

Page 25: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Dissipative Dissipative TermsTerms

Orthonormal basis:Orthonormal basis:

Population Relaxation Equations (

Phase Relaxation Equations

knknHi ],[

kknk

nknnnk

knnnnn Hi

],[

},...2,1:{| Nnn

Page 26: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Quantum Liouville Equation Quantum Liouville Equation (Phenomological)(Phenomological)

Incorporating these terms into a Incorporating these terms into a dissipation superoperatordissipation superoperator L LDD

Writing t as a N2 column vector V

Non-zero elements of LD areare (m,n)=m+(n-1)N

VLLV DH )(

)(],[ DLHi

Page 27: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Liouville Operator for a Three-Level Liouville Operator for a Three-Level SystemSystem

Page 28: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Three-state AtomsThree-state Atoms

1

3

2

1

12

13

3

2

12

32

V-system

Ladder system

3

221

23

-system

1

Page 29: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Decay in a Three-Level Decay in a Three-Level SystemSystem

1121

2212

21

122212

1121

ρ)tγ1(ρtγρt

ρtρ)tγ1(ρtγ

)(eee

eeet

Two-level case

In above choose 21=0 and =1/212 which

satisfies 2-level constraint)21γ12γ(2/1

333231

2322212/1312

2/22)1(11

)(

tete

tete

t

And add another level all new =0.

Page 30: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

““Eigenvalues” of a Three-level Eigenvalues” of a Three-level SystemSystem

Page 31: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Phase Decoherence in Three-Level Phase Decoherence in Three-Level SystemSystem

333231

2322212/1312

2/11

)(

te

te

t

Page 32: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

““Eigenvalues” of a Three-level Eigenvalues” of a Three-level SystemSystem

Pure DephasingPure Dephasing

Time (units of 1/)

Page 33: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Three Level Three Level SystemsSystems

Page 34: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Four-Level Four-Level SystemsSystems

Page 35: Constraints on Dissipative Processes Allan Solomon 1,2 and Sonia Schirmer 3 1 Dept. of Physics & Astronomy. Open University, UK email: a.i.solomon@open.ac.uk.

Constraints on Four-Level SystemsConstraints on Four-Level Systems