plans for strong-field QED experiments at FACET-II€¦ · Institute #1 #4 #1 R. #4 R. ™ ™...
Transcript of plans for strong-field QED experiments at FACET-II€¦ · Institute #1 #4 #1 R. #4 R. ™ ™...
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plans for strong-field QED experiments at FACET-II
David A. ReisStanford PULSE Institute
Departments of Applied Physics and Photon Science
Physics Opportunities at a Lepton Collider in the Fully Nonperturbative QED Regime, August 7–9, 2019, SLAC
+"#
https://www.exhilp.org
Free registration until August 15
https://www.exhilp.org
Free registration until August 15
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FACET-II SFQED proposal collaboration* approved as E320
Collaborating Institutions: Carleton University (Canada), Aarhus University (Denmark). Ecole Polytechnique(France) Max-Planck-Institut für Kernphysik (Germany), Helmholtz-Institut Jena (Germany), Friedrich-Schiller-Universität Jena (Germany), Universidade de Lisboa (Portugal), Queen's University Belfast (UK), California Polytechnic State University (CA USA), Lawrence Livermore National Laboratory (CA USA), Princeton University (NJ USA), SLAC National Accelerator Laboratory (CA USA), University of California Los Angeles (CA USA), University of Colorado Boulder (CO USA), University of Nebraska - Lincoln (NE USA)
SFQED theory & simulation A. DiPiazza, F. Fiuza, T. Grismayer, C.H. Keitel, S. Meuren, L.O. Silva, D. Del Sorbo, M. Tamburini, M. Vranic
SLAC E144 DAR (SF AMO/xray), T. Koffas (HEP)
LWFA SFQED experiments G. Sarri, M. Zepf
Crystal SFQED experiments R. Holtzapple, U. I. Uggerhoj
Strong-field AMO/x-ray science P.H. Bucksbaum, M. Fuchs, C. Rödel
Laser-plasma interaction, HEDP F. Albert, S. Corde, S. Glenzer, C. Joshi, M. Litos, W. Mori
Accelerator physics G. White
Detectors A. Dragone, C. J. Kenney
High intensity lasers A. Fry
(*@submission)
QED Critical Field (“Schwinger Field”)
Sauter (1931), Euler, Heisenberg, Schwinger
2 lc
2mc2
E
Dirac sea
e-e+
• Materialize pairs when work done in
(reduced) Compton wavelength equal
rest mass
(four orders higher for µ+µ-)
• Exponentially suppressed E < Ecr
• Critical intensity for EM-field (peak):
• Need to also conserve momentum (not possible in single plane-wave)
Photonics Spectra, Nov. 1997
Ecr =m2c4
e~c = 1.3⇥ 1016V/cm
eEcr�̄c = mc2
Icr = 4.6⇥ 1029W/cm2
Invariant field strength (classical and quantum parameters)
⌘ =e
mc2
qhAµAµi = eE�
2⇡mc2
⌥ =e~
m3c5
qh(Fµ⌫p⌫)2i =
eE⇤�c
2⇡mc2= ⌘
�c
�⇤
$∗ = $ 1 + ()
*+ = $,)( 1 + () − 1)Note as defined here E is rms value to be independent of polarization. for strong-fields and linear polarization peak value often used
Leads to time-averaged effective mass and ponderomotive energy:
−
- Ip
Photoionization/linear Breit-Wheeler
Above threshold
- Ip
TunnelingSchwinger breakdown
High-field, low frequency
e(-aΥ)
- Ip
Multi-photon IonizationNonlinear Breit-Wheeler
High field, below threshold
~ η(2n)
Transition depends on both field and frequency
⌘ = ⇠ = a0 =eE
m!c,⌥ = � =
E
Ec
Analogy: regimes of atomic ionization
Non-linear/non-perturbative QED
= + + + + · · ·
Exactly solvable in terms of dressed state (Furry, Volkov, …)
e!
e+
! k"µ
pµ
1
pµ
2
Photon emission
Multi-photon ComptonQuantum radiation reaction…
Photon decay
Multi-photon Breit-Wheeler Pair production“Schwinger” pair production…
⌘ =e
mc2
qhAµAµi = eE�
2⇡mc2⌥ =
e~m3c5
qh(Fµ⌫p⌫)2i =
eE⇤�c
2⇡mc2= ⌘
�c
�⇤-
See e.g. Reiss 1962, Nishikov and Ritus , 1963, Narozhni, Nishikov and Ritus, 1965…
pµ
k!µ
p!µ012
02
032
042
02 = 52 + 672 , 6 = ()$)
2(75)0) = $∗)
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How produce such high intensities?
50 GeVE-field is not Lorentz-invariant. boosted by
4g2 intensity 2g field
in electron’s frame
E144 reached U ~ 0.3, h ~ 0.3 (rms)
Bucksbaum et al., 2018 NAS Report, …reaching the brightest light
LCLS*
*LCLS @ ~1Å
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How produce such high intensities?
D. Strickland and G. Mourou, “Compression of amplified chirped optical pulses”, Opt. Commun. 56, 219 (1985)
1/2 of 2019 Physics Nobel
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Focused Intensity Frontier
20TW/13GeVFACET-II (E320)
20TW(lab frame)
50 GeV
Y >1 possible nowwith current facilities (SLAC/DESY…)…and modest laser
Front row: G. Horton-Smith, Th. Kotseroglou, W. Ragg, S. BoegeMiddle row: D. Meyerhofer, W. Bugg, A. Weidemann, D. Walz, J.Spencer, K.McDonald, A. MelissinosLast row: K. Shmakov, C. Bamber, U. Haug, D.Burke, C.BulaAbsent: S. Berridge, C. Field, Th. Koffas, E. Prebys, D.Reis
E144 experiment: nonlinear QED in laser+e- collisions
D.L.Burke et al, PRL79 1626(1997) C.Bamber et al, Phys.Rev. D60 090024(1999)
E144: 1st experiment in nonlinear QED (laser+ ultrarel. e- collisions)
Bula et al., PRL 1996, Burke et al., PRL 1997, Bamber et al., PRD. 1999
n=1
n=4
FFTB (now LCLS transport)
e + nw à e’ +w’ q+nk = q’ +k’
Calculations: h= 0.6, l=1054nm, circ. polarization.1J , A= 50µm2 , t=1.88 ps, 5•109 e- in 60x60x870µm3 (rms)
Nonlinear Compton Scattering
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(a)
t [psec]
x [µ
m]
(a)
t [psec]
x [µ
m]
(b)
-200
-100
0
100
-10 -5 0 5 10-200
-100
0
100
-10 -5 0 5 10
N1/Ng N2/Ng
Pert. NLC and finding overlap (t,x)
e- + Nw à e-’ +w’w’+nw à e+ + e-
q+Nk = q’ +k’k’+nk = e++e-
Most probably N=1, n=4–5 for IR
Background: non-sequential trident e- + nw -> e-’ +e+ + e-
Estimated to be 2–3 orders of magnitude lower, no theory at the timen=5–6
Nonlinear Breit-Wheeler pair production
Threshold, :;;1 = $∗)
e- + Nw à e-’ +w’w’+nw à e+ + e-
q+Nk = q’ +k’k’+nk = e++e-
Most probably N=1, n=4–5 for IR
n=5–6
Nonlinear Breit-Wheeler pair production
Threshold, :;;1 = $∗)
See e.g. Hu, Müller, Keitel, PRL 105, 080401 (2010)
Strong-field trident:
Threshold, < 1 − = ; = 4$∗
Also, Ilderton, PRL (2011) …
0
10
20
30
40
10 15 20
N(e
+ ) per
2 G
eV/c ON
OFF(a)
0
5
10
15
20
10 15 20
dN(e
+ )/dp
[1/G
eV/c] (b)
0
5
10
15
20
10 15 20positron momentum [GeV/c]
ONOFF
(c)
0
5
10
10 15 20positron momentum [GeV/c]
(d)
h>0.216
h>0.216
106±14 signal out of ~22k shots
69±9 signal out of ~22k shots
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E144 Measured in transition regime
19Multi-photon picture
Tunneling Picture (Schwinger)
Υ = E/Ec
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Anomalous 2-photon X-ray Compton, Be@1020 W/cm2. (h~10-3, U~10-5)
Fuchs et al., Nature Physics, 2015
-0.4! 0! 0.4! 0.8 ! 1.2! 1.6!
minimum redshift [keV]!-0.4! 0! 0.4! 0.8 ! 1.2! 1.6!
minimum redshift [keV]!
Low Intensity (2ω;$n=1)$High-Intensity (ω+ω;$n=2)$
-0.4! 0! 0.4! 0.8 ! 1.2! 1.6!
minimum redshift [keV]!-0.4! 0! 0.4! 0.8 ! 1.2! 1.6!
minimum redshift [keV]!
Low Intensity (2ω;$n=1)$High-Intensity (ω+ω;$n=2)$
! + ! ! !K(18 keV)
High Intensity n=2,w+w Low Intensity n=1, 2w
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Anomalous 2-photon X-ray Compton, Be@1020 W/cm2. (h~10-3, U~10-5)
-0.4! 0! 0.4! 0.8 ! 1.2! 1.6!
minimum redshift [keV]!-0.4! 0! 0.4! 0.8 ! 1.2! 1.6!
minimum redshift [keV]!
Low Intensity (2ω;$n=1)$High-Intensity (ω+ω;$n=2)$
But, semiclassical+QED/TDSE: no anomaly. Krebs, DAR, Santra, PRA, 2019
Additional missing momentum on order Z/a0
Proposed mechansismcombined scattering and absorption
Red-shift incompatible with free-electron or atomic impulse response
Fuchs et al., Nature Physics, 2015
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E320 on FACET-II will test various aspects of SFQED
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Laser Parameter Table
!1
Function Present Optimal Present
40 TW(Gratings set
limit)100 TW
(Pump sets limit)Limits?Why?
UpgradesDazzler/Wizzler
Deformable Mirror
Dazzler/etcDeformable
MirrorGAIA
Gratings
Dazzler/etcDeformable Mirror
GAIA-HPCompressor Box
Power-amp Pump [J] 2.8 3.6 7.5 16.0
Power-amp Output [J] 0.6 1.1 2.3 4.8 30% from pump to output
Beam Transport Input [J] ? 1.0 2.0 4.3 90% Expected due to polarizer
Compressor Input [J](beam transport output) 0.4 0.9 1.8 3.9
65% measured at FACET90% Expected from transport
input to compressor (11 optics @ 99%, 21 optics at 99.5%)
Beam Size @ Compressor
4 cm diameter150 ps fwhm
4 cm diameter150 ps fwhm
6 cm diameter150 ps fwhm
10 cm diameter900 ps fwhm
1.8 J@ 6 cm max input measured at MEC ?? ps
Compressor Output [J] 0.25 0.61 1.28 2.72 65% measured at FACET70% expected
Pulse Duration (fwhm) [fs] 70.0 35.0 35.0 35.0 <40 fs requires spectral
shaping
Peak Power [TW] 3.6 17.5 36.5 77.8
Intensity* [1018 W/cm^2] 23.7 116.3 242.4 517.0 3 um focus
a0* 3.3 7.3 10.6 15.4 3 um focus
Upgrade $** 0.0 50+100+100 100+100+400+25 100+100+400+Comp
*Intensity and a0 based on document sent around by Sebastian
FACET-II laser expected performance
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Reaching strong-field regime @FACET-II
Baseline: 20 TW, 10 GeV
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0.1 1 10 100
a0
0.1
1
10¬
10Ge
V
7Ge
V15Ge
V20
GeV
30Ge
V
1Ge
V2Ge
V
LWFA
E144E144
1020 W/cm2
1021 W/cm2
1019 W/cm2
fullquantumregime
moderatequantumregime
classicalregime
laser:perturbation
laser:nonperturbative
Reaching strong-field regime @FACET-II
U,c
h,x,a0
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Reaching strong-field regime @FACET-II. 20 TW laserSFQED@FACET-II: baseline setup (20 TW laser)
Major scientific objectives
Unstable strong-field quantum vacuum
≠æ first observation of tunneling pair production (≥ 103 pairs per shot)Quantum radiation reaction
≠æ failure of the classical Landau Lifshitz equation, quantum stochasticityBreakdown of perturbation theory
≠æ absorption of ≥ 102 laser photons, emission of ≥ 5 photons (per electron)
Electron spectrum
2 4 6 8 10electron energy [GeV]
10�4
10�3
10�2
10�1
100
prob
abili
ty[a
.u.]
2 4 6 8 1010�4
10�3
10�2
10�1
100
simul
atio
n:M
.Tam
burin
i
– Quantum radiation reaction: stochasticity– Deviations from Landau Lifshitz (dotted)
Photon spectrum
10�2 10�1 100 101
photon energy [GeV]
10�3
10�2
10�1
100
inte
nsity
[a.u
.]
10�2 10�1 100 10110�3
10�2
10�1
100
simul
atio
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– Highly nonlinear Compton scattering– Local constant field approx. fails (dotted)
Sebastian Meuren (Princeton University) 7 / 10 Probing SFQED with Ultraintense Laser
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Reaching strong-field regime @FACET-II. 20 TW laserSFQED@FACET-II: baseline setup (20 TW laser)
Major scientific objectives
Unstable strong-field quantum vacuum
≠æ first observation of tunneling pair production (≥ 103 pairs per shot)Quantum radiation reaction
≠æ failure of the classical Landau Lifshitz equation, quantum stochasticityBreakdown of perturbation theory
≠æ absorption of ≥ 102 laser photons, emission of ≥ 5 photons (per electron)
Electron spectrum
2 4 6 8 10electron energy [GeV]
10�4
10�3
10�2
10�1
100
prob
abili
ty[a
.u.]
2 4 6 8 1010�4
10�3
10�2
10�1
100
simul
atio
n:M
.Tam
burin
i
– Quantum radiation reaction: stochasticity– Deviations from Landau Lifshitz (dotted)
Photon spectrum
10�2 10�1 100 101
photon energy [GeV]
10�3
10�2
10�1
100
inte
nsity
[a.u
.]
10�2 10�1 100 10110�3
10�2
10�1
100
simul
atio
n:M
.Tam
burin
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– Highly nonlinear Compton scattering– Local constant field approx. fails (dotted)
Sebastian Meuren (Princeton University) 7 / 10 Probing SFQED with Ultraintense Laser
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Beamline layout (~IP to dump)
E-320 (SFQED)Phase 1, e- + e+ spectrometer + diagnostics
Phase 2, add gamma spectrometer
Phase 3-X, multi-color, upgraded laser? second IP for Gamma + laser…
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SFQED@FACET-II
w =1.55 eV, h = 17, U= 3
w =1.55 eV, h = 17, U= 1.6w =4.8 eV, h <<1, Y = 0
w =1.55 eV, h <<1, U = 0, circ pol.
strong-field Compton, quantum rad. reaction
strong-field Pair production
Vacuum birefringence
w =1.55 eV, h < 17, U< 0.4
Precision measurement using 100 TW, focused to 4µm
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“New” physics: re-collisions.
( ≫ 1, Υ ∼ 1, Stationary phase approximation, Tunneling, classical trajectories, re-collisions similar to SF-AMO
Possiblity for B4 + µ3, D4 + D3; DF… productions well below threshold
S. Meuren, thesis Heidelberg 2015
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And then what…
New facility in research yard or LCLSMulti-PW laser (already planning on MEC, but w/o conventional ultra-rel. Beam)Gang 2nd and 3rd km -> 30GeV, nm, fs beamsafterburner-> 60 + GeVx-rays…
100GeV collider?
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Acknowledgments
• FACET-II SFQED collaboration (S. Meuren et al.)
• E144 collaboration, (especially K. McDonald, A. Melissinos, T. Koffas)
• SFQED@SLAC working group: (DAR, P. Bucksbaum, T. Abel, R. Blandford, F. Fiuza, S. Glenzer, M. Hogan, V. Yakimenko, Z. Huang, C. Pellegrini, A. Fry, S. Brodsky, S. Meuren)
(DAR, PHB: FES, SM: HEP/FES)