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Strong-field physics in the x-ray regime Louis DiMauro ITAMP FEL workshop June 21, 2006 fundamental studies of intense laser-atom interactions generation.

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Presentation on theme: "Strong-field physics in the x-ray regime Louis DiMauro ITAMP FEL workshop June 21, 2006 fundamental studies of intense laser-atom interactions generation."— Presentation transcript:

1 strong-field physics in the x-ray regime Louis DiMauro ITAMP FEL workshop June 21, 2006 fundamental studies of intense laser-atom interactions generation and application of attosecond pulses ultra-fast optical engineering

2 LCLS parameters XFELs are an x-ray source of unprecedented brightness only viable sources are accelerator-based

3 LCLS is great but not perfect  e - undulator B-field w ~ cm SASE FEL lasing builds up from noise

4 …so theorists beware what we think we are measuring may not be what we are measuring! …and welcome to the 70’s!

5 Linac Coherent Light Source at SLAC 15 GeV e-beam, 100 meter long undulator output: 0.8-8 keV (1.5 A), 10 GW, 10 12 photons/shot, 230 fs, 120 Hz five thrust areas slated for first operations

6 AMOP at the LCLS LCLS experimental halls AMOS team located in the near-hall initial experimental end-station on soft x-ray beamline (0.8-2 keV) scientific thrust: fundamental strong-field interactions at short wavelengths

7 AMOS team experimental menu short term strategy shine light on Roger’s wall (scientific impact) define a prominent role in XFEL development atomic ionization (nonlinear physics/metrology) x-ray scattering from aligned molecules (laser/x-ray experiments) cluster dynamics (non-periodic imaging)

8 contrast: long and short wavelength strong-field physics ponderomotive potential is everything at long wavelengths e - in Coulomb + laser fields electron ponderomotive energy (au): U p = I/4  2 displacement:  = E/  2 PW/cm 2 titanium sapphire laser: U p ~ 60 eV &  ~ 50 au for LCLS @ 10 2 PW/cm 2 U p &  are zero!

9 contrast: long and short wavelength strong-field physics laser multiphoton ionization x-ray multiphoton ionization n=2 neon photoabsorption n=1 laser multiphoton ionization

10 x-ray strong field experiment x-ray multiphoton ionization photoionization Auger 2-photon, 2-electron sequential correlated ionization

11 needle in the haystack: coincidence measurements reaction microscopy Schmidt-Böcking J. Ullrich et al., JPB 30, 2917 (1997) detect by correlating particle-particle events

12 coincidence measurement true-to-false ratio: T/F =  t C f  (  1 C + N 1 )(  2 C +N 2 )  t,1,2 ( , ,  )  detection coefficients N 1,2  noise counts C  average count rate f  repetition rate the 120 Hz operation of the LCLS makes coincidence experiments high risk, thus the initial AMOS end-station will not have this capability.

13 AMOS end-station: single-shot measurements courtesy of John Bozek

14 LCLS parameters for strong-field studies photon energy:800 eV number of photons:10 13 /shot pulse energy:1 mJ peak power:5 GW focused spot size:1  m flux:10 33 cm -2 s -1 intensity:10 17 W/cm 2 period:2 as number of cycles:40,000 ponderomotive energy:25 meV displacement:0.003 au

15 global survey of single atom response Keldysh picture optical frequency tunneling frequency    = (I p /2U p ) 1/2  -1 “photon description”      “dc-tunneling picture”      tunnel MPI Ti:sap & Nd excimer  CO 2 data compiled based on both electron and ion experiments mir  lcls

16 1-photon, 1-electron ionization consider a 1-photon K-shell transition:  K  10 -18 cm 2 R K =  K F lcls  10 15 s -1 (saturated) t K = 1/R K = 1 fs photoionization L-shell neon photoabsorption K-shell rapid enough to ionize more than one electron! fast enough to compete with atomic relaxation? is the external field defining a new time-scale?

17 2-photon, 2-electron ionization 2-photon, 2-electron S.A. Novikov & A. N. Hopersky, JPB 35, L339 (2002) consider a 2-photon KK-shell transition:  KK  10 -49 cm 4 s R KK =  KK F 2 lcls  10 17 s -1 (saturated) t KK  10 as neon  KK  10 -52 cm 4 s so R KK   R K

18 2-photon, 2-electron ionization 2-photon, 2-electron are the electrons correlated? in a strong optical field single electron dynamics dominate. photoionizationAugerphotoionization i.e. is it sequential ionization?

19 2-photon, 1-electron ionization consider a 2-photon K-shell transition: estimate 2-photon cross-section,  2 perturbative scaling laws 1 :  2  10 -54 cm 4 s 2 nd -order perturbation theory 2 :  2  10 -52 cm 4 s 1 P. Lambropoulos and X. Tang, J. Opt. Soc. Am. B 4, 821 (1987) 2 S. A. Novikov and A. N. Hopersky, JPB 33, 2287 (2000) transition probability: P 2 =  2 F 2  lcls  0.1-1

20 x-ray above-threshold ionization estimate (2+1)-photon cross-section,  2+1  2+1 =  2  cycle   10 -90 cm 6 s 2 P 2+1 =  2+1 F 3  lcls  10 -4 ATI should be observable bound-continuum ATI bound-c-c ATI Auger ATI distinguishable

21 can the LCLS get to the strong-field regime impose a Keldysh parameter of one    = (I p /2U p ) 1/2  U p  400 eV (8 eV) @ 800 eV, intensity needed is 10 21 W/cm 2 (10 14 W/cm 2 )  = 0.3 au (19 au) number of photons is fixed, require tighter focus and shorter pulse  lcls ~ 10 fs (very possible) thus require a beam waist of 50 nm (in principle possible) tunnel MPI   lcls II

22 there are other sources on the horizon Cornell Energy Recovery Linac 10 7 photons/shot in 20 fs repetition rate: 0.1-1 MHz

23 coincidence measurement true-to-false ratio: T/F =  t C f  (  1 C + N 1 )(  2 C +N 2 )  t,1,2 ( , ,  )  detection coefficients N 1,2  noise counts C  average count rate f  repetition rate the 120 Hz operation of the LCLS makes coincidence experiments high risk, thus the initial AMOS end-station will not have this capability. the ERL does have the advantage of high duty cycle! does it have high enough intensity for exploring multiphoton processes?

24 maybe? consider a 2-photon K-shell transition: estimate 2-photon cross-section,  2 perturbative scaling laws 1 :  2  10 -54 cm 4 s 2 nd -order perturbation theory 2 :  2  10 -52 cm 4 s 1 P. Lambropoulos and X. Tang, J. Opt. Soc. Am. B 4, 821 (1987) 2 S. A. Novikov and A. N. Hopersky, JPB 33, 2287 (2000) ERL parameters: 10 6 /shot, 100 fs, 1A 20 nm waist yields flux ~10 30 cm -2 s -1 (10 15 W/cm 2 ) transition probability: P 2  10 -(5  7)

25 two-photon ionization LCLS use near resonant enhancement of  2 increase number of photons/shot over average power open the possibility of temporal metrology! ERL

26 2-photon, 2-electron ionization 2-photon, 2-electron S.A. Novikov & A. N. Hopersky, JPB 35, L339 (2002) consider a 2-photon KK-shell transition:  KK  10 -48 cm 4 s P KK  0.1 neon  KK  10 -52 cm 4 s coincidence investigations: atomic aligned molecules cluster dynamics

27 x-ray-laser metrology photoionization incoherent x-rays (250-400 eV) M L Auger M L Auger electron ~ 200 eV laser 10 12 W/cm 2   10 12 W/cm 2 Auger


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