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Is the Feynman path integral complex enough? Gke Ba ar University - - PowerPoint PPT Presentation

Is the Feynman path integral complex enough? Gke Ba ar University of North Carolina, Chapel Hill 04.22.2020 [with A. Alexandru, P. Bedaque, N. Warrington, G. Ridgway] 1 Motivations first-principles studies of strongly interacting


slide-1
SLIDE 1

Is the Feynman path integral complex enough?

Gökçe Başar

University of North Carolina, Chapel Hill

04.22.2020

1

[with A. Alexandru, P. Bedaque, N. Warrington, G. Ridgway]

slide-2
SLIDE 2

Motivations

2

first-principles studies of strongly interacting systems

slide-3
SLIDE 3

Motivations

3

slide-4
SLIDE 4

Motivations

temperature 1012 K chemical potential ∼310 MeV

heavy ion coll. early universe

quark gluon plasma hadron gas

you are here neutron stars

??

critical point

4

first-principles studies of strongly interacting systems

slide-5
SLIDE 5

Motivations: out-of-equilibrium, transport

5

Heavy ion collisions: Quark gluon plasma is a liquid !

slide-6
SLIDE 6

Motivations: out-of-equilibrium, transport

6

Heavy ion collisions: Quark gluon plasma is a liquid !

slide-7
SLIDE 7

Motivations: out-of-equilibrium, transport

7

Heavy ion collisions: Quark gluon plasma is a liquid !

slide-8
SLIDE 8

Motivations: out-of-equilibrium, transport

8

Heavy ion collisions: Quark gluon plasma is a liquid !

slide-9
SLIDE 9

Motivations: out-of-equilibrium, transport

9

Quark gluon plasma is a liquid what is the viscosity, conductivity …?

slide-10
SLIDE 10

Motivations

10

0.05 0.1 0.15 0.2 0.25 0.3

T (K) Hole doping x

~ T2 ~ T + T2

  • r

TFL? Tcoh? ~ T (T) S-shaped T* d-wave SC ~ Tn (1 < n < 2) A F M upturns in (T) [N.E. Hussey, ’08 ]

first-principles studies of strongly interacting systems

slide-11
SLIDE 11

Quantum Chromo Dynamics (QCD)

We know how quarks and gluons interact Why not just compute the phase diagram, viscosity, equation of state, etc…?

11

slide-12
SLIDE 12

Quantum fluctuations

animation: Derek Leinweber, University of Adelaide

we are interested in expectation values

⟨n⟩ ⇔ equation of state ⟨J(t)J(0)⟩ ⇔ conductivity ⟨Tab(t)Tcd(0)⟩ ⇔ viscosity

examples:

12

slide-13
SLIDE 13

Feynman path integral

~ ""g7

VO1.UME 20, NUMBER 2

  • Aran. , 1948

Space- ..ime A~~~iroac. i 1:o .5 on-.le. .a1:ivistic

4 uantuns

.V.:ec.zanies

  • R. P. I EvNMAN

Cornell University,

Ithaca, Veto York

Non-relativistic quantum mechanics is formulated here in a different

  • way. It is, however,

mathematically equivalent

to the familiar formulation. In quantum

mechanics the probability

  • f an event

which can happen in several different ways is the absolute square

  • f a sum of

complex contributions,

  • ne from each alternative
  • way. The probability

that a particle

will be

found to have a path x(t) lying somewhere within a region of space time is the square of a sum

  • f contributions,
  • ne from each path

in the region. The contribution from a single path is

postulated

to be an exponential

whose (imaginary) phase is the classical action (in units of h)

for the path in question. The total contribution

from all paths reaching x, t from the past is the wave function P(x, t). This is shown to satisfy Schroedinger's equation.

The relation to matrix and operator algebra is discussed.

Applications are indicated, in particular

to eliminate

the coordinates

  • f the field oscillators

from the equations

  • f quantum

electrodynamics.

  • I. INTRODUCTION

;'I is a curious

historical

fact that

modern

& - quantum

mechanics began with two quite di8'erent mathematical formulations:

the differ-

ential equation

  • f Schroedinger,

and the matrix algebra of Heisenberg.

The two, apparently

dis- similar approaches, were proved

to be mathe-

matically equivalent. These two points of view

were, destined

to complement

  • ne another

and

to be ultimately

synthesized

in Dirac's

trans- formation theory.

This paper

will describe what

is essentially

a

third formulation

  • f non-relativistic

quantum

  • theory. This formulation

was suggested

by some

  • f Dirac's' ' remarks

concerning

the relation

  • f

classical action' to quantum

  • mechanics. A proba-

bility amplitude

is associated

with an

entire motion of a particle as a function of time, rather than

simply with a position of the particle at a

particular time.

The formulation

is mathematically

equivalent

to

the

more usual formulations.

There are,

therefore, no fundamentally

new results.

How- ever, there is a pleasure

in recognizing

  • ld things

from a new point of view. Also, there are prob- lems for which

the new

point

  • f view offers a

distinct advantage.

For example,

if two systems A and 8 interact,

the coordinates

  • f one of the

systems, say 8, may

be eliminated

from

the

equations describing the motion of A. The inter-

' P. A. M. Dirac, The Principles

  • f Quantum

3Eeohanics

(The

Clarendon Press, Oxford,

1935), second

edition,

Section 33;also, Physik. Zeits. Sowjetunion 3, 64 (1933).

' P. A. M. Dirac, Rev. Mod. Phys.

1'7, 195 (1945).

3 Throughout

this paper the term "action" will be used for the time integral

  • f the

Lagrangian along a path. %'hen this path is the one actually taken by a particle, moving classically,

the integral

should

more properly be called Hamilton's

6rst principle

function.

367

x(t)

space is the square of a sum

  • f contributions,
  • ne from each path

in the region. The contribution

from a single path is postulated

to be an exponential

whose (imaginary) phase is the classical action (in units of h)

for the path in question. The total contribution

from all paths reaching x, t from the past is the wave function P(x, t). This is shown to satisfy Schroedinger's

equation. The relation to matrix

ⅈ S [ x ( t ) ]

x(t)

13

slide-14
SLIDE 14

x(t)

space is the square of a sum

  • f contributions,
  • ne from each path

in the region. The contribution

from a single path is postulated

to be an exponential

whose (imaginary) phase is the classical action (in units of h)

for the path in question. The total contribution

from all paths reaching x, t from the past is the wave function P(x, t). This is shown to satisfy Schroedinger's

equation. The relation to matrix

field field

~ ""g7

VO1.UME 20, NUMBER 2

  • Aran. , 1948

Space- ..ime A~~~iroac. i 1:o .5 on-.le. .a1:ivistic

4 uantuns

.V.:ec.zanies

  • R. P. I EvNMAN

Cornell University,

Ithaca, Veto York

Non-relativistic quantum mechanics is formulated here in a different

  • way. It is, however,

mathematically equivalent

to the familiar formulation. In quantum

mechanics the probability

  • f an event

which can happen in several different ways is the absolute square

  • f a sum of

complex contributions,

  • ne from each alternative
  • way. The probability

that a particle

will be

found to have a path x(t) lying somewhere within a region of space time is the square of a sum

  • f contributions,
  • ne from each path

in the region. The contribution from a single path is

postulated

to be an exponential

whose (imaginary) phase is the classical action (in units of h)

for the path in question. The total contribution

from all paths reaching x, t from the past is the wave function P(x, t). This is shown to satisfy Schroedinger's equation.

The relation to matrix and operator algebra is discussed.

Applications are indicated, in particular

to eliminate

the coordinates

  • f the field oscillators

from the equations

  • f quantum

electrodynamics.

  • I. INTRODUCTION

;'I is a curious

historical

fact that

modern

& - quantum

mechanics began with two quite di8'erent mathematical formulations:

the differ-

ential equation

  • f Schroedinger,

and the matrix algebra of Heisenberg.

The two, apparently

dis- similar approaches, were proved

to be mathe-

matically equivalent. These two points of view

were, destined

to complement

  • ne another

and

to be ultimately

synthesized

in Dirac's

trans- formation theory.

This paper

will describe what

is essentially

a

third formulation

  • f non-relativistic

quantum

  • theory. This formulation

was suggested

by some

  • f Dirac's' ' remarks

concerning

the relation

  • f

classical action' to quantum

  • mechanics. A proba-

bility amplitude

is associated

with an

entire motion of a particle as a function of time, rather than

simply with a position of the particle at a

particular time.

The formulation

is mathematically

equivalent

to

the

more usual formulations.

There are,

therefore, no fundamentally

new results.

How- ever, there is a pleasure

in recognizing

  • ld things

from a new point of view. Also, there are prob- lems for which

the new

point

  • f view offers a

distinct advantage.

For example,

if two systems A and 8 interact,

the coordinates

  • f one of the

systems, say 8, may

be eliminated

from

the

equations describing the motion of A. The inter-

' P. A. M. Dirac, The Principles

  • f Quantum

3Eeohanics

(The

Clarendon Press, Oxford,

1935), second

edition,

Section 33;also, Physik. Zeits. Sowjetunion 3, 64 (1933).

' P. A. M. Dirac, Rev. Mod. Phys.

1'7, 195 (1945).

3 Throughout

this paper the term "action" will be used for the time integral

  • f the

Lagrangian along a path. %'hen this path is the one actually taken by a particle, moving classically,

the integral

should

more properly be called Hamilton's

6rst principle

function.

367

~ ""g7

VO1.UME 20, NUMBER 2

  • Aran. , 1948

Space- ..ime A~~~iroac. i 1:o .5 on-.le. .a1:ivistic

4 uantuns

.V.:ec.zanies

  • R. P. I EvNMAN

Cornell University,

Ithaca, Veto York

Non-relativistic quantum mechanics is formulated here in a different

  • way. It is, however,

mathematically equivalent

to the familiar formulation. In quantum

mechanics the probability

  • f an event

which can happen in several different ways is the absolute square

  • f a sum of

complex contributions,

  • ne from each alternative
  • way. The probability

that a particle

will be

found to have a path x(t) lying somewhere within a region of space time is the square of a sum

  • f contributions,
  • ne from each path

in the region. The contribution from a single path is

postulated

to be an exponential

whose (imaginary) phase is the classical action (in units of h)

for the path in question. The total contribution

from all paths reaching x, t from the past is the wave function P(x, t). This is shown to satisfy Schroedinger's equation.

The relation to matrix and operator algebra is discussed.

Applications are indicated, in particular

to eliminate

the coordinates

  • f the field oscillators

from the equations

  • f quantum

electrodynamics.

  • I. INTRODUCTION

;'I is a curious

historical

fact that

modern

& - quantum

mechanics began with two quite di8'erent mathematical formulations:

the differ-

ential equation

  • f Schroedinger,

and the matrix algebra of Heisenberg.

The two, apparently

dis- similar approaches, were proved

to be mathe-

matically equivalent. These two points of view

were, destined

to complement

  • ne another

and

to be ultimately

synthesized

in Dirac's

trans- formation theory.

This paper

will describe what

is essentially

a

third formulation

  • f non-relativistic

quantum

  • theory. This formulation

was suggested

by some

  • f Dirac's' ' remarks

concerning

the relation

  • f

classical action' to quantum

  • mechanics. A proba-

bility amplitude

is associated

with an

entire motion of a particle as a function of time, rather than

simply with a position of the particle at a

particular time.

The formulation

is mathematically

equivalent

to

the

more usual formulations.

There are,

therefore, no fundamentally

new results.

How- ever, there is a pleasure

in recognizing

  • ld things

from a new point of view. Also, there are prob- lems for which

the new

point

  • f view offers a

distinct advantage.

For example,

if two systems A and 8 interact,

the coordinates

  • f one of the

systems, say 8, may

be eliminated

from

the

equations describing the motion of A. The inter-

' P. A. M. Dirac, The Principles

  • f Quantum

3Eeohanics

(The

Clarendon Press, Oxford,

1935), second

edition,

Section 33;also, Physik. Zeits. Sowjetunion 3, 64 (1933).

' P. A. M. Dirac, Rev. Mod. Phys.

1'7, 195 (1945).

3 Throughout

this paper the term "action" will be used for the time integral

  • f the

Lagrangian along a path. %'hen this path is the one actually taken by a particle, moving classically,

the integral

should

more properly be called Hamilton's

6rst principle

function.

367

Fields

The QFT path integral

⟨𝒫⟩ = ∫ [dϕ]eiS[ϕ]𝒫[ϕ]

all fields

14

domain of PI: space of all fields

ϕ

slide-15
SLIDE 15

x(t)

space is the square of a sum

  • f contributions,
  • ne from each path

in the region. The contribution

from a single path is postulated

to be an exponential

whose (imaginary) phase is the classical action (in units of h)

for the path in question. The total contribution

from all paths reaching x, t from the past is the wave function P(x, t). This is shown to satisfy Schroedinger's

equation. The relation to matrix

field field

real part with imaginary time

A crash course on Lattice Field Theory

~ ""g7

VO1.UME 20, NUMBER 2

  • Aran. , 1948

Space- ..ime A~~~iroac. i 1:o .5 on-.le. .a1:ivistic

4 uantuns

.V.:ec.zanies

  • R. P. I EvNMAN

Cornell University,

Ithaca, Veto York

Non-relativistic quantum mechanics is formulated here in a different

  • way. It is, however,

mathematically equivalent

to the familiar formulation. In quantum

mechanics the probability

  • f an event

which can happen in several different ways is the absolute square

  • f a sum of

complex contributions,

  • ne from each alternative
  • way. The probability

that a particle

will be

found to have a path x(t) lying somewhere within a region of space time is the square of a sum

  • f contributions,
  • ne from each path

in the region. The contribution from a single path is

postulated

to be an exponential

whose (imaginary) phase is the classical action (in units of h)

for the path in question. The total contribution

from all paths reaching x, t from the past is the wave function P(x, t). This is shown to satisfy Schroedinger's equation.

The relation to matrix and operator algebra is discussed.

Applications are indicated, in particular

to eliminate

the coordinates

  • f the field oscillators

from the equations

  • f quantum

electrodynamics.

  • I. INTRODUCTION

;'I is a curious

historical

fact that

modern

& - quantum

mechanics began with two quite di8'erent mathematical formulations:

the differ-

ential equation

  • f Schroedinger,

and the matrix algebra of Heisenberg.

The two, apparently

dis- similar approaches, were proved

to be mathe-

matically equivalent. These two points of view

were, destined

to complement

  • ne another

and

to be ultimately

synthesized

in Dirac's

trans- formation theory.

This paper will describe what

is essentially

a

third formulation

  • f non-relativistic

quantum

  • theory. This formulation

was suggested

by some

  • f Dirac's' ' remarks

concerning

the relation

  • f

classical action' to quantum

  • mechanics. A proba-

bility amplitude

is associated

with an

entire motion of a particle as a function of time, rather than

simply with a position of the particle at a

particular time.

The formulation

is mathematically

equivalent

to

the

more usual formulations.

There are,

therefore, no fundamentally

new results.

How- ever, there is a pleasure

in recognizing

  • ld things

from a new point of view. Also, there are prob- lems for which

the new

point

  • f view offers a

distinct advantage.

For example,

if two systems A and 8 interact,

the coordinates

  • f one of the

systems, say 8, may

be eliminated

from

the

equations describing the motion of A. The inter-

' P. A. M. Dirac, The Principles

  • f Quantum

3Eeohanics

(The

Clarendon Press, Oxford,

1935), second

edition,

Section 33;also, Physik. Zeits. Sowjetunion 3, 64 (1933).

' P. A. M. Dirac, Rev. Mod. Phys.

1'7, 195 (1945).

3 Throughout

this paper the term "action" will be used for the time integral

  • f the

Lagrangian along a path. %'hen this path is the one actually taken by a particle, moving classically,

the integral

should

more properly be called Hamilton's

6rst principle

function.

367

Fields Lattice

  • Discrete space-time
  • Imaginary time

e−i ̂

Ht → e− ̂ Hτ

thermal physics!

Main features:

15

slide-16
SLIDE 16

A crash course on Lattice Field Theory

  • Discrete space-time
  • Imaginary time

e−i ̂

Ht → e− ̂ Hτ

thermal physics!

Main features:

⟨𝒫⟩ = ∫ 𝒫[ϕ] = Tr[e− ̂

H/T ̂

𝒫] e−S[ϕ] dϕ1…dϕN

finite positive

e−S[ϕ]

  • importance of the field configuration 𝜚:

16

slide-17
SLIDE 17

Importance sampling (“Monte-Carlo” method)

e−S[ϕ]

importance of the field configuration 𝜚:

|

:

¥r¥

:

*

¥ A

. . . . . . . . . . . .

As

"

.

space of all fields

pick out the important (small action) configurations path integral ~ statistical average with

P(ϕ) ∝ e−S[ϕ]

⟨𝒫⟩ ≈ 1 𝒪

𝒪

a=1

𝒫[ϕa]

17

slide-18
SLIDE 18

Lattice QCD

lattice importance sampling (Monte-Carlo)

18

slide-19
SLIDE 19

The sign problem

19

In a variety of problems of interest S is complex

  • Most theories with finite density
  • Hubbard model away from half filling
  • Dynamical problems (transport, out-of-equilibrium physics…)
  • QCD with nonzero 𝞲 angle

. . .

e−S[ϕ] is not a probability distribution

slide-20
SLIDE 20

The sign problem

20

  • 4
  • 2

2 4 x

  • 3.5x10191

3.5x10191 Re[ⅇ-S]

∞ −∞

e−(x+42i)2dx = 2 π

slide-21
SLIDE 21

The sign problem

finite density

  • ut-of-equlibrium

∝ e−SR[ϕ]

importance ∝ e−SR[ϕ]

“reweighting”

⟨𝒫⟩ = ⟨𝒫e−iSI[ϕ]⟩SR ⟨e−iSI[ϕ]⟩SR ⟨e−iSI[ϕ]⟩SR ∝ e−volume/T

need exponentially large resources

21

slide-22
SLIDE 22

The sign problem

low − T

QGP

22

slide-23
SLIDE 23

Ways around the sign problem

low − T

QGP

23

  • Imaginary chemical potential
  • Taylor series in
  • Dual variables
  • Fermion bags
  • Complex Langevin
  • Canonical partition function

. . .

μ

slide-24
SLIDE 24

A complex way around the sign problem

∞ −∞

e−(x+42i)2dx = 2 π

horrific sign problem

  • 4
  • 2

2 4 10 20 30 40 50

z

  • 4
  • 2

2 4

  • 3×10191
  • 2×10191
  • 1×10191

1×10191 2×10191 3×10191

24

slide-25
SLIDE 25

A complex way around sign problem

horrific sign problem better

  • 4
  • 2

2 4 10 20 30 40 50

z

  • 4
  • 2

2 4

  • 3×10191
  • 2×10191
  • 1×10191

1×10191 2×10191 3×10191

  • 4
  • 2

2 4

  • 4×1015
  • 2×1015

2×1015 4×1015

25

∫𝒟 e−(z+42i)2dz = 2 π

slide-26
SLIDE 26
  • 4
  • 2

2 4 10 20 30 40 50

z

  • 4
  • 2

2 4

  • 4
  • 2

2 4 6 8 10

  • 4
  • 2

2 4

  • 3×10191
  • 2×10191
  • 1×10191

1×10191 2×10191 3×10191

  • 4
  • 2

2 4

  • 4×1015
  • 2×1015

2×1015 4×1015

A complex way around the sign problem

∫𝒟 e−(z+42i)2dz = 2 π

horrific sign problem better much better

26

slide-27
SLIDE 27

The main idea: deform the QFT path integral domain to a better one in complex field space where the sign problem is mild.

Review article : ”Complex paths around the sign problem” [Alexandru, GB, Bedaque, Warrington] coming soon… [also work by Cristoforetti, Di Renzo et al, Fujii et al., Tanizaki et al.,… ] Mathematical origins: Picard-Lefschetz theory [Pham, Fedoryuk, Witten, ….]

27

slide-28
SLIDE 28

Good deformations

:

N

.

t

:

#

.

.

complex field space

  • riginal domain

deformed domain

  • path integral on ℳ = path integral on
  • sign problem on ℳ << sign problem on

ℝN ℝN

(“allowed”) (“good”)

28

slide-29
SLIDE 29

Good deformations

:

N

.

t

:

#

.

.

ϕ(0) ϕ(Tflow)

  • path integral on ℳ = path integral on
  • sign problem on ℳ << sign problem on

ℝN ℝN

(“allowed”) (“good”)

dϕ(τ) dτ = ∂S[ϕ] ∂ϕ follow an equation of motion, ``holomorphic gradient flow”

29

slide-30
SLIDE 30

Strategy

deformation discretization importance sampling

30

Dynamics Finite density

slide-31
SLIDE 31

Real time dynamics

⟨𝒫(t)𝒫(0)⟩ = 1 Z ∫ [dϕ]e

i ℏ S[ϕ]𝒫(t)𝒫(0)

e

i ℏ S[ϕ] leads to quantum interference

…and the ultimate sign problem ⟨e−iSI[ϕ]⟩SR = 0 transport (viscosity, conductivity),

  • ut-of equilibrium physics…

31

slide-32
SLIDE 32

Real time dynamics - 1+1d QFT

interacting Bose gas:

ℒ = 1 2(∂ϕ)2 − 1 2 m2ϕ2 − λ 4! ϕ4

free theory 𝝁=0

  • Re[C]
  • Im[C]
  • free theory

0.0 0.5 1.0 1.5 2.0

  • 4
  • 2

2 4 t Cp=0(t)

  • Re[C]
  • Im[C]
  • 0.0

0.5 1.0 1.5 2.0

  • 4
  • 2

2 4 t Cp=2 πL(t)

Cp(t) = ⟨ϕ(t, p)ϕ(0,p)⟩β

[Alexandru, GB, Bedaque, Ridgway, Vartak, Warrington, PRL 117081602, PRD 95 114501]

32

slide-33
SLIDE 33

Real time dynamics - 1+1d QFT

interacting Bose gas:

ℒ = 1 2(∂ϕ)2 − 1 2 m2ϕ2 − λ 4! ϕ4

weak coupling 𝝁=0.1

  • Re[C]
  • Im[C]
  • 1st order perturbation

free theory

0.0 0.5 1.0 1.5 2.0

  • 4
  • 2

2 4 t Cp=0(t)

  • Re[C]
  • Im[C]
  • 0.0

0.5 1.0 1.5 2.0

  • 4
  • 2

2 4 t Cp=2 πL(t)

Cp(t) = ⟨ϕ(t, p)ϕ(0,p)⟩β

[Alexandru, GB, Bedaque, Ridgway, Vartak, Warrington, PRL 117081602, PRD 95 114501]

33

slide-34
SLIDE 34
  • Re[C]
  • Im[C]
  • exact

1st order perturbation free theory

0.0 0.5 1.0 1.5 2.0

  • 4
  • 2

2 4 t Cp=0(t)

Real time dynamics - 1+1d QFT

interacting Bose gas:

ℒ = 1 2(∂ϕ)2 − 1 2 m2ϕ2 − λ 4! ϕ4

weak coupling 𝝁=0.1

  • Re[C]
  • Im[C]
  • 0.0

0.5 1.0 1.5 2.0

  • 4
  • 2

2 4 t Cp=2 πL(t)

Cp(t) = ⟨ϕ(t, p)ϕ(0,p)⟩β

[Alexandru, GB, Bedaque, Ridgway, Vartak, Warrington, PRL 117081602, PRD 95 114501]

34

slide-35
SLIDE 35
  • Re[C]
  • Im[C]
  • 0.0

0.5 1.0 1.5

  • 0.3
  • 0.2
  • 0.1

0.0 0.1 0.2 0.3 t Cp=2 πL(t)

  • Re[C]
  • Im[C]
  • free theory

0.0 0.5 1.0 1.5

  • 4
  • 2

2 4 t Cp=0(t)

Real time dynamics - 1+1d QFT

interacting Bose gas:

ℒ = 1 2(∂ϕ)2 − 1 2 m2ϕ2 − λ 4! ϕ4

strong coupling 𝝁=1 Cp(t) = ⟨ϕ(t, p)ϕ(0,p)⟩β

[Alexandru, GB, Bedaque, Ridgway, Vartak, Warrington, PRL 117081602, PRD 95 114501]

35

slide-36
SLIDE 36
  • Re[C]
  • Im[C]
  • 0.0

0.5 1.0 1.5

  • 0.3
  • 0.2
  • 0.1

0.0 0.1 0.2 0.3 t Cp=2 πL(t)

  • Re[C]
  • Im[C]
  • 1st order perturbation

free theory

0.0 0.5 1.0 1.5

  • 4
  • 2

2 4 t Cp=0(t)

Real time dynamics - 1+1d QFT

interacting Bose gas:

ℒ = 1 2(∂ϕ)2 − 1 2 m2ϕ2 − λ 4! ϕ4

strong coupling 𝝁=1 Cp(t) = ⟨ϕ(t, p)ϕ(0,p)⟩β

[Alexandru, GB, Bedaque, Ridgway, Vartak, Warrington, PRL 117081602, PRD 95 114501]

36

slide-37
SLIDE 37
  • Re[C]
  • Im[C]
  • 0.0

0.5 1.0 1.5

  • 0.3
  • 0.2
  • 0.1

0.0 0.1 0.2 0.3 t Cp=2 πL(t)

  • Re[C]
  • Im[C]
  • exact

1st order perturbation free theory

0.0 0.5 1.0 1.5

  • 4
  • 2

2 4 t Cp=0(t)

Real time dynamics - 1+1d QFT

interacting Bose gas:

ℒ = 1 2(∂ϕ)2 − 1 2 m2ϕ2 − λ 4! ϕ4

strong coupling 𝝁=1 Cp(t) = ⟨ϕ(t, p)ϕ(0,p)⟩β

[Alexandru, GB, Bedaque, Ridgway, Vartak, Warrington, PRL 117081602, PRD 95 114501]

37

[see also follow-up by Mou, Saffin, Tranberg, ‘18]

slide-38
SLIDE 38

Real time dynamics -Hybrid Monte Carlo

Case Study : 0+1 d anharmonic oscillator

ℒ = 1 2 · ϕ2 − 1 2 m2ϕ2 − λ 4! ϕ4

in progress

38

p z z’ x x’

[also (finite density) Fujii, Honda, Kato, Kikukawa, Komatsu, Sano, JHEP 10 (2013) 147 01]

slide-39
SLIDE 39

Real time dynamics -Hybrid Monte Carlo

Case Study : 0+1 d anharmonic oscillator

ℒ = 1 2 · ϕ2 − 1 2 m2ϕ2 − λ 4! ϕ4

in progress

39

δRe<T x(t)x(0)>

1 2 3 4

  • 0.04
  • 0.02

0.00 0.02 0.04 t

  • Re<T x(t)x(0)>
  • Im<T x(t)x(0)>
  • ● ●
  • ● ● ● ● ●
  • ● ● ● ● ● ● ● ● ● ● ● ●
  • ● ● ● ● ● ● ● ● ● ● ● ● ● ● ● ● ● ● ● ● ● ● ● ●

1 2 3 4

  • 1.0
  • 0.5

0.0 0.5 1.0 t

PRELIMINARY

Nt = 24, Nβ = 4, λ = 24

slide-40
SLIDE 40

Many body physics - 2d Thirring model

g2

chain of interacting fermions S = ∫ d2x ¯ ψa (γμ∂μ + m + μγ0) ψa + g2 2Nf (ψaγμψa)(ψbγμψb) → Nf 2g2 ∫ d2xAμAμ + tr log(∂ + A + μγ0 + m) / /

  • a prototype of QCD
  • a 2d cousin of the Hubbard model

asymptotically free, sign problem at finite density [Alexandru, GB, Bedaque, Ridgway, Warrington, Phys. Rev. D95, 014502 ]

40

slide-41
SLIDE 41

Many body physics - 2d Thirring model

ℝN

1 2 3 4 0.0 0.2 0.4 0.6 0.8 1.0 μ/mf Re〈e-ⅈ SI〉

ℝN

1 2 3 4 0.0 0.2 0.4 0.6 0.8 1.0 1.2 1.4 μ/mf 〈n〉/mf

sign problem equation of state

[Alexandru, GB, Bedaque, Ridgway, Warrington, Phys. Rev. D95, 014502 ]

41

slide-42
SLIDE 42

Many body physics - 2d Thirring model

ℝN Tflow=0

1 2 3 4 0.0 0.2 0.4 0.6 0.8 1.0 1.2 1.4 μ/mf 〈n〉/mf

ℝN Tflow=0

1 2 3 4 0.0 0.2 0.4 0.6 0.8 1.0 μ/mf Re〈e-ⅈSI〉

sign problem equation of state

[Alexandru, GB, Bedaque, Ridgway, Warrington, Phys. Rev. D95, 014502 ]

42

slide-43
SLIDE 43

Many body physics - 2d Thirring model

ℝN Tflow=0 Tflow=0.4

1 2 3 4 0.0 0.2 0.4 0.6 0.8 1.0 1.2 1.4 μ/mf 〈n〉/mf

ℝN Tflow=0 Tflow=0.4

1 2 3 4 0.0 0.2 0.4 0.6 0.8 1.0 μ/mf Re〈e-ⅈSI〉

sign problem equation of state

[Alexandru, GB, Bedaque, Ridgway, Warrington, Phys. Rev. D95, 014502 ]

43

slide-44
SLIDE 44

Many body physics - 2d Thirring model

Equation of state: low temperature limit

T/mf0.38 T/mf0.19 T/mf0.13 T/mf0.09

0.0 0.5 1.0 1.5 2.0 0.0 0.2 0.4 0.6 0.8 /mf n/mf

particularly bad sign problem: ⟨e−iSI[ϕ]⟩SR ∝ e−volume/T

[Alexandru, GB, Bedaque, Ridgway, Warrington, Phys. Rev. D95, 014502 ]

44

slide-45
SLIDE 45

Many body physics - 2d Thirring model

Nt×Nx=10×10 Nt×Nx=10×20

1 2 3 4 0.0 0.5 1.0 1.5 μ/mf 〈n〉/mf

Nt×Nx=12×12 Nt×Nx=16×16 Nt×Nx=20×20

0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 0.0 0.5 1.0 1.5 2.0 μ/mf 〈n〉/mf

continuum limit thermodynamic limit

Equation of state

[Alexandru, GB, Bedaque, Ridgway, Warrington, Phys. Rev. D95, 014502 ]

45

slide-46
SLIDE 46

Gauge theories - 2d QED

baryon 2

  • 1
  • 1

QED with 3 ``quarks” with charges q=2,-1,-1 S =

3

a=1 ∫ d2x [F2 + ¯

ψ a (γμ(∂μ − gqaAμ) + m − μγ0) ψ a ]

0.2 0.4 0.6 0.8 1 1 2 3 4 5 hσi µB/mB RN

10

MT=0.01 MT=0.02 MT=0.05 0.2 0.4 0.6 0.8 1 1 2 3 4 5 hni µB/mB RN

10

MT=0.01 MT=0.02 MT=0.05

sign problem equation of state

46

slide-47
SLIDE 47

Gauge theories - heavy dense QCD

[Zambello, Di Renzo, Phys. Rev. D95, 014502 ] n: density L: Polyakov loop

  • In the limit

mq → ∞ effective theory of Polyakov loops

  • Still has a sign problem for but easier to simulate

μ ≠ 0

  • Exploratory study on a few-site lattice with

ℳ ~ ∑ ``Lefschetz thimbles” (fixed points of flow+fluctuations)

47

slide-48
SLIDE 48

Many body physics - Hubbard model

[Ulybyshev, Winterowd, Zafeiropoulos PRD 101 (1), 014508]

48

2d Hubbard model away from half filling on a Honeycomb lattice

hcos ImSi hcos arg Ji hΣGi BSS-QMC 0.2363±0.0032 0.2363±0.0032 HMC,α=1.0 0.9627±0.0038 0.427±0.014 0.351±0.015 HMC,α=0.8 0.797±0.022 0.915±0.008 0.644±0.028

average sign conventional MC deformation ~ ∑ “thimbles”

(1a)

fixed point of flow = saddle point of S[𝜚]

slide-49
SLIDE 49

Other deformations: “Learnifolds”

[Alexandru, Bedaque, Lamm, Lawrence Phys.Rev.D 96 (2017) 9, 094505] ϕ Im ˜ ϕ

:

N

.

t

:

#

.

.

ϕ ˜ ϕ

Machine learning, training set: points on ℳ

49

  • utput: ℒ ≈ℳ
slide-50
SLIDE 50

Sign optimized manifolds

[Mori et al. ’17-’19, Alexandru et al. ‘18, Bursa et al. ’18, Kashiwa et al. ‘19, Detmold et al. ‘20]

⟨e−iSI⟩λ = ∫ℳλ d[ϕ]e−S ∫ℳλ d[ϕ]e−SR maximize the average phase: within a family of manifolds minimize the sign problem ℳλ

:

N

.

t

:

#

.

.

ℳλ

50

slide-51
SLIDE 51 temperature 1012 K chemical potential ∼310 MeV heavy ion coll. early universe quark gluon plasma hadron gas you are here neutron stars

??

critical point

flow QFT: real time dynamics, finite density

  • ther deformations, ansatzë

simulated annealing

φ0 φ0 φ1 φ0

1

φn−1 φ0

n1

φn ... ... accept/reject

Metropolis step w/ p1 Metropolis step w/ pn Metropolis step w/ pn Metropolis step w/ p1

Hybrid Monte Carlo pseudo-fermions, estimators machine learning, path optimization

51