Davida Kollmar Department of Physics, Yeshiva University ... · Detecting Transitions Have been...

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Davida Kollmar Department of Physics, Yeshiva University, New York, NY Collaborators: Lea F. Santos (Yeshiva University, New York, NY)

Transcript of Davida Kollmar Department of Physics, Yeshiva University ... · Detecting Transitions Have been...

Page 1: Davida Kollmar Department of Physics, Yeshiva University ... · Detecting Transitions Have been different ways to detect these transitions, borrowing tools from quantum information

Davida Kollmar

Department of Physics, Yeshiva University, New York, NY

Collaborators:

Lea F. Santos (Yeshiva University, New York, NY)

Page 2: Davida Kollmar Department of Physics, Yeshiva University ... · Detecting Transitions Have been different ways to detect these transitions, borrowing tools from quantum information

Outline

Introduction to QPTs

Introduction to ICE

Examine specific spin-½ systems

Page 3: Davida Kollmar Department of Physics, Yeshiva University ... · Detecting Transitions Have been different ways to detect these transitions, borrowing tools from quantum information

Introduction to QPTs

Quantum Phase Transitions

Competition between terms

𝐻 = 𝐻0 + 𝑔𝐻1

Opening/closing energy gap

Orders of Transitions

○ Berezinskii-Kosterlitz-Thouless transition

Examine the ground state and first

excited state

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Detecting Transitions

Have been different ways to detect these transitions, borrowing tools from quantum information

Entanglement

○ Concurrence

○ Entanglement entropy

○ Quantum Discord

Fidelity

𝐹 = Ψ λ Ψ λ + 𝛿

ICE

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Invariant Correlational Entropy

This quantity is given by

𝑆 = −Tr {𝜌 ln(𝜌 )}

Use average energy density matrix:

𝜌 =𝜌𝑔 + 𝜌𝑔+𝛿 +⋯+ 𝜌𝑔+(𝑁−1)𝛿

𝑁

Check graph for peaks or inflection points

Page 6: Davida Kollmar Department of Physics, Yeshiva University ... · Detecting Transitions Have been different ways to detect these transitions, borrowing tools from quantum information

1D Spin-½

Typical many body system

Good model for real materials

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XXZ Model-Heisenberg Model

The Hamiltonian for this model is given

by:

𝐻 = 𝐽 𝑆𝑗𝑥𝑆𝑗+1𝑥 + 𝑆𝑗

𝑦𝑆𝑗+1𝑦+ ∆𝑆𝑗

𝑧𝑆𝑗+1𝑧

𝐿

𝑗=1

Parameter to vary: Δ

antiferromagnetic ferromagnetic xy

-1 1

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XXZ Model-Heisenberg Model

-2 -1 0 1 2D

-3.5

-3

-2.5

-2

-1.5

-1

-0.5E

ner

gy

Sz=-3,3 Sz=0

Sz=-1,1

Sz=0

Sz=-1,1

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XXZ Model-Heisenberg Model

0 0.5 1 1.5 2D

0

0.2

0.4

0.6

0.8

1

Fid

elit

y

First Excited State

L=10 𝐹 = Ψ λ Ψ λ + 𝛿

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Using ICE on the XXZ Model

First excited state: peak at transition

Ground state: inflection point at

transition

0 0.5 1 1.5 2D

0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

Inv

aria

nt

Co

rrel

atio

nal

En

tro

py

First Excited

State

L=10

0 0.5 1 1.5D

0.02

0.04

0.06

0.08

Inv

ari

an

t C

orr

ela

tio

nal

En

tro

py

L=12

L=10

L=8

L=6

Ground

State

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NN+NNN Model

The Hamiltonian for this model is:

𝐻 = 𝑆𝑗𝑆𝑗+1 + 𝜆𝑆𝑗𝑆𝑗+2

𝐿

𝑗=1

Parameter to vary: λ

The transition is found numerically,

where an energy gap appears

fluid dimer

0.241

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NN+NNN Model

First excited state, not ground state

Sz=0 subspace

0 0.1 0.2 0.3 0.4 0.5D

-4.4

-4.2

-4

-3.8

-3.6

-3.4

-3.2

En

erg

y

Sz=-1,0,1

Sz=-1,0,1

Sz=0

Sz=0

λ

Chen et al

PRE 76, 061108 (2007)

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NN+NNN Model: ICE

First excited state: peak at transition

L=8

L=6

L=10

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Future Directions

Examine different models

Ising Model in the Transverse Field

Bose Einstein Condensate

Study larger systems

Scaling analysis

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Acknowledgements

Dr. Berliner, Dr. Kressel, and the Kressel

Research Scholarship committee

Deans at Stern College for Women