in Bose systems - Isaac Newton Institute€¦ ·  · 2014-05-31Lecture Notes: arXiv:1302.1448...

35
Non-Thermal Fixed Points – Universality, topology & turbulence in Bose systems Thomas Gasenzer Thomas Gasenzer Institut für Theoretische Physik Institut für Theoretische Physik Ruprecht-Karls Universität Heidelberg Ruprecht-Karls Universität Heidelberg Philosophenweg 16 • 69120 Heidelberg • Germany Philosophenweg 16 • 69120 Heidelberg • Germany ExtreMe Matter Institute EMMI ExtreMe Matter Institute EMMI GSI Helmholtzzentrum für Schwerionenforschung GmbH GSI Helmholtzzentrum für Schwerionenforschung GmbH

Transcript of in Bose systems - Isaac Newton Institute€¦ ·  · 2014-05-31Lecture Notes: arXiv:1302.1448...

Non-Thermal Fixed Points –Universality, topology & turbulence

in Bose systems

Thomas GasenzerThomas Gasenzer

Institut für Theoretische PhysikInstitut für Theoretische PhysikRuprecht-Karls Universität HeidelbergRuprecht-Karls Universität Heidelberg

Philosophenweg 16 • 69120 Heidelberg • GermanyPhilosophenweg 16 • 69120 Heidelberg • Germany

ExtreMe Matter Institute EMMIExtreMe Matter Institute EMMIGSI Helmholtzzentrum für Schwerionenforschung GmbHGSI Helmholtzzentrum für Schwerionenforschung GmbH

Lecture Notes:arXiv:1302.1448 [cond-mat.quant-gas]

Non-Thermal Fixed Points –Universality, topology & turbulence

in Bose systems

Thomas GasenzerThomas Gasenzer

Institut für Theoretische PhysikInstitut für Theoretische PhysikRuprecht-Karls Universität HeidelbergRuprecht-Karls Universität Heidelberg

Philosophenweg 16 • 69120 Heidelberg • GermanyPhilosophenweg 16 • 69120 Heidelberg • Germany

ExtreMe Matter Institute EMMIExtreMe Matter Institute EMMIGSI Helmholtzzentrum für Schwerionenforschung GmbHGSI Helmholtzzentrum für Schwerionenforschung GmbH

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Thanks & credits

collaboration with:

… & my former students:Boris Nowak, Jan Schole ( Heidelberg), Maximilian Schmidt ( Jülich), Christian Scheppach ( Cambridge, UK) (all involved in work presented here),

as well as

Cédric Bodet, Alexander Branschädel ( KIT), Roman Hennig, Nikolai Philipp, Stefan Keßler ( Erlangen), Matthias Kronenwett, Philipp Struck ( Konstanz), Kristan Temme ( Vienna), Martin Trappe ( Singapore), Pascal Weckesser, Jan Zill ( Queensland)

LGFG BaWue

€€€...

Groups of Markus Oberthaler, Jörg Schmiedmayer,Jürgen Berges, Sebastian Diehl, Jan Pawlowski

Linda Martini Steven Mathey Sebastian Erne Sebastian Bock Markus Karl Thorge Müller Sebastian Heupts Bart Andrews Isara Chantesana Alexander Liluashvili

(not on picture: Martin Gärttner, Denes Sexty)

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Transient stationaritye.g. Turbulence

Time flies

Initial state:Far from equilibrium

Final state:Thermal equilibrium

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Transient stationaritye.g. Turbulence

Prethermalisation

Time flies

Initial state:Far from equilibrium

Final state:Thermal equilibrium

(partially) universal dynamicspre-thermalisation

[Berges, Borsanyi, Wetterich (2004), Moeckel, Kehrein (2008), and many more now ]

[Ske

tch

by C

. W

ette

rich

]

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Transient stationaritye.g. Turbulence

Prethermalisation

Universal dynamics

Initial state:Far from equilibrium

Final state:Thermal equilibrium

Non-thermal fixed point

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Classical Turbulence

“Big whirls have little whirls that feed on their velocity, and little whirls have lesser whirls and so on to viscosity.”

(Richardson, 1920)

Lewis F. Richardson(1881-1953)Richardson cascade

large scales (source) → small scales (sink)

Leonardo da Vinci (1452-1519)

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Kolmogorov41 Turbulence CascadeTransport of kinetic energy E:

log E(k)

log k

pump

dump

Leonardo da Vinci (1452-1519)

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Kolmogorov41 Turbulence CascadeStationary scaling E(k) within inertial region:

log E(k)

log k

Incompressible fluid:

E(k) ~ k—5/3

pump

dumpcascade

Uriel Frisch, Turbulence. The Legacy of A. N. Kolmogorov. (CUP, 1995)

Cascade

Leonardo da Vinci (1452-1519)

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Semi-classical Simulations (c-field methods, TWA)

Done on GPUs& Multicore Cl.

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

2D Bose gas: Quench dynamicsB. Nowak, D. Sexty, TG, PRB 84(R) (11); B. Nowak, J. Schole, D. Sexty, TG, PRA 85 (12)

“Initial” distribution

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

2D Bose gas: Quench dynamicsB. Nowak, D. Sexty, TG, PRB 84(R) (11); B. Nowak, J. Schole, D. Sexty, TG, PRA 85 (12)

thermal

~T/k2

(Rayleigh-Jeans regime of BE distribution)

1e/T−1

≈ T

“Final” distribution

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

2D Bose gas: Quench dynamicsB. Nowak, D. Sexty, TG, PRB 84(R) (11); B. Nowak, J. Schole, D. Sexty, TG, PRA 85 (12)

⇒ bidirectional redistribution

1e/T−1

≈ T

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

2D Bose gas: Quench dynamicsB. Nowak, D. Sexty, TG, PRB 84(R) (11); B. Nowak, J. Schole, D. Sexty, TG, PRA 85 (12)

thermal

~T/k2

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Superfluid hydro of Bose-condensed Gas

The Gross-Pitaevskii Equation, (g = 4πa0/m)

using the defs.

can be written as

Continuity equation Euler equation

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

2D Bose gas: Quench dynamicsB. Nowak, D. Sexty, TG, PRB 84(R) (11); B. Nowak, J. Schole, D. Sexty, TG, PRA 85 (12)

( + zero-mode )

Phase angle

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

2D Bose gas: Quench dynamicsB. Nowak, D. Sexty, TG, PRB 84(R) (11); B. Nowak, J. Schole, D. Sexty, TG, PRA 85 (12)

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

2D Bose gas: Quench dynamicsB. Nowak, D. Sexty, TG, PRB 84(R) (11); B. Nowak, J. Schole, D. Sexty, TG, PRA 85 (12)

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Non-Thermal Fixed Point

Particles

Energy

B. Nowak, D. Sexty, TG, PRB 84(R) (11); B. Nowak, J. Schole, D. Sexty, TG, PRA 85 (12)

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Wave Turbulence – e.g. on water [H. Xia et al., EPL 91 (10) 14002]

[Zakharov & Filonenko (67)]

(kinetic) WT Theory prediction:

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Non-Thermal Fixed Point

Particles

Energy J. Berges, A. Rothkopf, J. Schmidt, PRL 101 (08) 041603, J. Berges, G. Hoffmeister, NPB 813 (09) 383,C. Scheppach, J. Berges, TG PRA 81 (10) 033611

Wave turbulence: Power laws from kinetic eqs.

B. Nowak, D. Sexty, TG, PRB 84(R) (11); B. Nowak, J. Schole, D. Sexty, TG, PRA 85 (12)

= 0

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Non-Thermal Fixed Point

Particles

Energy J. Berges, A. Rothkopf, J. Schmidt, PRL 101 (08) 041603, J. Berges, G. Hoffmeister, NPB 813 (09) 383,C. Scheppach, J. Berges, TG PRA 81 (10) 033611

nIR ~ k −d −2

IR power laws from (2PI 1/N & fRG) field theory:

B. Nowak, D. Sexty, TG, PRB 84(R) (11); B. Nowak, J. Schole, D. Sexty, TG, PRA 85 (12)

= 0

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Transient stationaritye.g. Turbulence

Prethermalisation

Non-thermal fixed point

Initial state:Far from equilibrium

Final state:Thermal equilibrium

Non-thermal fixed point

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Approach of the NTFP

J. Schole, B. Nowak, TG, PRA 86 (12) 013624

mor

e ph

ase

cohe

renc

e

larger Vortex-Antivortex distances

lC

* = Phase coherence lengthlD*

= Vortex-Antivortex pair distance

time

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Approach of the NTFP

J. Schole, B. Nowak, TG, PRA 86 (12) 013624

mor

e ph

ase

cohe

renc

e

larger Vortex-Antivortex distances

logtime steps

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Approach of the NTFP

J. Schole, B. Nowak, TG, PRA 86 (12) 013624

mor

e ph

ase

cohe

renc

e

larger Vortex-Antivortex distances

dilu

tion

, un

bind

ing

pair binding

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Non-Thermal Fixed Point in 3DB. Nowak, J. Schole, TG, arXiv:1206.3181v2 [cond-mat.quant-gas]

lD ~ vortex ring radius,

lC ~ phase coherence length

Dilution process: cf. also Kelvin-wave cascade Kozik & Svistunov (03-11)

k‒ 2.5

k‒ 10

initial spectrum

log k

log

n(k

)

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Many other phenomena

Non-Thermal Fixed Points

Vortex Dynamics in 2&3D

1D Soliton Gas

Charge confinement in Higgs models

“Kibble-Zurek”, Exciton-Polaritons, Cosmology, QGP, ...

Pattern formation in Spinor gases

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

The End

Supplementary slides

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Kolmogorov scaling of Qu. Turbulence(Simulations of Gross-Pitaevskii Equation)

Figure from:

M. Kobayashi & M. Tsubota,J. Phys. Soc. Jpn (2005).M. Tsubota, arXiv:1004.5458 [cond-mat].

Extensive work on Qu. Turbulence (mainly beyond sf. Helium):

Vinen 1950's-; & Donnelly, 2002, 07.Svistunov, Berloff, Kozik, … 1995-.Nore, Abid, Brachet, 1995-. Krstulovic,Gurarie 1995.Maurer & Tabeling, 1999Tsubota 2000-.Parker & Adams, 2005L'vov, Nazarenko, Budenko, 2007...Horng, Gou, et al., 2008-Bagnato et al., 2009-Anderson, Bradley, Davis, Neely, … 2010-…

not to mention ≈∞ work on classical Turbulence

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

2-component Bose gas

~ g

~ g12

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

M. Karl, B. Nowak, TG, Sci. Rep. 3, 2394 (2013); & new paper: arXiv:1307.7368 [cond-mat.quant-gas]

Build-up of IR scaling

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Gauge Turbulence

TG, L. McLerran, J.M. Pawlowski, D. Sexty, 1307.5301 [hep-ph]

U(1) Higgs model:

Electricchargedistribution

Gauge invariantHiggs phase

Holography: From Gravity to Quantum Matter · Isaac Newton Institute · Cambridge · 18 Sep 2013 Thomas Gasenzer

Gauge Turbulence

TG, L. McLerran, J.M. Pawlowski, D. Sexty, 1307.5301 [hep-ph]

Suppression of Higgs condensationfor strong gauge coupling (type I superconductor)

Electricchargedistribution

Gauge invariantHiggs phase

cond

ensa

te

time