Ultrafast and Intense-Field Nonlinear Optics Calculator

Analyze ultrashort pulses, beams, and Kerr effects. Compute fluence, electric field, Keldysh factor, and cutoff. Use clear inputs, exports, formulas, examples, and plain guidance.

Calculator Inputs

Reset

Example Data Table

Item Example Value
Pulse Energy30 µJ
Pulse Duration FWHM35 fs
Wavelength800 nm
Beam Radius25 µm
Linear Refractive Index1.0003
Nonlinear Index3.000e-23 m²/W
Interaction Length10 mm
Ionization Potential / Bandgap15.76 eV
Repetition Rate1 kHz
Peak Power805,714,285.714 W
Peak Intensity8.2069e+13 W/cm²
B-Integral1.933714 rad
Keldysh Parameter1.267590
Estimated HHG Cutoff31.306326 eV

Formula Used

Peak power: Ppeak ≈ 0.94 × Epulse / τFWHM

Average power: Pavg = Epulse × repetition rate

Average fluence: F = Epulse / (πw²)

Peak fluence: F0 = 2Epulse / (πw²)

Peak intensity: I0 = 2Ppeak / (πw²)

Field amplitude: Efield = √[2I / (n₀cε₀)]

B-integral: B = (2π/λ) × n₂ × I × L

Ponderomotive energy: Up(eV) = 9.337 × 10-14 × I(W/cm²) × λ²(µm²)

Keldysh parameter: γ = √[Ip / (2Up)]

HHG cutoff estimate: Ecutoff = Ip + 3.17Up

Rayleigh range: zR = πw² / λ

How to Use This Calculator

  1. Enter pulse energy in microjoules and pulse duration in femtoseconds.
  2. Provide wavelength and Gaussian beam radius at the interaction point.
  3. Enter the linear and nonlinear refractive indices for the medium.
  4. Set the interaction length for the nonlinear region or sample.
  5. Provide the ionization potential or effective bandgap in electronvolts.
  6. Enter repetition rate if you also want average power.
  7. Click calculate to show results below the header and above the form.
  8. Use the CSV or PDF buttons to save the generated output.

About This Calculator

Ultrafast and intense-field nonlinear optics links short pulses, high peak power, and nonlinear material response. Engineering work in this area often needs quick estimates before simulation or lab alignment. This page combines pulse, beam, and strong-field measures in one place.

The calculator starts from pulse energy, duration, wavelength, and beam radius. From those inputs, it estimates Gaussian peak power and on-axis peak intensity. It then extends the result to field amplitude, Kerr phase accumulation, and simple strong-field indicators.

B-integral helps estimate how much nonlinear phase may build through a medium. Large values can indicate spectral broadening, self-phase modulation, or a need to reduce length, intensity, or nonlinear index. That makes the value useful during design checks.

Ponderomotive energy and the Keldysh parameter help classify the interaction regime. When gamma is large, multiphoton behavior is stronger. When gamma approaches or drops below one, tunneling behavior becomes more important. This gives a practical first-pass view of field strength.

The HHG cutoff estimate gives a simple ceiling for high-order harmonic photon energy from the chosen field and target potential. It is not a full propagation or phase-matching model, but it is helpful for planning wavelength, focusing, and target choices.

Use the example table as a starting point, then refine inputs with your laboratory or design values. The graph adds a quick temporal pulse view, while the exports make it easier to share results with colleagues or include them in reports.

FAQs

1) What does this calculator estimate?

It estimates Gaussian peak power, average power, fluence, peak intensity, electric field amplitude, B-integral, ponderomotive energy, Keldysh parameter, HHG cutoff, photon energy, photon count, Rayleigh range, and confocal parameter from your pulse and beam inputs.

2) Why is Gaussian pulse shape used here?

Many ultrafast systems are approximated well by Gaussian temporal and spatial profiles. That makes the calculator practical for first-pass engineering estimates, while still remaining simple enough for fast design checks and lab planning.

3) What beam radius should I enter?

Enter the 1/e² Gaussian beam radius at focus or at the interaction region. Do not enter full diameter unless you first divide it by two. Consistent beam definition matters strongly for intensity and fluence estimates.

4) What does the B-integral tell me?

B-integral estimates accumulated nonlinear phase. Higher values can signal stronger self-phase modulation and rising risk of pulse distortion. It is useful for checking whether a chosen material length and intensity are reasonable.

5) How should I interpret the Keldysh parameter?

Gamma much greater than one suggests multiphoton-dominated behavior. Gamma near one indicates transition behavior. Gamma below one points toward tunneling-like behavior. It is a quick regime indicator, not a complete physical model.

6) Is the HHG cutoff value exact?

No. It is a simple estimate based on ionization potential and ponderomotive energy. Real harmonic generation also depends on propagation, phase matching, depletion, pulse shape, target density, and many experimental details.

7) Can I use this for solids and gases?

Yes, as a first-pass estimator. For solids, the entered target potential can represent an effective bandgap. For gases, it can represent ionization potential. Always validate final designs with experiment or full simulation.

8) Why are CSV and PDF downloads included?

They make results easier to archive, compare, and share. You can save output during test runs, attach it to design notes, or send quick summaries to teammates without retyping every calculated value.

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Important Note: All the Calculators listed in this site are for educational purpose only and we do not guarentee the accuracy of results. Please do consult with other sources as well.