Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli...

86
Calculation of Generalized Pauli Constraints Murat Altunbulak Department of Mathematics Dokuz Eylul University April, 2016 Murat Altunbulak Oxford 2016

Transcript of Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli...

Page 1: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Calculation of Generalized Pauli Constraints

Murat Altunbulak

Department of MathematicsDokuz Eylul University

April, 2016

Murat Altunbulak Oxford 2016

Page 2: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Notations

Murat Altunbulak Oxford 2016

Page 3: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Notations

Quantum States

Quantum system A is described by a complex Hilbert space HA,

called state space.

Pure state = unit vector |ψ〉 ∈ HA or projector operator |ψ〉〈ψ|Mixed state = classical mixture of pure states

ρ =∑i

pi |ψi 〉〈ψi | ; pi ≥ 0 ;∑i

pi = 1

ρ is a non-negative (ρ ≥ 0) Hermitian operator with Trρ = 1, calledDensity matrix.

Murat Altunbulak Oxford 2016

Page 4: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Notations

Quantum States

Quantum system A is described by a complex Hilbert space HA,called state space.

Pure state = unit vector |ψ〉 ∈ HA or projector operator |ψ〉〈ψ|Mixed state = classical mixture of pure states

ρ =∑i

pi |ψi 〉〈ψi | ; pi ≥ 0 ;∑i

pi = 1

ρ is a non-negative (ρ ≥ 0) Hermitian operator with Trρ = 1, calledDensity matrix.

Murat Altunbulak Oxford 2016

Page 5: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Notations

Quantum States

Quantum system A is described by a complex Hilbert space HA,called state space.

Pure state = unit vector |ψ〉 ∈ HA or projector operator |ψ〉〈ψ|

Mixed state = classical mixture of pure states

ρ =∑i

pi |ψi 〉〈ψi | ; pi ≥ 0 ;∑i

pi = 1

ρ is a non-negative (ρ ≥ 0) Hermitian operator with Trρ = 1, calledDensity matrix.

Murat Altunbulak Oxford 2016

Page 6: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Notations

Quantum States

Quantum system A is described by a complex Hilbert space HA,called state space.

Pure state = unit vector |ψ〉 ∈ HA or projector operator |ψ〉〈ψ|Mixed state = classical mixture of pure states

ρ =∑i

pi |ψi 〉〈ψi | ; pi ≥ 0 ;∑i

pi = 1

ρ is a non-negative (ρ ≥ 0) Hermitian operator with Trρ = 1, calledDensity matrix.

Murat Altunbulak Oxford 2016

Page 7: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Notations

Quantum States

Quantum system A is described by a complex Hilbert space HA,called state space.

Pure state = unit vector |ψ〉 ∈ HA or projector operator |ψ〉〈ψ|Mixed state = classical mixture of pure states

ρ =∑i

pi |ψi 〉〈ψi | ; pi ≥ 0 ;∑i

pi = 1

ρ is a non-negative (ρ ≥ 0) Hermitian operator with Trρ = 1, calledDensity matrix.

Murat Altunbulak Oxford 2016

Page 8: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Notations

Superposition Principle

implies that the state space of composite system AB splits into tensorproduct of its components A and B

HAB = HA ⊗HB

Density Matrix of Composite Systems

Density matrix of composite system can be written as linear combination

ρAB =∑α

aαLαA ⊗ LαB

where LαA, LαB are linear operators on HA, HB , respectively.

Murat Altunbulak Oxford 2016

Page 9: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Notations

Superposition Principle

implies that the state space of composite system AB splits into tensorproduct of its components A and B

HAB = HA ⊗HB

Density Matrix of Composite Systems

Density matrix of composite system can be written as linear combination

ρAB =∑α

aαLαA ⊗ LαB

where LαA, LαB are linear operators on HA, HB , respectively.

Murat Altunbulak Oxford 2016

Page 10: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Notations

Reduced state

Its reduced matrices are defined by partial traces

ρA =∑α

aαTr(LαB)LαA := TrB(ρAB)

ρB =∑α

aαTr(LαA)LαB := TrA(ρAB)

they are called one-particle reduced density matrices.

Murat Altunbulak Oxford 2016

Page 11: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Notations

Reduced state

Its reduced matrices are defined by partial traces

ρA =∑α

aαTr(LαB)LαA := TrB(ρAB)

ρB =∑α

aαTr(LαA)LαB := TrA(ρAB)

they are called one-particle reduced density matrices.

Murat Altunbulak Oxford 2016

Page 12: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Notations

Reduced state

Its reduced matrices are defined by partial traces

ρA =∑α

aαTr(LαB)LαA := TrB(ρAB)

ρB =∑α

aαTr(LαA)LαB := TrA(ρAB)

they are called one-particle reduced density matrices.

Murat Altunbulak Oxford 2016

Page 13: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Notations

Reduced state

Its reduced matrices are defined by partial traces

ρA =∑α

aαTr(LαB)LαA := TrB(ρAB)

ρB =∑α

aαTr(LαA)LαB := TrA(ρAB)

they are called one-particle reduced density matrices.

Murat Altunbulak Oxford 2016

Page 14: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Pauli Exclusion Principle

Murat Altunbulak Oxford 2016

Page 15: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Pauli exclusion principle

Initial form (1925)

state that no two identical fermions may occupy the same quantumstate.

In the language of density matrices it can be stated as followsLet ρN : H⊗N , H⊗N = state space of N electrons.Define ρ = ρN1 + ρN2 + . . .+ ρNN sum of all reduced states ρNi : H. ρis called electron density matrix.In terms of electron density matrix ρ, Pauli principle amounts to〈ψ|ρ|ψ〉 ≤ 1⇐⇒ Specρ ≤ 1

Modern Version (1926)

Heisenberg-Dirac replaced the Pauli exclusion principle byskew-symmetry of multi-electron wave function

which implies that the state space of N electrons shrinks to∧NH ⊂ H⊗N .

This implies the original Pauli principle, because ψ ∧ ψ = 0.

Murat Altunbulak Oxford 2016

Page 16: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Pauli exclusion principle

Initial form (1925)

state that no two identical fermions may occupy the same quantumstate.

In the language of density matrices it can be stated as follows

Let ρN : H⊗N , H⊗N = state space of N electrons.Define ρ = ρN1 + ρN2 + . . .+ ρNN sum of all reduced states ρNi : H. ρis called electron density matrix.In terms of electron density matrix ρ, Pauli principle amounts to〈ψ|ρ|ψ〉 ≤ 1⇐⇒ Specρ ≤ 1

Modern Version (1926)

Heisenberg-Dirac replaced the Pauli exclusion principle byskew-symmetry of multi-electron wave function

which implies that the state space of N electrons shrinks to∧NH ⊂ H⊗N .

This implies the original Pauli principle, because ψ ∧ ψ = 0.

Murat Altunbulak Oxford 2016

Page 17: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Pauli exclusion principle

Initial form (1925)

state that no two identical fermions may occupy the same quantumstate.

In the language of density matrices it can be stated as followsLet ρN : H⊗N , H⊗N = state space of N electrons.

Define ρ = ρN1 + ρN2 + . . .+ ρNN sum of all reduced states ρNi : H. ρis called electron density matrix.In terms of electron density matrix ρ, Pauli principle amounts to〈ψ|ρ|ψ〉 ≤ 1⇐⇒ Specρ ≤ 1

Modern Version (1926)

Heisenberg-Dirac replaced the Pauli exclusion principle byskew-symmetry of multi-electron wave function

which implies that the state space of N electrons shrinks to∧NH ⊂ H⊗N .

This implies the original Pauli principle, because ψ ∧ ψ = 0.

Murat Altunbulak Oxford 2016

Page 18: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Pauli exclusion principle

Initial form (1925)

state that no two identical fermions may occupy the same quantumstate.

In the language of density matrices it can be stated as followsLet ρN : H⊗N , H⊗N = state space of N electrons.Define ρ = ρN1 + ρN2 + . . .+ ρNN sum of all reduced states ρNi : H. ρis called electron density matrix.

In terms of electron density matrix ρ, Pauli principle amounts to〈ψ|ρ|ψ〉 ≤ 1⇐⇒ Specρ ≤ 1

Modern Version (1926)

Heisenberg-Dirac replaced the Pauli exclusion principle byskew-symmetry of multi-electron wave function

which implies that the state space of N electrons shrinks to∧NH ⊂ H⊗N .

This implies the original Pauli principle, because ψ ∧ ψ = 0.

Murat Altunbulak Oxford 2016

Page 19: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Pauli exclusion principle

Initial form (1925)

state that no two identical fermions may occupy the same quantumstate.

In the language of density matrices it can be stated as followsLet ρN : H⊗N , H⊗N = state space of N electrons.Define ρ = ρN1 + ρN2 + . . .+ ρNN sum of all reduced states ρNi : H. ρis called electron density matrix.In terms of electron density matrix ρ, Pauli principle amounts to〈ψ|ρ|ψ〉 ≤ 1⇐⇒ Specρ ≤ 1

Modern Version (1926)

Heisenberg-Dirac replaced the Pauli exclusion principle byskew-symmetry of multi-electron wave function

which implies that the state space of N electrons shrinks to∧NH ⊂ H⊗N .

This implies the original Pauli principle, because ψ ∧ ψ = 0.

Murat Altunbulak Oxford 2016

Page 20: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Pauli exclusion principle

Initial form (1925)

state that no two identical fermions may occupy the same quantumstate.

In the language of density matrices it can be stated as followsLet ρN : H⊗N , H⊗N = state space of N electrons.Define ρ = ρN1 + ρN2 + . . .+ ρNN sum of all reduced states ρNi : H. ρis called electron density matrix.In terms of electron density matrix ρ, Pauli principle amounts to〈ψ|ρ|ψ〉 ≤ 1⇐⇒ Specρ ≤ 1

Modern Version (1926)

Heisenberg-Dirac replaced the Pauli exclusion principle byskew-symmetry of multi-electron wave function

which implies that the state space of N electrons shrinks to∧NH ⊂ H⊗N .

This implies the original Pauli principle, because ψ ∧ ψ = 0.

Murat Altunbulak Oxford 2016

Page 21: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Pauli exclusion principle

Initial form (1925)

state that no two identical fermions may occupy the same quantumstate.

In the language of density matrices it can be stated as followsLet ρN : H⊗N , H⊗N = state space of N electrons.Define ρ = ρN1 + ρN2 + . . .+ ρNN sum of all reduced states ρNi : H. ρis called electron density matrix.In terms of electron density matrix ρ, Pauli principle amounts to〈ψ|ρ|ψ〉 ≤ 1⇐⇒ Specρ ≤ 1

Modern Version (1926)

Heisenberg-Dirac replaced the Pauli exclusion principle byskew-symmetry of multi-electron wave function

which implies that the state space of N electrons shrinks to∧NH ⊂ H⊗N .

This implies the original Pauli principle, because ψ ∧ ψ = 0.

Murat Altunbulak Oxford 2016

Page 22: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Pauli exclusion principle

Initial form (1925)

state that no two identical fermions may occupy the same quantumstate.

In the language of density matrices it can be stated as followsLet ρN : H⊗N , H⊗N = state space of N electrons.Define ρ = ρN1 + ρN2 + . . .+ ρNN sum of all reduced states ρNi : H. ρis called electron density matrix.In terms of electron density matrix ρ, Pauli principle amounts to〈ψ|ρ|ψ〉 ≤ 1⇐⇒ Specρ ≤ 1

Modern Version (1926)

Heisenberg-Dirac replaced the Pauli exclusion principle byskew-symmetry of multi-electron wave function

which implies that the state space of N electrons shrinks to∧NH ⊂ H⊗N .

This implies the original Pauli principle, because ψ ∧ ψ = 0.

Murat Altunbulak Oxford 2016

Page 23: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Statement of The Problem

Murat Altunbulak Oxford 2016

Page 24: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Statement of the problem

In the latter case, electron density matrix becomes ρ = NρN1 ,Trρ = N.

Problem

What are the constraints on electron density matrix ρ beyond the originalPauli principle Specρ ≤ 1.

Pure N-representability

The above problem became known as (pure) N-representability problemafter A.J. Coleman (1963).

Mixed N-representability

More generally we have mixed N-representability problem:“What are the constraints on the spectra of a mixed state and itsreduced matrix?”

Murat Altunbulak Oxford 2016

Page 25: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Statement of the problem

In the latter case, electron density matrix becomes ρ = NρN1 ,Trρ = N.

Problem

What are the constraints on electron density matrix ρ beyond the originalPauli principle Specρ ≤ 1.

Pure N-representability

The above problem became known as (pure) N-representability problemafter A.J. Coleman (1963).

Mixed N-representability

More generally we have mixed N-representability problem:“What are the constraints on the spectra of a mixed state and itsreduced matrix?”

Murat Altunbulak Oxford 2016

Page 26: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Statement of the problem

In the latter case, electron density matrix becomes ρ = NρN1 ,Trρ = N.

Problem

What are the constraints on electron density matrix ρ beyond the originalPauli principle Specρ ≤ 1.

Pure N-representability

The above problem became known as (pure) N-representability problemafter A.J. Coleman (1963).

Mixed N-representability

More generally we have mixed N-representability problem:“What are the constraints on the spectra of a mixed state and itsreduced matrix?”

Murat Altunbulak Oxford 2016

Page 27: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Statement of the problem

In the latter case, electron density matrix becomes ρ = NρN1 ,Trρ = N.

Problem

What are the constraints on electron density matrix ρ beyond the originalPauli principle Specρ ≤ 1.

Pure N-representability

The above problem became known as (pure) N-representability problemafter A.J. Coleman (1963).

Mixed N-representability

More generally we have mixed N-representability problem:“What are the constraints on the spectra of a mixed state and itsreduced matrix?”

Murat Altunbulak Oxford 2016

Page 28: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

What was known before 2008?

Murat Altunbulak Oxford 2016

Page 29: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

What was known before 2008?

Initial constraints

Ordering inequalities λ1 ≥ λ2 ≥ . . . ≥ λr ≥ 0

Normalization condition Trρ =∑

i λi = N

Two-particle (∧2Hr ) and Two-hole (∧r−2Hr ) systems

Constraints on electron density matrix ρ is given by even degeneracyof its eigenvalues, i.e. λ1 = λ2 ≥ λ3 = λ4 ≥ . . .Similar results hold for two-hole system.

Murat Altunbulak Oxford 2016

Page 30: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

What was known before 2008?

Initial constraints

Ordering inequalities λ1 ≥ λ2 ≥ . . . ≥ λr ≥ 0

Normalization condition Trρ =∑

i λi = N

Two-particle (∧2Hr ) and Two-hole (∧r−2Hr ) systems

Constraints on electron density matrix ρ is given by even degeneracyof its eigenvalues, i.e. λ1 = λ2 ≥ λ3 = λ4 ≥ . . .Similar results hold for two-hole system.

Murat Altunbulak Oxford 2016

Page 31: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

What was known before 2008?

Initial constraints

Ordering inequalities λ1 ≥ λ2 ≥ . . . ≥ λr ≥ 0

Normalization condition Trρ =∑

i λi = N

Two-particle (∧2Hr ) and Two-hole (∧r−2Hr ) systems

Constraints on electron density matrix ρ is given by even degeneracyof its eigenvalues, i.e. λ1 = λ2 ≥ λ3 = λ4 ≥ . . .

Similar results hold for two-hole system.

Murat Altunbulak Oxford 2016

Page 32: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

What was known before 2008?

Initial constraints

Ordering inequalities λ1 ≥ λ2 ≥ . . . ≥ λr ≥ 0

Normalization condition Trρ =∑

i λi = N

Two-particle (∧2Hr ) and Two-hole (∧r−2Hr ) systems

Constraints on electron density matrix ρ is given by even degeneracyof its eigenvalues, i.e. λ1 = λ2 ≥ λ3 = λ4 ≥ . . .Similar results hold for two-hole system.

Murat Altunbulak Oxford 2016

Page 33: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

What was known before 2008?

Borland-Dennis system

For the system ∧3H6 of three electrons of rank 6, theN-representability conditions are given by the following (in)equalities:

λ1 + λ6 = λ2 + λ5 = λ3 + λ4 = 1, λ4 ≤ λ5 + λ6,

Sufficiency proved by Borland-Dennis (1972)

Necessity proved by Ruskai (2007)

Murat Altunbulak Oxford 2016

Page 34: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

What was known before 2008?

Borland-Dennis system

For the system ∧3H6 of three electrons of rank 6, theN-representability conditions are given by the following (in)equalities:

λ1 + λ6 = λ2 + λ5 = λ3 + λ4 = 1, λ4 ≤ λ5 + λ6,

Sufficiency proved by Borland-Dennis (1972)

Necessity proved by Ruskai (2007)

Murat Altunbulak Oxford 2016

Page 35: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

What was known before 2008?

Borland-Dennis system

For the system ∧3H6 of three electrons of rank 6, theN-representability conditions are given by the following (in)equalities:

λ1 + λ6 = λ2 + λ5 = λ3 + λ4 = 1, λ4 ≤ λ5 + λ6,

Sufficiency proved by Borland-Dennis (1972)

Necessity proved by Ruskai (2007)

Murat Altunbulak Oxford 2016

Page 36: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Formal Solution of Mixed N-representability

Murat Altunbulak Oxford 2016

Page 37: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Formal Solution

Solution of Mixed N-representability

Main Theorem. Let ρN : ∧NHr (TrρN = 1) be mixed state and ρ : Hr

(Trρ = N) be its particle density matrix.

Then all constraints onSpecρ = λ : λ1 ≥ λ2 ≥ . . . ≥ λr and SpecρN = µ : µ1 ≥ µ2 ≥ . . . ≥ µR

(R =(rN

)= dim∧NHr ) are given by the following linear inequalities

(Generalized Pauli Constraints)∑i

aiλv(i) ≤∑k

(∧Na)kµw(k) (a, v ,w)

Here, ∧Na consists of all sums ai1 + ai2 + · · ·+ aiN ,1 ≤ i1 < i2 < · · · < iN ≤ r arranged in decreasing order, v ∈ Sr andw ∈ SR subject to topological condition cwv (a) 6= 0 explained soon.

Murat Altunbulak Oxford 2016

Page 38: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Formal Solution

Solution of Mixed N-representability

Main Theorem. Let ρN : ∧NHr (TrρN = 1) be mixed state and ρ : Hr

(Trρ = N) be its particle density matrix. Then all constraints onSpecρ = λ : λ1 ≥ λ2 ≥ . . . ≥ λr and SpecρN = µ : µ1 ≥ µ2 ≥ . . . ≥ µR

(R =(rN

)= dim∧NHr ) are given by the following linear inequalities

(Generalized Pauli Constraints)

∑i

aiλv(i) ≤∑k

(∧Na)kµw(k) (a, v ,w)

Here, ∧Na consists of all sums ai1 + ai2 + · · ·+ aiN ,1 ≤ i1 < i2 < · · · < iN ≤ r arranged in decreasing order, v ∈ Sr andw ∈ SR subject to topological condition cwv (a) 6= 0 explained soon.

Murat Altunbulak Oxford 2016

Page 39: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Formal Solution

Solution of Mixed N-representability

Main Theorem. Let ρN : ∧NHr (TrρN = 1) be mixed state and ρ : Hr

(Trρ = N) be its particle density matrix. Then all constraints onSpecρ = λ : λ1 ≥ λ2 ≥ . . . ≥ λr and SpecρN = µ : µ1 ≥ µ2 ≥ . . . ≥ µR

(R =(rN

)= dim∧NHr ) are given by the following linear inequalities

(Generalized Pauli Constraints)∑i

aiλv(i) ≤∑k

(∧Na)kµw(k) (a, v ,w)

Here, ∧Na consists of all sums ai1 + ai2 + · · ·+ aiN ,1 ≤ i1 < i2 < · · · < iN ≤ r arranged in decreasing order, v ∈ Sr andw ∈ SR subject to topological condition cwv (a) 6= 0 explained soon.

Murat Altunbulak Oxford 2016

Page 40: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Formal Solution

Solution of Mixed N-representability

Main Theorem. Let ρN : ∧NHr (TrρN = 1) be mixed state and ρ : Hr

(Trρ = N) be its particle density matrix. Then all constraints onSpecρ = λ : λ1 ≥ λ2 ≥ . . . ≥ λr and SpecρN = µ : µ1 ≥ µ2 ≥ . . . ≥ µR

(R =(rN

)= dim∧NHr ) are given by the following linear inequalities

(Generalized Pauli Constraints)∑i

aiλv(i) ≤∑k

(∧Na)kµw(k) (a, v ,w)

Here, ∧Na consists of all sums ai1 + ai2 + · · ·+ aiN ,1 ≤ i1 < i2 < · · · < iN ≤ r arranged in decreasing order, v ∈ Sr andw ∈ SR subject to topological condition cwv (a) 6= 0 explained soon.

Murat Altunbulak Oxford 2016

Page 41: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Remark

Solution of Pure N-representability

Solution of pure N-representability problem can be deduced from theabove theorem by specialization µi = 0 for i 6= 1, because pure statescorresponds projector operators |ψ〉〈ψ|.

In this case all costraints together with ordering ineqaulities andnormalization condition describe a convex polytope, called MomentPolytope.

Murat Altunbulak Oxford 2016

Page 42: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Remark

Solution of Pure N-representability

Solution of pure N-representability problem can be deduced from theabove theorem by specialization µi = 0 for i 6= 1, because pure statescorresponds projector operators |ψ〉〈ψ|.In this case all costraints together with ordering ineqaulities andnormalization condition describe a convex polytope, called MomentPolytope.

Murat Altunbulak Oxford 2016

Page 43: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Nature of Topological Condition cvw(a) 6= 0

Murat Altunbulak Oxford 2016

Page 44: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Nature of Topological Condition cvw(a) 6= 0

Consider flag variety

Fa(Hr ) = {X : Hr → Hr | a = Spec(X )}

and morphism

ϕa : Fa(Hr ) → F∧Na(∧NHr )

X 7→ X (N)

Here, X (N) : ψ1 ∧ ψ2 ∧ . . . ∧ ψN 7→∑

i ψ1 ∧ ψ2 ∧ . . . ∧ Xψi ∧ . . . ∧ ψN .

Murat Altunbulak Oxford 2016

Page 45: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Nature of Topological Condition cvw(a) 6= 0

Consider flag variety

Fa(Hr ) = {X : Hr → Hr | a = Spec(X )}

and morphism

ϕa : Fa(Hr ) → F∧Na(∧NHr )

X 7→ X (N)

Here, X (N) : ψ1 ∧ ψ2 ∧ . . . ∧ ψN 7→∑

i ψ1 ∧ ψ2 ∧ . . . ∧ Xψi ∧ . . . ∧ ψN .

Murat Altunbulak Oxford 2016

Page 46: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Nature of Topological Condition cvw(a) 6= 0

Consider flag variety

Fa(Hr ) = {X : Hr → Hr | a = Spec(X )}

and morphism

ϕa : Fa(Hr ) → F∧Na(∧NHr )

X 7→ X (N)

Here, X (N) : ψ1 ∧ ψ2 ∧ . . . ∧ ψN 7→∑

i ψ1 ∧ ψ2 ∧ . . . ∧ Xψi ∧ . . . ∧ ψN .

Murat Altunbulak Oxford 2016

Page 47: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Nature of Topological Condition cvw(a) 6= 0

The coefficients cvw (a) are defined via induced morphism of cohomology

ϕ∗a : H∗(F∧Na(∧NHr )) → H∗(Fa(Hr )),

σw 7→∑v

cvw (a)σv

written in the basis of Schubert cocycles σw .

Murat Altunbulak Oxford 2016

Page 48: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Nature of Topological Condition cvw(a) 6= 0

The coefficients cvw (a) are defined via induced morphism of cohomology

ϕ∗a : H∗(F∧Na(∧NHr )) → H∗(Fa(Hr )),

σw 7→∑v

cvw (a)σv

written in the basis of Schubert cocycles σw .

Murat Altunbulak Oxford 2016

Page 49: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Nature of Topological Condition cvw(a) 6= 0

The coefficients cvw (a) are defined via induced morphism of cohomology

ϕ∗a : H∗(F∧Na(∧NHr )) → H∗(Fa(Hr )),

σw 7→∑v

cvw (a)σv

written in the basis of Schubert cocycles σw .

Murat Altunbulak Oxford 2016

Page 50: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Connection with Representation Theory

Murat Altunbulak Oxford 2016

Page 51: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Connection with Representation Theory

Plethysm

Consider the m-th symmetric power of ∧NHr , called Plethysm

It splits into irreducible components Hλ, parameterized by Young

diagrams λ = of size N.m, with multiplicity mλ

Sm(∧NHr ) =∑λ

mλHλ.

Problem

“Which irreducible representations Hλ of U(Hr ) can appear in thedecomposition of Sm(∧NHr )?”

Surprisingly solution of this problem coincides with that of pureN-representability problem.

Murat Altunbulak Oxford 2016

Page 52: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Connection with Representation Theory

Plethysm

Consider the m-th symmetric power of ∧NHr , called Plethysm

It splits into irreducible components Hλ, parameterized by Young

diagrams λ = of size N.m, with multiplicity mλ

Sm(∧NHr ) =∑λ

mλHλ.

Problem

“Which irreducible representations Hλ of U(Hr ) can appear in thedecomposition of Sm(∧NHr )?”

Surprisingly solution of this problem coincides with that of pureN-representability problem.

Murat Altunbulak Oxford 2016

Page 53: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Connection with Representation Theory

Plethysm

Consider the m-th symmetric power of ∧NHr , called Plethysm

It splits into irreducible components Hλ, parameterized by Young

diagrams λ = of size N.m, with multiplicity mλ

Sm(∧NHr ) =∑λ

mλHλ.

Problem

“Which irreducible representations Hλ of U(Hr ) can appear in thedecomposition of Sm(∧NHr )?”

Surprisingly solution of this problem coincides with that of pureN-representability problem.

Murat Altunbulak Oxford 2016

Page 54: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Connection with Representation Theory

Plethysm

Consider the m-th symmetric power of ∧NHr , called Plethysm

It splits into irreducible components Hλ, parameterized by Young

diagrams λ = of size N.m, with multiplicity mλ

Sm(∧NHr ) =∑λ

mλHλ.

Problem

“Which irreducible representations Hλ of U(Hr ) can appear in thedecomposition of Sm(∧NHr )?”

Surprisingly solution of this problem coincides with that of pureN-representability problem.

Murat Altunbulak Oxford 2016

Page 55: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Connection with Representation Theory

Connection

treat the diagrams λ as spectra.λ : λ1 ≥ λ2 ≥ . . . ≥ λr .

normalize them to a fixed size λ̃ = λ/m s.t.

Trλ̃ = N.

Representation theoretical solution

Theorem. Every λ̃ obtained from irreducible componentHλ ⊂ Sm(∧NHr ) is a spectrum of one point reduced matrix ρ of a purestate ψ ∈ ∧NHr . Moreover every one point reduced spectrum is a convexcombination of such spectra λ̃ with bounded m ≤ M.

Murat Altunbulak Oxford 2016

Page 56: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Connection with Representation Theory

Connection

treat the diagrams λ as spectra.λ : λ1 ≥ λ2 ≥ . . . ≥ λr .normalize them to a fixed size λ̃ = λ/m s.t.

Trλ̃ = N.

Representation theoretical solution

Theorem. Every λ̃ obtained from irreducible componentHλ ⊂ Sm(∧NHr ) is a spectrum of one point reduced matrix ρ of a purestate ψ ∈ ∧NHr . Moreover every one point reduced spectrum is a convexcombination of such spectra λ̃ with bounded m ≤ M.

Murat Altunbulak Oxford 2016

Page 57: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Connection with Representation Theory

Connection

treat the diagrams λ as spectra.λ : λ1 ≥ λ2 ≥ . . . ≥ λr .normalize them to a fixed size λ̃ = λ/m s.t.

Trλ̃ = N.

Representation theoretical solution

Theorem. Every λ̃ obtained from irreducible componentHλ ⊂ Sm(∧NHr ) is a spectrum of one point reduced matrix ρ of a purestate ψ ∈ ∧NHr . Moreover every one point reduced spectrum is a convexcombination of such spectra λ̃ with bounded m ≤ M.

Murat Altunbulak Oxford 2016

Page 58: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Connection with Representation Theory

Connection

treat the diagrams λ as spectra.λ : λ1 ≥ λ2 ≥ . . . ≥ λr .normalize them to a fixed size λ̃ = λ/m s.t.

Trλ̃ = N.

Representation theoretical solution

Theorem. Every λ̃ obtained from irreducible componentHλ ⊂ Sm(∧NHr ) is a spectrum of one point reduced matrix ρ of a purestate ψ ∈ ∧NHr .

Moreover every one point reduced spectrum is a convexcombination of such spectra λ̃ with bounded m ≤ M.

Murat Altunbulak Oxford 2016

Page 59: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Connection with Representation Theory

Connection

treat the diagrams λ as spectra.λ : λ1 ≥ λ2 ≥ . . . ≥ λr .normalize them to a fixed size λ̃ = λ/m s.t.

Trλ̃ = N.

Representation theoretical solution

Theorem. Every λ̃ obtained from irreducible componentHλ ⊂ Sm(∧NHr ) is a spectrum of one point reduced matrix ρ of a purestate ψ ∈ ∧NHr . Moreover every one point reduced spectrum is a convexcombination of such spectra λ̃ with bounded m ≤ M.

Murat Altunbulak Oxford 2016

Page 60: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Practical Algorithm

Murat Altunbulak Oxford 2016

Page 61: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Practical Algorithm

For a fixed M the convex hull of the spectra λ̃ from previous Theoremgives an inner approximation to the moment polytope,

while any set ofinequalities of Main Theorem amounts to its outer approximation. Thissuggests the following approach to the pure N-representability problem,which combines both theorems.

The Algorithm

Find all irreducible components Hλ ⊂ Sm(∧NHr ) for m ≤ M.

Calculate the convex hull of the corresponding spectra λ̃ which givesan inner approximation P in

M ⊂ P for the moment polytope P.

Identify the facets of P inM that are given by the inequalities of the

Main Theorem. They cut out an outer approximation PoutM ⊃ P.

Increase M and continue until P inM = Pout

M .

Murat Altunbulak Oxford 2016

Page 62: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Practical Algorithm

For a fixed M the convex hull of the spectra λ̃ from previous Theoremgives an inner approximation to the moment polytope,while any set ofinequalities of Main Theorem amounts to its outer approximation.

Thissuggests the following approach to the pure N-representability problem,which combines both theorems.

The Algorithm

Find all irreducible components Hλ ⊂ Sm(∧NHr ) for m ≤ M.

Calculate the convex hull of the corresponding spectra λ̃ which givesan inner approximation P in

M ⊂ P for the moment polytope P.

Identify the facets of P inM that are given by the inequalities of the

Main Theorem. They cut out an outer approximation PoutM ⊃ P.

Increase M and continue until P inM = Pout

M .

Murat Altunbulak Oxford 2016

Page 63: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Practical Algorithm

For a fixed M the convex hull of the spectra λ̃ from previous Theoremgives an inner approximation to the moment polytope,while any set ofinequalities of Main Theorem amounts to its outer approximation. Thissuggests the following approach to the pure N-representability problem,which combines both theorems.

The Algorithm

Find all irreducible components Hλ ⊂ Sm(∧NHr ) for m ≤ M.

Calculate the convex hull of the corresponding spectra λ̃ which givesan inner approximation P in

M ⊂ P for the moment polytope P.

Identify the facets of P inM that are given by the inequalities of the

Main Theorem. They cut out an outer approximation PoutM ⊃ P.

Increase M and continue until P inM = Pout

M .

Murat Altunbulak Oxford 2016

Page 64: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Practical Algorithm

For a fixed M the convex hull of the spectra λ̃ from previous Theoremgives an inner approximation to the moment polytope,while any set ofinequalities of Main Theorem amounts to its outer approximation. Thissuggests the following approach to the pure N-representability problem,which combines both theorems.

The Algorithm

Find all irreducible components Hλ ⊂ Sm(∧NHr ) for m ≤ M.

Calculate the convex hull of the corresponding spectra λ̃ which givesan inner approximation P in

M ⊂ P for the moment polytope P.

Identify the facets of P inM that are given by the inequalities of the

Main Theorem. They cut out an outer approximation PoutM ⊃ P.

Increase M and continue until P inM = Pout

M .

Murat Altunbulak Oxford 2016

Page 65: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Practical Algorithm

For a fixed M the convex hull of the spectra λ̃ from previous Theoremgives an inner approximation to the moment polytope,while any set ofinequalities of Main Theorem amounts to its outer approximation. Thissuggests the following approach to the pure N-representability problem,which combines both theorems.

The Algorithm

Find all irreducible components Hλ ⊂ Sm(∧NHr ) for m ≤ M.

Calculate the convex hull of the corresponding spectra λ̃ which givesan inner approximation P in

M ⊂ P for the moment polytope P.

Identify the facets of P inM that are given by the inequalities of the

Main Theorem. They cut out an outer approximation PoutM ⊃ P.

Increase M and continue until P inM = Pout

M .

Murat Altunbulak Oxford 2016

Page 66: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Practical Algorithm

For a fixed M the convex hull of the spectra λ̃ from previous Theoremgives an inner approximation to the moment polytope,while any set ofinequalities of Main Theorem amounts to its outer approximation. Thissuggests the following approach to the pure N-representability problem,which combines both theorems.

The Algorithm

Find all irreducible components Hλ ⊂ Sm(∧NHr ) for m ≤ M.

Calculate the convex hull of the corresponding spectra λ̃ which givesan inner approximation P in

M ⊂ P for the moment polytope P.

Identify the facets of P inM that are given by the inequalities of the

Main Theorem. They cut out an outer approximation PoutM ⊃ P.

Increase M and continue until P inM = Pout

M .

Murat Altunbulak Oxford 2016

Page 67: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Practical Algorithm

For a fixed M the convex hull of the spectra λ̃ from previous Theoremgives an inner approximation to the moment polytope,while any set ofinequalities of Main Theorem amounts to its outer approximation. Thissuggests the following approach to the pure N-representability problem,which combines both theorems.

The Algorithm

Find all irreducible components Hλ ⊂ Sm(∧NHr ) for m ≤ M.

Calculate the convex hull of the corresponding spectra λ̃ which givesan inner approximation P in

M ⊂ P for the moment polytope P.

Identify the facets of P inM that are given by the inequalities of the

Main Theorem. They cut out an outer approximation PoutM ⊃ P.

Increase M and continue until P inM = Pout

M .

Murat Altunbulak Oxford 2016

Page 68: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

How it works?

Murat Altunbulak Oxford 2016

Page 69: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

How it works?

The above algorithm works perfectly only for some small systems.

Borland-Dennis System (N = 3, r = 6)

We only need to calculate symmetric powers of ∧3H6 up to 4th degree.

That is, M = 4.Symmetric powers contains the following components

m λ1 [1, 1, 1, 0, 0, 0]2 [2, 2, 2, 0, 0, 0], [2, 1, 1, 1, 1, 0]3 [2, 2, 2, 1, 1, 1], [3, 3, 3, 0, 0, 0], [3, 2, 2, 1, 1, 0]4 [2, 2, 2, 2, 2, 2], [3, 3, 3, 1, 1, 1], [4, 4, 4, 0, 0, 0],

[3, 3, 2, 2, 1, 1], [4, 3, 3, 1, 1, 0], [4, 2, 2, 2, 2, 0]

Murat Altunbulak Oxford 2016

Page 70: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

How it works?

The above algorithm works perfectly only for some small systems.

Borland-Dennis System (N = 3, r = 6)

We only need to calculate symmetric powers of ∧3H6 up to 4th degree.That is, M = 4.

Symmetric powers contains the following components

m λ1 [1, 1, 1, 0, 0, 0]2 [2, 2, 2, 0, 0, 0], [2, 1, 1, 1, 1, 0]3 [2, 2, 2, 1, 1, 1], [3, 3, 3, 0, 0, 0], [3, 2, 2, 1, 1, 0]4 [2, 2, 2, 2, 2, 2], [3, 3, 3, 1, 1, 1], [4, 4, 4, 0, 0, 0],

[3, 3, 2, 2, 1, 1], [4, 3, 3, 1, 1, 0], [4, 2, 2, 2, 2, 0]

Murat Altunbulak Oxford 2016

Page 71: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

How it works?

The above algorithm works perfectly only for some small systems.

Borland-Dennis System (N = 3, r = 6)

We only need to calculate symmetric powers of ∧3H6 up to 4th degree.That is, M = 4.Symmetric powers contains the following components

m λ1 [1, 1, 1, 0, 0, 0]2 [2, 2, 2, 0, 0, 0], [2, 1, 1, 1, 1, 0]3 [2, 2, 2, 1, 1, 1], [3, 3, 3, 0, 0, 0], [3, 2, 2, 1, 1, 0]4 [2, 2, 2, 2, 2, 2], [3, 3, 3, 1, 1, 1], [4, 4, 4, 0, 0, 0],

[3, 3, 2, 2, 1, 1], [4, 3, 3, 1, 1, 0], [4, 2, 2, 2, 2, 0]

Murat Altunbulak Oxford 2016

Page 72: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

How it works?

The above algorithm works perfectly only for some small systems.

Borland-Dennis System (N = 3, r = 6)

We only need to calculate symmetric powers of ∧3H6 up to 4th degree.That is, M = 4.Symmetric powers contains the following components

m λ1 [1, 1, 1, 0, 0, 0]2 [2, 2, 2, 0, 0, 0], [2, 1, 1, 1, 1, 0]3 [2, 2, 2, 1, 1, 1], [3, 3, 3, 0, 0, 0], [3, 2, 2, 1, 1, 0]4 [2, 2, 2, 2, 2, 2], [3, 3, 3, 1, 1, 1], [4, 4, 4, 0, 0, 0],

[3, 3, 2, 2, 1, 1], [4, 3, 3, 1, 1, 0], [4, 2, 2, 2, 2, 0]

Murat Altunbulak Oxford 2016

Page 73: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

How it works?

Borland-Dennis System (N = 3, r = 6)

After the normalization we obtain the spectra λ̃

m λ̃1 [1, 1, 1, 0, 0, 0]2 [1, 1, 1, 0, 0, 0], [1, 12 ,

12 ,

12 ,

12 , 0]

3 [ 23 ,23 ,

23 ,

23 ,

13 ,

13 ], [1, 1, 1, 0, 0, 0], [1, 23 ,

23 ,

13 ,

13 , 0]

4 [ 12 ,12 ,

12 ,

12 ,

12 ,

12 ], [ 34 ,

34 ,

34 ,

14 ,

14 ,

14 ], [1, 1, 1, 0, 0, 0],

[ 34 ,34 ,

12 ,

12 ,

14 ,

14 ], [1, 34 ,

34 ,

14 ,

14 , 0], [1, 12 ,

12 ,

12 ,

12 , 0]

Taking convex hull of these spectra we obtain the full moment polytopewhich is described by 3 equalities and 1 inequality.

N = 3, r = 7

M = 8.

N = 4, r = 8

M = 10.

Murat Altunbulak Oxford 2016

Page 74: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

How it works?

Borland-Dennis System (N = 3, r = 6)

After the normalization we obtain the spectra λ̃

m λ̃1 [1, 1, 1, 0, 0, 0]2 [1, 1, 1, 0, 0, 0], [1, 12 ,

12 ,

12 ,

12 , 0]

3 [ 23 ,23 ,

23 ,

23 ,

13 ,

13 ], [1, 1, 1, 0, 0, 0], [1, 23 ,

23 ,

13 ,

13 , 0]

4 [ 12 ,12 ,

12 ,

12 ,

12 ,

12 ], [ 34 ,

34 ,

34 ,

14 ,

14 ,

14 ], [1, 1, 1, 0, 0, 0],

[ 34 ,34 ,

12 ,

12 ,

14 ,

14 ], [1, 34 ,

34 ,

14 ,

14 , 0], [1, 12 ,

12 ,

12 ,

12 , 0]

Taking convex hull of these spectra we obtain the full moment polytopewhich is described by 3 equalities and 1 inequality.

N = 3, r = 7

M = 8.

N = 4, r = 8

M = 10.

Murat Altunbulak Oxford 2016

Page 75: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

How it works?

Borland-Dennis System (N = 3, r = 6)

After the normalization we obtain the spectra λ̃

m λ̃1 [1, 1, 1, 0, 0, 0]2 [1, 1, 1, 0, 0, 0], [1, 12 ,

12 ,

12 ,

12 , 0]

3 [ 23 ,23 ,

23 ,

23 ,

13 ,

13 ], [1, 1, 1, 0, 0, 0], [1, 23 ,

23 ,

13 ,

13 , 0]

4 [ 12 ,12 ,

12 ,

12 ,

12 ,

12 ], [ 34 ,

34 ,

34 ,

14 ,

14 ,

14 ], [1, 1, 1, 0, 0, 0],

[ 34 ,34 ,

12 ,

12 ,

14 ,

14 ], [1, 34 ,

34 ,

14 ,

14 , 0], [1, 12 ,

12 ,

12 ,

12 , 0]

Taking convex hull of these spectra we obtain the full moment polytopewhich is described by 3 equalities and 1 inequality.

N = 3, r = 7

M = 8.

N = 4, r = 8

M = 10.

Murat Altunbulak Oxford 2016

Page 76: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

How it works?

Borland-Dennis System (N = 3, r = 6)

After the normalization we obtain the spectra λ̃

m λ̃1 [1, 1, 1, 0, 0, 0]2 [1, 1, 1, 0, 0, 0], [1, 12 ,

12 ,

12 ,

12 , 0]

3 [ 23 ,23 ,

23 ,

23 ,

13 ,

13 ], [1, 1, 1, 0, 0, 0], [1, 23 ,

23 ,

13 ,

13 , 0]

4 [ 12 ,12 ,

12 ,

12 ,

12 ,

12 ], [ 34 ,

34 ,

34 ,

14 ,

14 ,

14 ], [1, 1, 1, 0, 0, 0],

[ 34 ,34 ,

12 ,

12 ,

14 ,

14 ], [1, 34 ,

34 ,

14 ,

14 , 0], [1, 12 ,

12 ,

12 ,

12 , 0]

Taking convex hull of these spectra we obtain the full moment polytopewhich is described by 3 equalities and 1 inequality.

N = 3, r = 7

M = 8.

N = 4, r = 8

M = 10.Murat Altunbulak Oxford 2016

Page 77: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

How it works?

N = 3, r = 8

Using the above algorithm we manage to calculate symmetric powers upto M = 24. Resulting polytope was not the full moment polytope.That is, P in

24 6= Pout24 .

There was one problematic facet.To get rid of this, we resort to use a numerical minimization of the linearform obtained from the problematic facet over all particle densitymatrices.It turns out that the form attains its minimum at a single point.Adding this new point gives a polytope P whose all facets are covered bythe Main Theorem.Thus the polytope is the genuine moment polytope for ∧3H8 which isgiven by 31 independent inequalities.

Murat Altunbulak Oxford 2016

Page 78: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

How it works?

N = 3, r = 8

Using the above algorithm we manage to calculate symmetric powers upto M = 24. Resulting polytope was not the full moment polytope.

That is, P in24 6= Pout

24 .There was one problematic facet.To get rid of this, we resort to use a numerical minimization of the linearform obtained from the problematic facet over all particle densitymatrices.It turns out that the form attains its minimum at a single point.Adding this new point gives a polytope P whose all facets are covered bythe Main Theorem.Thus the polytope is the genuine moment polytope for ∧3H8 which isgiven by 31 independent inequalities.

Murat Altunbulak Oxford 2016

Page 79: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

How it works?

N = 3, r = 8

Using the above algorithm we manage to calculate symmetric powers upto M = 24. Resulting polytope was not the full moment polytope.That is, P in

24 6= Pout24 .

There was one problematic facet.To get rid of this, we resort to use a numerical minimization of the linearform obtained from the problematic facet over all particle densitymatrices.It turns out that the form attains its minimum at a single point.Adding this new point gives a polytope P whose all facets are covered bythe Main Theorem.Thus the polytope is the genuine moment polytope for ∧3H8 which isgiven by 31 independent inequalities.

Murat Altunbulak Oxford 2016

Page 80: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

How it works?

N = 3, r = 8

Using the above algorithm we manage to calculate symmetric powers upto M = 24. Resulting polytope was not the full moment polytope.That is, P in

24 6= Pout24 .

There was one problematic facet.

To get rid of this, we resort to use a numerical minimization of the linearform obtained from the problematic facet over all particle densitymatrices.It turns out that the form attains its minimum at a single point.Adding this new point gives a polytope P whose all facets are covered bythe Main Theorem.Thus the polytope is the genuine moment polytope for ∧3H8 which isgiven by 31 independent inequalities.

Murat Altunbulak Oxford 2016

Page 81: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

How it works?

N = 3, r = 8

Using the above algorithm we manage to calculate symmetric powers upto M = 24. Resulting polytope was not the full moment polytope.That is, P in

24 6= Pout24 .

There was one problematic facet.To get rid of this, we resort to use a numerical minimization of the linearform obtained from the problematic facet over all particle densitymatrices.

It turns out that the form attains its minimum at a single point.Adding this new point gives a polytope P whose all facets are covered bythe Main Theorem.Thus the polytope is the genuine moment polytope for ∧3H8 which isgiven by 31 independent inequalities.

Murat Altunbulak Oxford 2016

Page 82: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

How it works?

N = 3, r = 8

Using the above algorithm we manage to calculate symmetric powers upto M = 24. Resulting polytope was not the full moment polytope.That is, P in

24 6= Pout24 .

There was one problematic facet.To get rid of this, we resort to use a numerical minimization of the linearform obtained from the problematic facet over all particle densitymatrices.It turns out that the form attains its minimum at a single point.

Adding this new point gives a polytope P whose all facets are covered bythe Main Theorem.Thus the polytope is the genuine moment polytope for ∧3H8 which isgiven by 31 independent inequalities.

Murat Altunbulak Oxford 2016

Page 83: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

How it works?

N = 3, r = 8

Using the above algorithm we manage to calculate symmetric powers upto M = 24. Resulting polytope was not the full moment polytope.That is, P in

24 6= Pout24 .

There was one problematic facet.To get rid of this, we resort to use a numerical minimization of the linearform obtained from the problematic facet over all particle densitymatrices.It turns out that the form attains its minimum at a single point.Adding this new point gives a polytope P whose all facets are covered bythe Main Theorem.

Thus the polytope is the genuine moment polytope for ∧3H8 which isgiven by 31 independent inequalities.

Murat Altunbulak Oxford 2016

Page 84: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

How it works?

N = 3, r = 8

Using the above algorithm we manage to calculate symmetric powers upto M = 24. Resulting polytope was not the full moment polytope.That is, P in

24 6= Pout24 .

There was one problematic facet.To get rid of this, we resort to use a numerical minimization of the linearform obtained from the problematic facet over all particle densitymatrices.It turns out that the form attains its minimum at a single point.Adding this new point gives a polytope P whose all facets are covered bythe Main Theorem.Thus the polytope is the genuine moment polytope for ∧3H8 which isgiven by 31 independent inequalities.

Murat Altunbulak Oxford 2016

Page 85: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Number of Constraints for systems of rank ≤ 10

r N Number of constraints7 3 48 3 318 4 159 3 529 4 60

10 3 9310 4 12510 5 161

Murat Altunbulak Oxford 2016

Page 86: Calculation of Generalized Pauli Constraints · In terms of electron density matrix ˆ, Pauli principle amounts to h jˆj i 1 ()Specˆ 1 Modern Version (1926) Heisenberg-Dirac replaced

Thank You for your attention!!!

Murat Altunbulak Oxford 2016