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A. Dubietis coauthored the 1992 paper introducing chirped and stretched pulse parametric amplification in beta barium borate with G. Jonušauskas and A. Piskarskas. Its publisher Abstract reports compressed pulses of $70\mathrm{fs}$ and approximately $0.9\mathrm{GW}$ output power.^[ref]

The approach connects optical parametric amplifier with the central logic of chirped pulse amplification: amplify a temporally stretched signal, then compensate its spectral phase to recover a short optical pulse. The amplified optical bandwidth matters because a narrow spectrum cannot support an arbitrarily short pulse, even with ideal compression.

For an original Gaussian pulse example, an intensity full width at half maximum $\Delta t$ and ordinary-frequency intensity width $\Delta \nu$ satisfy $\Delta t\Delta \nu =2\ln 2/\pi \approx 0.441$ for a transform-limited pulse. Thus a Gaussian spectrum of width $10\mathrm{THz}$ supports a transform-limited intensity duration of about $44.1\mathrm{fs}$. A measured duration of $100\mathrm{fs}$ with that same spectrum would have time-bandwidth product one, exceeding the transform-limited value. Residual spectral phase can account for such broadening, though the product alone does not uniquely reconstruct that phase. The stipulated bandwidth and durations are illustrative, not additional experimental data from the paper.

A. Piskarskas coauthored the 1992 demonstration of optical parametric chirped pulse amplification with A. Dubietis and G. Jonušauskas. The paper amplified chirped, stretched pulses in beta barium borate and reported compression to $70\mathrm{fs}$.^[ref]

The method combines two useful operations. A chirp correlates optical frequency with position within an optical pulse, permitting the pulse to be stretched before amplification and recompressed afterward. An optical parametric amplifier transfers energy from a pump wave to a signal and an idler through an interaction governed by nonlinear optics. Stretching limits the instantaneous signal intensity during amplification while leaving a route to short final duration.

For an original rectangular-pulse estimate, take laser pulse energy $E=1\mathrm{mJ}$. A duration of $100\mathrm{fs}$ gives $P=E/\tau =10\mathrm{GW}$, whereas stretching to $10\mathrm{ps}$ gives $100\mathrm{MW}$ at the same energy. The factor of 100 follows from the stipulated pulse shape and duration ratio. Real shaped pulses require the corresponding relation between laser pulse energy, peak power and pulse duration; amplification and recompression also introduce losses. These numbers illustrate the design principle, not the 1992 apparatus's energy or pump conditions.

G. Jonušauskas coauthored the 1992 beta barium borate experiment with A. Dubietis and A. Piskarskas, demonstrating parametric amplification of chirped and stretched femtosecond pulses.^[ref]

An optical parametric amplifier must satisfy both frequency relations and phase matching. For a pump, signal and idler with angular frequencies ${\omega }_p,{\omega }_s,{\omega }_i$, the three-wave process obeys ${\omega }_p={\omega }_s+{\omega }_i$. Coherent buildup also depends on their wavevectors: ideally ${\mathbf{k}}_p={\mathbf{k}}_s+{\mathbf{k}}_i$. Matching frequencies alone does not ensure that fields generated at different positions add constructively.

For an original undepleted-pump, weak-conversion illustration, suppose the driving amplitude is uniform along a crystal of length $L$. A scalar phase mismatch $\Delta k$ makes the generated field proportional toAt exact phase matching the limiting amplitude is proportional to $L$. At $\Delta kL=2\pi$ the idealized integral is zero because contributions cancel. This elementary coherent-sum model explains the need to control crystal orientation and optical frequencies; it is not the full high-gain solution or a reported setting from Jonušauskas's experiment.

An optical parametric amplifier transfers energy from a pump beam into a signal and an idler through nonlinear optics. For the common three-wave mixing process, their angular frequencies obey ${\omega }_p={\omega }_s+{\omega }_i$. A strong pump and a weaker signal enter a nonlinear medium; the signal grows and an idler is generated.

Efficient growth requires phase matching so that contributions generated along the medium reinforce. Changing crystal orientation or temperature can tune the matched frequencies. Measuring the signal with and without the pump tests amplification, while observing the corresponding idler checks the frequency-conversion mechanism. The pump supplies the extra energy; the process does not require a stored population inversion.^[ref]

Optical parametric chirped pulse amplification combines the stretch–amplify–compress sequence of chirped pulse amplification with an optical parametric amplifier. A stretched signal pulse overlaps a strong pump pulse in a nonlinear crystal. Three-wave mixing transfers pump energy into the signal and an idler; subsequent pulse compression brings the amplified signal's frequencies back together. The pump supplies the added energy, rather than a stored population inversion.^[ref]

A. Dubietis, G. Jonušauskas and A. Piskarskas reported chirped and stretched pulse parametric amplification in beta barium borate in 1992. Their paper establishes a concrete early implementation of the parametric route; its published title identifies the nonlinear crystal.^[ref]

For pump, signal and idler angular frequencies, the conversion obeysEfficient amplification also requires phase matching, so contributions generated along the crystal reinforce. For collinear propagation the corresponding wave-vector relation is $k_p=k_s+k_i$; a noncollinear geometry requires the vector relation. Crystal dispersion and the chosen geometry determine which signal bandwidth is efficiently amplified.

An original energy-accounting example uses a 515-nanometre pump and an 800-nanometre signal. Their vacuum wavelengths giveSuppose 40 percent of a 2-millijoule pump is converted into signal–idler pairs, with negligible seed energy and other losses in this chosen model. Each conversion divides photon energy according to frequency, so the added signal energy isThe idler receives the remaining 0.285 millijoule. Assigning all depleted pump energy to the signal would violate this accounting.

If a compressor transmits 80 percent of that signal energy into a 50-femtosecond Gaussian pulse, the surviving energy is 0.412 millijoule. The chirped pulse amplification energy budget givesThese are stipulated teaching values, not a reconstruction of the 1992 experiment. Stretching lowers peak power during amplification; it does not remove the need to manage pump intensity or optical damage.

A useful apparatus check varies pump–signal delay while recording signal and idler spectra and energies. This tests temporal overlap and the frequency-conversion relation. Measuring the compressed pulse separately checks whether amplified bandwidth and residual spectral phase support the claimed pulse duration. Gain alone does not demonstrate successful compression, and an energy measurement alone does not establish peak power.

An optical parametric oscillator places an optical parametric amplifier inside an optical resonator that feeds back at least one generated wave. Pump energy is converted into signal and idler waves satisfying the frequency relation of the underlying three-wave mixing process.

Oscillation begins when round-trip gain overcomes loss at an allowed resonator mode. Below that threshold, weak generated emission can still occur, but sustained oscillation is absent. Tuning the phase matching and resonator together gives a tunable source at wavelengths difficult to obtain directly from a particular laser. Pump power alone does not select the output: cavity resonances, conversion gain and optical losses also matter.

A single optical mode in a squeezed vacuum state. In principal optical quadratures, its variances are $e^{-2r}/4$ and $e^{2r}/4$, while its mean photon number is ${\sinh }^{2}r$. Its mean field vanishes. A degenerate optical parametric amplifier generates the state by pair creation with phase fixed by the pump. Loss admixes unsqueezed vacuum and limits the measured variance reduction.

A degenerate optical parametric amplifier sends a strong pump at $2\omega$ through a phase-matched second-order nonlinear medium, creating pairs in a selected mode near $\omega$. With the pump treated classically and undepleted, the effective interaction is quadratic in the mode's creation and annihilation operators. Vacuum input evolves into an optical squeezed vacuum; the pump phase fixes the quiet optical quadrature. A cavity enhances the interaction below oscillation threshold. balanced homodyne detection compares this optical quadrature's noise with the blocked-signal vacuum reference; phase locking, detector balance, electronic-noise measurement and loss calibration distinguish squeezing from an instrumental noise reduction. A primary cavity experiment observed below-vacuum noise by degenerate down conversion and balanced homodyne readout.^[ref]

Use $S(r)=\exp [\frac{r}{2}(a^2-a^{†2})]$, so $S^{†}aS=a\cosh r-a^{†}\sinh r$. Write $s={\sinh }^{2}r$, $c=\cosh r$ and $N=a^{†}a$. Vacuum expectations then givePair creation makes the mean field zero while the mean photon number is positive. Expanding the transformed ladder operators in the vacuum gives the squeezed-vacuum photon-number moments: $⟨N(N-1)⟩=3s^2+s$ and $⟨N^2⟩=3s^2+2s$; equivalently $\mathrm{Var}N=2s(s+1)$.

The vectors produced by photon addition and photon subtraction in the paper are not normalized. Their squared norms are $s+1$ and $s$, respectively. A particularly direct evaluation isBoth successful operations therefore prepare the same squeezed one-photon state, up to an overall phase, whenever subtraction has nonzero probability. Since $⟨1|S^{†}NS|1⟩=c^2+2s=1+3s$, the unnormalized moments areThe printed photon-added formula equals $M_{+}$, not a normalized mean. With its literal unnormalized convention, the corresponding subtraction result is $M_{-}$ andThis difference tends to one as $r\to 0$ and grows as $\frac{3}{4}{e}^{2r}$ for large positive $r$. Keeping this convention recovers the paper's requested expression without misidentifying it as a physical conditional mean.

For the normalization of photon-added and photon-subtracted states, divide by the squared norms to obtain actual conditional means:These equalities for subtraction require $s>0$. As $r\to 0$ the normalized successful subtraction tends to $|1⟩$, but its success probability vanishes; exactly at $r=0$, $a|0⟩=0$ gives no conditional state. At large $r$, both normalized means grow as $3e^{2r}/4$, while their difference remains zero.

For the photon statistics of a squeezed vacuum, the even-number probabilities areAfter subtraction the normalized distribution is $p_n^{-}=(n+1)p_{n+1}/s$. It has only odd occupation and no vacuum component. photon addition gives $p_n^{+}=n{p}_{n-1}/(s+1)$, identical here to $p_n^{-}$. The diagram uses normalized distributions with an explicitly chosen $r$, rather than treating the unnormalized moments as means.

A subtraction event samples initial occupation with weight $n$, preferentially selecting the larger components before removing one photon. In general ${\bar{n}}_{-}=⟨N(N-1)⟩/⟨N⟩=⟨N⟩-1+\mathrm{Var}N/⟨N⟩$. Here the large variance gives ${\bar{n}}_{-}-⟨N⟩=1+2s>0$. This conditional photon-number bias does not create energy by removing a photon: the unconditional ensemble also includes the runs without a heralded event.