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Polaritons in some interacting exciton systems Peter Littlewood, - PowerPoint PPT Presentation

Polaritons in some interacting exciton systems Peter Littlewood, Argonne and U Chicago Richard Brierley (Yale) Cele Creatore (Cambridge) Paul Eastham (Trinity College, Dublin) Francesca Marchetti (Madrid) Marzena Szymanska (UCL) Jonathan


  1. Polaritons in some interacting exciton systems Peter Littlewood, Argonne and U Chicago Richard Brierley (Yale) Cele Creatore (Cambridge) Paul Eastham (Trinity College, Dublin) Francesca Marchetti (Madrid) Marzena Szymanska (UCL) Jonathan Keeling and Justyna Cwik (St Andrews) Sahinur Reja (Dresden) Alex Edelman (Chicago)

  2. Outline  Brief review of a microscopic model for polariton condensation and quasi-equilibrium theory  Quantum dynamics out of equilibrium – pumped dynamics beyond mean field theory and dynamical instabilities – use of chirped pump pulses to generate non-equilibrium populations, possibly with entanglement  Polariton systems with strong electron-phonon coupling – e.g. organic microcavities – Can you condense into phonon polariton states?  Cavity – coupled Rydberg atoms – Competition between superfluid and quantum crystal 8/27/2015 5

  3. Polaritons: Matter-Light Composite Bosons [C. Weisbuch et al., PRL 69 3314 (1992)] photon in-plane ph momentum energy UP photon mirror QW mirror QW exciton LP Effective Mass m * ~ 10 -4 m e T BEC ~ 1/m * momentum 8/27/2015 6

  4. Bogoliubov spectrum Vortices BEC Kasprzak et al 2006 Utsunomiya et al,2008 Coupled condensates Lagoudakis et al 2008 Power law correlations Tosi et al 2012 Superflow Roumpos et al 2012 8/27/2015 7 Amo et al, 2011

  5. Polaritons and the Dicke Model – a.k.a Jaynes-Tavis-Cummings model Excitons as “spins” Double Empty Single Spins are flipped by absorption/emission of photon N ~ [(photon wavelength)/(exciton radius)] d >> 1 Mean field theory – i.e. BCS coherent state – expected to be good approximation Transition temperature depends on coupling constant 8/27/2015 10

  6. Mean field theory of Condensation Eastham & PBL, Increasing excitation density PRB 64, 235101 (2001) No inhomogeneous broadening Zero detuning Δ = ω – ε = 0 Upper polariton Excitation energies (condensed state) Coherent light Lower polariton Chemical potential (condensed state) Chemical potential (normal state) 8/27/2015 11

  7. Phase diagram with detuning: appearance of “Mott lobe” Solid State Commun, 116, 357 (2000); PRB 64, 235101 (2001) Detuning D = ( w - e )/ g T=0 D = 3 D = 1 Photon occupation Inverse temperature D = 0 Exciton occupation 8/27/2015 12

  8. Single Mott Lobe for s=1/2 state Photon condensate Δ = 2 Δ =3 μ Superradiant Mott Ins. Phase Δ =1 Polariton condensate Δ =0 negative detuning Eastham and Littlewood, Solid State Communications 116 (2000) 357--361 8/27/2015 13

  9. 2D polariton spectrum Keeling et al PRL 93, 226403 (2004) • Below critical temperature polariton dispersion is linear – Bogoliubov sound mode appears • Include disorder as inhomogeneous broadening Energy Momentum 8/27/2015 14

  10. Beyond mean field: Interaction driven or dilute gas? • Conventional “BEC of polaritons” will give high transition temperature Upper polariton because of light mass m * • Single mode Dicke model gives g transition temperature ~ g Lower polariton Which is correct? BEC k // Mean kT c a o = characteristic field separation of excitons a o > Bohr radius 0.1 g Dilute gas BEC only for 2 na 0 excitation levels < 10 9 cm -2 or so A further crossover to the plasma regime when 2 ~ 1 na B 8/27/2015 18

  11. Condensation in polaritons with strong electron- phonon coupling Justina Cwik, Jonathan Keeling (St Andrews); Sahinur Reja (Cambridge-> Dresden) Europhysics Letters 105 (2014) 47009 8/27/2015 Telluride2011 48

  12. Cwik, Reja, Keeling, PBL “ Dicke- Holstein” model EPL 105 (2014) 47009 Exciton-polariton (as before) + coupling to local phonon mode Mimics coupling of Frenkel exciton to optical phonon Cavity Exciton Rabi coupling Phonon Local (Holstein) coupling With strong exciton-phonon coupling, exciton develops sidebands Can you have condensation into a phonon replica? Method: mean field for photons; numerical diagonalization of phonon 8/27/2015 49

  13. Phase diagram – critical detuning Re- entrant ‘Mott lobes’ N=0 N=1 8/27/2015 50

  14. Super-radiant phase stabilized by raising temperature 8/27/2015 51

  15. Vibrational replicas • Paradox? Infinite number of vibrational replicas at energies ε -n Ω – some of which must be therefore below the chemical potential. • Resolution: Photon spectral weight vanishes at most level crossings 8/27/2015 52

  16. Interacting excitons – Rydberg atoms in optical cavities Alex Edelman (Chicago) 8/27/2015 54

  17. Ingredients Ingredients: Coupled 2-level systems Nearly Resonant Cavity photons …and interacting …on a lattice – Why a lattice? Blockade Effect: • As an emergent lattice structure • As a dilute limit Löw, J Phys B (2012)

  18. A detour: Cu 2 O Kazimierczuk, T., Fröhlich, D., Scheel, S., Stolz, H. & Bayer, M. Giant Rydberg excitons in the copper oxide Cu2O. Nature 514, 343 – 347 (2014).

  19. Rydberg polaritons Represent exciton as two fermionic levels with a constraint of single occupancy Here, simplify as 2D lattice model with (a) nearest neighbour interactions, (b) generalised long range interactions Consider instability of the superradiant polariton state. No weak coupling instability if U(q) > 0 In strong coupling expect an effective interaction that generates a (short) length scale from the density itself. Mixing of amplitude and phase modes only allowed at non-zero momentum. See also Zhang et al PRL 110, 090402 (2013) 8/27/2015 58

  20. Model and Method Photons Density waves Excitons (as fermions ) Photons Fluctuations : Mean Field:

  21. Phase Diagram: U = 0 g Τ condensed normal ρ μ

  22. Phase Diagram: Finite U (mean field) g g condensed normal μ μ Trivial effect – occupancy + interactions shifts excitons closer to resonance with photon

  23. Mean Field Excitation Spectrum (U=0) Normal State ω = k Condensed State ω ω Δ = 0 Δ = 3 k k

  24. Excitation Spectrum – With Interactions Normal State ω Completely unmodified! • Low-density limit • Dispersionless excitons (spins) k Condensed State ω U = 0 An instability develops at q= π (in units of the lattice) U = U crit k

  25. Diagnosing the Instability g condensate |U|=|U crit | instability line ??? Coupling normal Condensate Amplitude Photon Dispersion Exciton energy normal Mean-field phase boundary μ

  26. Diagnosing the Instability m*=10 Infinite-bandwidth limit: m*=.01 Compare: Fermions Bosons

  27. Staggered Mean Field Spins (as fermions) Photons Photons Density waves g condensed (homogeneous) First-order transition Coexistence of normal normal condensate and normal ordered phase “ supersolid ” μ

  28. Staggered Stability Analysis “First - order” ω line condensed “ supersolid" k Staggered state instability line normal normal normal

  29. Variational Monte Carlo Data Confirm | ψ 0 | 2 φ 0 φ π g μ 0 1 -1 1 0 1 Coexistence

  30. Long-range interactions U |i-j| = U δ <ij> U 0 /|i-j| α ( α =6 for van der Waals forces in Rydberg atoms) = U 0 (n.n.) +U 0 /2 (n.n.n .) +… g = 0 ground state: Complete Devil’s Staircase (Bak and Bruinsma 1982)

  31. Long-range interactions g > 0: half- filling story repeats “self - similarly” at other fillings | ψ 0 | 2 <S> g g μ μ 0 1 1/2 -1/2

  32. ‘ Supersolid ’ phase? • Possibility of phase with both superfluid and charge order • Has three acoustic modes (two sound and Bogoliubov) • Has two amplitude modes (upper polariton and CDW amplitude mode) • Amplitude modes mix; sound modes do not (not a gauge theory) • Cold atom version of NbSe 2 ? • Does this phase continue to be present without the lattice ? 8/27/2015 76

  33. Acknowledgements Paul Eastham (Trinity College Dublin) Jonathan Keeling (St Andrews) Francesca Marchetti (Madrid) Marzena Szymanska (UCL) Richard Brierley (Cambridge/Yale) Sahinur Reja (Dresden) Cavendish Laboratory University of Cambridge Alex Edelman (Chicago) Cele Creatore (Cambridge) Collaborators: Richard Phillips, Jacek Kasprzak, Le Si Dang, Alexei Ivanov, Leonid Levitov, Richard Needs, Ben Simons, Sasha Balatsky, Yogesh Joglekar, Jeremy Baumberg, Leonid Butov, David Snoke, Benoit Deveaud, Georgios Roumpos, Yoshi Yamamoto 8/27/2015 78

  34. The Seven Ages of Physicists In As You Like It Shakespeare outlined the seven ages of man From the infant, to the schoolboy, the lover, the soldier and then ....

  35. The Fifth Age “And then the Justice, In fair round belly with good capon lined, With eyes severe, and beard of formal cut, Full of wise saws and modern instances”

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