attosecond-physics

Layer 1 — Physics24 concepts in this subtree

Physics of light pulses and dynamics on the attosecond (1 as = 10⁻¹⁸ s) time-scale. 2023 Nobel Prize (L'Huillier, Krausz, Agostini) recognised the high-harmonic-generation (HHG) pathway to attosecond extreme-UV / soft-X-ray pulses via the…

HHG three-step model (Corkum 1993): ionise → propagate → recombine
Attosecond streak camera: momentum shift Δp(τ) = e·A_IR(τ)
CPA (Strickland-Mourou 1985, 2018 Nobel): stretch → amplify → compress
Keldysh parameter γ = √(I_p/(2U_p)): multiphoton ↔ tunnel boundary
HHG cutoff (Corkum 1993): ℏω_max = I_p + 3.17·U_p
Ponderomotive energy: U_p = e²E₀²/(4m_eω²); practical U_p[eV] ≈ 9.33·10⁻¹⁴·I[W/cm²]·λ²[μm²]
Strong-field-approximation saddle-point: ∂_t S(p,t) = 0; Hamilton–Jacobi action
RABBITT sideband S_{2q} = A + B·cos(Δφ + 2ω_IR τ_d); Bessel-function amplitudes
Gaussian wavepacket spreading: σ(t) = √(ℏ²t² + 4m²σ₀⁴)/(2mσ₀); heat-like diffusion
HHG cutoff E_max = I_p + 317·U_p/100 via SFA saddle-point Hamilton–Jacobi action
RABBITT: S_{2q} = A + B·cos(Δφ + 2ωτ); J₀(0) = 1; J₁(z) ≈ z/2 weak-field
Wavepacket σ(t) = √(ℏ²t² + 4m²σ₀⁴)/(2mσ₀); σ(0) = σ₀; lim_{t→∞} dσ/dt = ℏ/(2mσ₀)
HHG three-step (Corkum 1993)
Isolated attosecond pulse (Krausz 2001)
RABBITT (Paul 2001 / Muller 2002)
Eisenbud-Wigner-Smith delay
Charge migration (Cederbaum 1999)
Keldysh-Faisal-Reiss SFA
First attopulse (Hentschel 2001)
Train (Paul 2001)
HHG model (Corkum 1993)
Wigner delay (Eisenbud-Wigner 1955)
Streak camera (Itatani 2002)
Water-window HHG (Popmintchev 2012)
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