Atom-Photon Interactions: Methods and Results

presented by gilad laredo n.w
1 / 18
Embed
Share

Dive into the world of atom-photon interactions with Gilad Laredo's presentation from Spring 2017. Explore the transition probabilities, time-independent Hamiltonians, and the Floquet theorem. Learn how to solve complex equations and generalize problems in this fascinating field of study.

  • Atom-photon
  • Interaction
  • Transition probability
  • Hamiltonian
  • Floquet theorem

Uploaded on | 0 Views


Download Presentation

Please find below an Image/Link to download the presentation.

The content on the website is provided AS IS for your information and personal use only. It may not be sold, licensed, or shared on other websites without obtaining consent from the author. If you encounter any issues during the download, it is possible that the publisher has removed the file from their server.

You are allowed to download the files provided on this website for personal or commercial use, subject to the condition that they are used lawfully. All files are the property of their respective owners.

The content on the website is provided AS IS for your information and personal use only. It may not be sold, licensed, or shared on other websites without obtaining consent from the author.

E N D

Presentation Transcript


  1. Presented by Gilad Laredo Atom-photons interactions 118137 Spring 2017

  2. 2?cos?? Introduction ,E ,E System evolves according to Schr dinger eq. ( ) ( ) t ( ) ( ) t 2 cos b E t a a t a a t d dt = i 2 cos b t E ( ) t 2 transition probability to be in at time ' ' a t ( ) 1 =

  3. But how do we solve this? ( ) ( ) t ( ) ( ) t 2 cos b E t a a t a a t d dt = i Difficult 2 cos b t E ? i t i t i t = + 2cos t e e e By the RWA: ( ) ( ) t ( ) ( ) t i t a a t a a t E be d dt = i Easy i t be E ( ) 1 = RWA = rotating wave approximation

  4. Paper goal Present methods and results obtained while solving the transition probability for: ( ) ( ) t ( ) ( ) t 2 cos b E t a a t a a t d dt = i 2 cos b t E Without the rotating wave approximation time independent Hamiltonian Infinite matrix representation Floquet theorem Time periodic Hamiltonian

  5. time independent Hamiltonian Infinite matrix representation Floquet theorem Time periodic Hamiltonian ( ) ( ) t ( ) ( ) ( ) t ) Generalize the problem: H t T 2 cos b ; E t a a F t t a a + t d dt i = i d dt 2 cos b ( ) ( ) t F t c ( ( ) t = = H H t E Q c c : Constant diagonal matrix ( ) ( ) t e Generalize the problem: Step 1 determine general form of solution (Floquet): = iQt F t d dt ( ) ( ( ) ( ) t F t ( ) ( ) t ( ) t = t T + = H H H ; i F t H : Matrix c c c Step 2 equivalence to (infinite) eigenvalue problem. of periodic functions ) ( ) , ( ) , n k k n + = ( ) n F q F , , kn , k ( ) ( ) ( ) 0 t Step 3 express time-evolution operator: = = 1 2 T ( ; ) U t t F t F 0

  6. 's q Eigenvalue equation for Floquet Hamiltonian ( ) H ( ) , ( ) , n k k n + = ( ) n F q F , , kn , k = ( ) t in t ( ) n H H e c , , ( ) n ( ) ( ) = in t iq t ( ) , n exp exp F t F , n Greek letters atomic states Roman letters Fourier components ( ) ( ) t e = iQt F t d dt ( ) ( ) ( ) t F t = Hc i F t

  7. ( ) H ( ) , ( ) , - - Floquet Floquet Hamiltonian Hamiltonian H n k k n + = ( ) n F q F F , , kn , k ,E ( ) ( ) t ( ) ( ) t 2 cos b E t a a t a a t An example d dt = i 2 cos b t E ,E 2 0 0 0 0 b 0 b 0 0 0 0 b + 0 0 0 b 0 0 0 0 0 0 b + E b b E 0 0 0 0 0 0 0 0 b 0 0 E b E H F 0 0 0 0 0 0 b 0 0 + E b 0 0 0 E 0 0 0 0 E 0 2 b E

  8. n m = + ( ) H H ; ; n m n , , , F n m = = = = = = = = , , , 2 1 1 2 0 0 0 0 b 0 b 0 0 0 0 b + 0 0 0 b 0 0 0 0 0 0 b + n n n n n E b b E 0 0 0 0 0 0 0 0 b 0 0 E , , , , , 0 0 1 1 2 b E 0 0 0 0 0 0 b 0 0 + E b 0 0 0 a n E 0 0 0 0 n n E 0 2 b E / ; n , 2 , 1 , 1 ,0 ,0 ,1 ,1 , 2 / ; m ( ) 2 cos b E t ( ) , ( ) , n k k n + = ( ) H n F q F , , kn 2 cos b t E , k Floquet state H F

  9. n m = + ( ( ) ) H H ; ; n m n ( ) 0 t , , , F n m Time evolution operator = 1 ( ; ) U t t F t F 0 ( ) ( ) t e = iQt F t Using: the periodic structure of The unitarity of Is a complete set Some calculations U H F ( ) , n { } F / ,n ( ) ( ) n t = i H ; , exp ,0 t t n i t t e 0 0 F n Transition amplitude in Floquet space Time evolution operator of ( ) H Ct

  10. Relation to Quantized Field Theory ( ) ( ) n t = i H ; , exp ,0 U t t n i t t e 0 0 F n Transition amplitude in Floquet space Time evolution operator of ( ) H Ct The transition amplitudes in Floquet space is the Fourier series coefficients of the time evolution operator(!) the resolvant operator is the Fourier transform of ( ) ( ) 0 0 ; ( G z U t t z H = = + 1 ( ) ; U t t 0 ( ) 1 = + + + ) V G G VG G VG VG 0 0 0 0 0 0

  11. ( ) ( ) H , exp ,0 G z n i t t 0 F But is in Floquet space (not Hilbert-Fock quantum space ) F H Q= + + H H H H atom field interaction ( ) ( ) 1 2 1 q m p a e p a e + j t j t + * k k N 0 , , k k , , k k 2 , k , k 0 H H Two differences between and : Q F H 1. start form n=0 while at Q H H F 2. off-diagonal elements depend on n . Q

  12. = = = = = = = = , , , 2 1 1 2 0 0 0 0 b 0 b 0 0 0 0 b + 0 0 0 b 0 0 0 0 0 0 b + n n n n n E b b E 0 0 0 0 0 0 0 0 b 0 0 E , , , , , 0 0 1 1 2 b E 0 0 0 0 0 0 b 0 0 + E b 0 0 0 a n E 0 0 0 0 n n E 0 2 b E / ; n , 2 , 1 , 1 ,0 ,0 ,1 ,1 , 2 / ; m

  13. H H Main differences between and : H and are similar but NOT the same! F H Q F Q H 1. off-diagonal elements depend on n . Q H 2. start form n=0 while at Q H But, our writer didn t give up. F Jon H. Shirley solution : consider in the vicinity of some very large photon number N H Q why? ( ) In the matrix region, the off-diagonal terms change slowly. if is an eigenvalue of then + F H 1 a a N , is also eigenvalue. n

  14. 1 N Therefore: = + + + N H H H H H 1 atom field int Floquet Q Authors claim : The quantum state is approximately isomorphic to the Floquet state for . ;m N m + ;N m Floquet states can be interpret as quantum states containing a definite though very large number of photons.

  15. = + + + N H H H H H 1 atom field int Floquet Q = = = = = = = = , , , 2 1 1 2 0 0 0 0 b 0 b 0 0 0 0 b + 0 0 0 b 0 0 0 0 0 0 b + n n n n n E b b E 0 0 0 0 0 0 0 0 b 0 0 E , , , , , 0 0 1 1 2 b E 0 0 0 0 0 0 b 0 0 + E b 0 0 0 a n E 0 0 0 0 n n E 0 2 b E / ; n , 2 , 1 , 1 ,0 ,0 ,1 ,1 , 2 / ; m

  16. + N H H ( 1 Could we reconstruct from the semiclassical amplitude ? Floquet ) 0 t t Q ; U 2 0/4 e in t n e n Using coherent states. Assuming large number of photons. peaked at Using the periodicity properties of to get rid of N. ( ) 0 ; , n Quantum-Floquet theory: Equivalent to semiclassical theory. Admits interpretation in terms of quantized field. 0 n 2 ! n n A n 2 0/ 2 n A N and extremely small elsewhere H F ( ) in t = H exp ,0 U t t n i t t e 0 F

  17. H More AMAZING things with F Rabi formula + correction: Valid for large times No averaging over a continuum (Fermi s golden rule) Bloch-Siegert shift: easier derivation Simple derivation of higher orders Transition probability for multiple quantum transitions (non-directly connected states) P , t b = 0.25 b = 0.5 ;0 ;1 ;2 ;3 Applied to more than 2 level quantum state.

  18. All of this because - i t i t i t = + 2cos t e e e Thank you.

Related


More Related Content