bischel_1986b#
W. K. Bischel and M. J. Dyer, “Wavelength dependence of the absolute Raman gain coefficient for the Q(1) transition in H2”, J. Opt. Soc. Am. B 3, 677 (1986)
Source record · Catalogue · Review register
Source kind: measurement
Recorded technique: Pulsed pump / cw probe Raman gain (and inverse Raman absorption) on the Q(1) line of normal H2 at 298 K in a 62 cm cell, collimated collinear beams, both lasers single frequency: 532 nm pump (single-frequency doubled YAG, 20 ns) with a 683 nm ring dye probe; 594 nm pulsed dye pump with the 476.5 nm Ar+ probe (inverse Raman, giving the gain at 477 nm); 307 nm (doubled dye) pump with the 351.4 nm Ar+ probe. Pump area from a scanned 0.1 mm aperture (Eq. 1), gain from the time integral of ln(S/S0) (Eq. 3); corrections for the laser linewidth, the pump intensity (inverse Raman) and the density (477 nm, 12.3 amagat), measurements at 20 amagat otherwise (pp. 677-680).
Materials in structured entries: H2
Dataset quantities: dephasing_time, raman_gain, raman_line_shift, raman_shift, raman_transition_polarizability
Contents: 8 datasets; 5 formulas.
Curation notes#
Journal pages 677-682 = PDF pages 1-6 (page n of the PDF is p. 676 + n). Identity checked on the first page. Source id bischel_1986b: bischel_1986 is the same authors’ Phys. Rev. A 33, 3113 (1986) (Ref. 14 here), curated in another extraction.
TABLE 1 (p. 680), ‘Comparison of Measured and Calculated Q(1) Gain Coefficients at 298 K’, gamma in 10^-9 cm/W against the pump wavelength (nm): this work at 532 (2.5 +- 0.4), 477 (3.5 +- 0.3) and 308 (6.6 +- 0.8); previous work at 694 (1.5 +- 0.8, Ref. 8, Bloembergen et al.), 530 (1.8 +- 0.4, Ref. 10, Venkin et al.), 353 (5.0 +- 0.5, Ref. 12, Komine, personal communication) and 265 (5.5 +- 1.6, no footnote: Venkin et al. measured at 530 and 265 nm, p. 677); Eq. (11) at all seven. ‘The error bars listed are our best estimate of the absolute uncertainty in the measured values. They were obtained by adding the standard deviation calculated from the scatter in the data to a reasonable estimate of the systematic error in the measurement technique’ (p. 680): level not stated. The text gives the UV pump as 307 nm (pp. 677, 678, 681) where Table 1 prints 308; Eq. (11) gives 7.05 at 308 nm and 7.09 at 307 nm against the printed 7.06, so 308 is the wavelength of the calculated column. Wavelengths are nominal laser lines (air or vacuum not stated; the difference is below the printed precision). Measured values are the high-density limit: the 532 and 308 nm data at 20 amagat need no density correction, the 477 nm value (inverse Raman at 12.3 amagat) was raised 4 % to the high-density limit (p. 680). The 477 nm and 308 nm values include the laser-linewidth correction (+15 to 30 %, p. 679-680); the 477 nm value is extrapolated to zero pump fluence (Fig. 4).
STATE of the gain datasets (the quantity requires one): recorded as { 21.82 atm, 298 K }, the ideal-gas pressure of 20 amagat at 298 K (the density of the 532 and 308 nm measurements; the temperature of Table 1’s caption). The values are the high-density limit, independent of the density (Eq. 11; p. 681). The previous-work rows carry the same state for comparison only: their own conditions are not given here.
FORMULAS (p. 681): Eq. (11), the room-temperature gain in wavelength, density and temperature (through Delta nu); Eq. (5), the cross section of Bischel and Black (Ref. 20); Eq. (8), the linewidth (reproduced from Ref. 14 = bischel_1986); Eqs. (9)-(10), the line shift. Eq. (11) reproduces Table 1’s calculated column to <= 0.25 % (all seven wavelengths, vacuum or air alike; checked 2026-09-26). Its constant 9.37e6 follows from Eqs. (4) and (5) with R = 0.99, K_B = 0.658, Delta nu = 52 rho MHz and 1 amagat = 2.6868e19 cm^-3: 9.43e6 (0.6 % above; the paper does not give its constants).
TEXT VALUES: the transition polarizabilities ‘alpha_01 = 1.11 x 10^-25 cm^3 and gamma_01 = 0.951 x 10^-25 cm^3 for lambda_p = 500 nm’ (Ref. 22, W. Huo, personal communication, 1983), used for the polarization correction R = 0.99 of Eq. (6) to Eq. (7) (p. 681; the Q-branch average sum_J f_J b_JJ = 0.321 at 298 K) - the datasets alpha01_H2 and gamma01_H2, reproduced; the zero-density transition frequency ‘nu_r(0) = 4155.25 +- 0.01 cm^-1’ (Refs. 28-31, p. 681) - shift_H2, reproduced; the shift coefficient ‘At 298 K, we have measured C = -96 MHz/amagat’ (Ref. 14) - line_shift_H2, reproduced from bischel_1986; ‘D = 0.174 MHz amagat^-2’ (Ref. 26, Murray and Javan, curated as murray_1972: their Q_1(0) coefficient, see the formula) in the formula line_shift_eq9; ‘T2 = 6.1 nsec amagat’ (from Refs. 13-16, p. 679) - T2_H2, reproduced; ‘the room-temperature value of 52 MHz/amagat for the Raman linewidth’ (p. 681, Eq. (8) at 298 K, 51.8 rounded). Also: the dye-laser calibration, ‘For a H2 density of 12.1 amagats, we measured an effective linewidth of 860 MHz where the true linewidth is 650 MHz’ (p. 678), and ‘the Raman linewidth of 1055 MHz at a density of 20 amagats’ (p. 680): both from Eq. (8), not new measurements.
FWHM: ‘Delta nu is the full width at half-maximum Raman linewidth in hertz’ (Eq. 4, p. 680); Eq. (8) is ‘a best-fit formula for the FWHM Raman linewidth Delta nu in megahertz at any temperature and density (rho < 100 amagats)’, including Dicke narrowing (309/rho in MHz amagat) (p. 681).
H2 is normal hydrogen at 298 K (‘K_B ... equal to 0.658 at 298 K for the J = 1 level in H2’, p. 681). Ref. 8 is printed ‘IEEE J. Quantum Electron. QE-3, 197 (1976)’ (Ottusch and Rockwell cite it as 1967): kept as printed.
Recorded bibliographic identity status: VALIDATED_WITH_WARNINGS. This concerns identification of the source; it does not establish the scientific correctness of its contents.
Datasets#
bischel_1986b/gain_H2#
{
"id": "gain_H2",
"material": "H2",
"file": "H2/bischel_1986b__gain_H2.csv",
"table": "tbl_33f36ba412af",
"quantity": "raman_gain",
"unit": "cm/W",
"scale": 1e-09,
"abscissa_unit": "nm",
"state": {
"pressure_atm": 21.82,
"temperature_k": 298.0
},
"density": "ideal",
"use": "primary",
"uncertainty": {
"column": true,
"level": "not stated"
},
"parameters": {
"transition": "v=0-1 Q(1)"
}
}
Table 1 (p. 680), ‘This Work’: the measured steady-state high-density-limit gain of H2 Q(1) at 298 K against the pump wavelength (532 nm gain, 477 nm from inverse Raman absorption, 308 nm gain), sigma the printed +- (the scatter’s standard deviation plus an estimate of the systematic error, level not stated). State: 20 amagat at 298 K (see the record’s notes).
bischel_1986b/gain_previous_H2#
{
"id": "gain_previous_H2",
"material": "H2",
"file": "H2/bischel_1986b__gain_previous_H2.csv",
"table": "tbl_33f36ba412af",
"quantity": "raman_gain",
"unit": "cm/W",
"scale": 1e-09,
"abscissa_unit": "nm",
"state": {
"pressure_atm": 21.82,
"temperature_k": 298.0
},
"density": "ideal",
"use": "reproduced",
"reproduced_from": [
"N. Bloembergen, G. Bret, P. Lallemand, A. Pine and P. Simova, IEEE J. Quantum Electron. QE-3, 197 (1976) (year as printed)",
"G. V. Venkin, L. L. Kulyuk and D. I. Maleev, Kvantovaya Elektron. (Moscow) 2, 2475 (1975) [Sov. J. Quantum Electron. 5, 1348 (1976)]",
"H. Komine, Northrop Research and Technology Center (personal communication, 1983)"
],
"uncertainty": {
"column": true,
"level": "not stated"
},
"parameters": {
"transition": "v=0-1 Q(1)"
}
}
Table 1 (p. 680), ‘Previous Work’: 694 nm (a, Ref. 8, broadband ruby laser, ‘~50%’ quoted error, p. 677), 530 nm (b, Ref. 10), 353 nm (c, Ref. 12, unpublished), 265 nm (no footnote; Ref. 10’s quadrupled line, p. 677). Conditions (density, temperature) not given here; the state is the table’s for comparison only.
bischel_1986b/gain_eq11_H2#
{
"id": "gain_eq11_H2",
"material": "H2",
"file": "H2/bischel_1986b__gain_eq11_H2.csv",
"table": "tbl_33f36ba412af",
"quantity": "raman_gain",
"unit": "cm/W",
"scale": 1e-09,
"abscissa_unit": "nm",
"state": {
"pressure_atm": 21.82,
"temperature_k": 298.0
},
"density": "ideal",
"use": "check",
"parameters": {
"transition": "v=0-1 Q(1)"
}
}
Table 1 (p. 680), gamma_cal from Eq. (11) at 298 K in the high-density limit (Delta nu = 52 rho MHz), reproduced by the formula gain_eq11 to <= 0.25 %.
bischel_1986b/alpha01_H2#
{
"id": "alpha01_H2",
"material": "H2",
"table": "text",
"quantity": "raman_transition_polarizability",
"unit": "cm3",
"scale": 1e-25,
"abscissa_unit": "nm",
"use": "reproduced",
"reproduced_from": [
"W. Huo, NASA Ames Research Center (personal communication, 1983)"
],
"parameters": {
"transition": "v=0-1 Q branch (Q(1))",
"invariant": "mean"
}
}
1 inline points in the source record.
p. 681: ‘Using the values given by Ref. 22 of alpha_01 = 1.11 x 10^-25 cm^3 and gamma_01 = 0.951 x 10^-25 cm^3 for lambda_p = 500 nm’: the isotropic transition polarizability of the v = 0 -> 1 Q-branch transition of H2, in Eq. (6), dsigma/dOmega = (2 pi nu_s)^4 (alpha_01^2 + (4/45) b_JJ gamma_01^2). Rotational state not specified (the Q(1) line is the application). An ab initio value by personal communication.
bischel_1986b/gamma01_H2#
{
"id": "gamma01_H2",
"material": "H2",
"table": "text",
"quantity": "raman_transition_polarizability",
"unit": "cm3",
"scale": 1e-25,
"abscissa_unit": "nm",
"use": "reproduced",
"reproduced_from": [
"W. Huo, NASA Ames Research Center (personal communication, 1983)"
],
"parameters": {
"transition": "v=0-1 Q branch (Q(1))",
"invariant": "anisotropy"
}
}
1 inline points in the source record.
p. 681: gamma_01 = 0.951 x 10^-25 cm^3 at lambda_p = 500 nm (Ref. 22), the anisotropic transition polarizability of the v = 0 -> 1 transition, as alpha01_H2.
bischel_1986b/shift_H2#
{
"id": "shift_H2",
"material": "H2",
"table": "text",
"quantity": "raman_shift",
"unit": "cm-1",
"abscissa": "label",
"use": "reproduced",
"reproduced_from": [
"stoicheff_1957",
"J. V. Foltz, D. H. Rank and T. A. Wiggins, J. Mol. Spectrosc. 21, 208 (1966)",
"P. J. Brannon, C. H. Church and C. W. Peters, J. Mol. Spectrosc. 27, 44 (1968)",
"D. E. Jennings, A. Weber and J. W. Brault, Appl. Opt. 25, 284 (1986)"
],
"uncertainty": {
"column": true,
"level": "not stated"
},
"parameters": {
"transition": "v=0-1 Q(1), zero density"
}
}
1 inline points in the source record.
p. 681: ‘The zero-pressure transition frequency nu_r(0) has been measured [28-31] to be nu_r(0) = 4155.25 +- 0.01 cm^-1’ (the Q(1) line). Level of the +- not stated. A value formed from four papers, not a copy of one. Stoicheff’s (Ref. 28, curated as stoicheff_1957 since 2026-09-27): Q_1(1) = 4155.201 cm-1 at 1-2 atm, ‘about +-0.05’ (its Table I and p. 731), 0.05 below this value, within its accuracy; bischel_1986’s text quotes ‘Stoicheff 4155.207’, his line ‘extrapolated to zero density using Eq. (4)’ (their shift coefficient).
bischel_1986b/line_shift_H2#
{
"id": "line_shift_H2",
"material": "H2",
"table": "text",
"quantity": "raman_line_shift",
"unit": "MHz/amagat",
"abscissa": "none",
"use": "reproduced",
"reproduced_from": [
"bischel_1986"
],
"parameters": {
"transition": "v=0-1 Q(1)",
"perturber": "self",
"temperature_k": 298.0
}
}
1 inline points in the source record.
p. 681: ‘At 298 K, we have measured C = -96 MHz/amagat’ (Ref. 14, Phys. Rev. A 33, 3113, curated as bischel_1986), the linear density coefficient of the Q(1) shift, Eq. (9); its temperature law is Eq. (10) (formula line_shift_eq10).
bischel_1986b/T2_H2#
{
"id": "T2_H2",
"material": "H2",
"table": "text",
"quantity": "dephasing_time",
"unit": "ns amagat",
"abscissa": "none",
"use": "reproduced",
"reproduced_from": [
"W. K. Bischel and M. J. Dyer, in Excimer Lasers-83, C. K. Rhodes, H. Egger and H. Pummer, Eds. (AIP, New York, 1983)",
"bischel_1986",
"A. Owyoung, Opt. Lett. 2, 91 (1978)",
"H. Hunt, W. L. Barnes and P. J. Brannon, Phys. Rev. A 1, 1570 (1970)"
],
"parameters": {
"transition": "v=0-1 Q(1)"
}
}
1 inline points in the source record.
p. 679: ‘We know from Raman linewidth measurements [13-16] that T2 = 6.1 nsec amagat’: the high-density T2 of Q(1) times the density, T2 = 6.1/rho ns (rho in amagat); room temperature. Consistent with T2 = 1/(pi Delta nu) and Delta nu = 52 rho MHz (1/(pi x 52 MHz) = 6.12 ns).
Formulas#
bischel_1986b/gain_eq11#
{
"id": "gain_eq11",
"material": "H2",
"equation": "Eq. (11), p. 681",
"printed": "gamma_g = 9.37 x 10^6 (52 rho/Delta nu) (K_B/0.658) (nu_p - 4155) (7.19 x 10^9 - nu_p^2)^-2",
"variable": "nu_p: the pump frequency in cm^-1; rho: the density in amagat; Delta nu: the FWHM linewidth in MHz from Eq. (8); K_B: the Boltzmann population of J = 1 (0.658 at 298 K); gamma_g in cm/W",
"state": "298 K as printed; other temperatures through Delta nu (Eq. 8) and K_B",
"density": "ideal",
"range": "pump 2000-190 nm, 1-100 amagat, 77-500 K (p. 681)",
"coefficients": {
"C": "9.37e6",
"linewidth_hd_MHz_per_amagat": "52",
"KB_298": "0.658",
"nu_R": "4155",
"nu_i2": "7.19e9"
},
"check": "Reproduces Table 1's calculated column at all seven pump wavelengths to <= 0.25 % with nu_p = 1/lambda (e.g. 532 nm: 2.935 against 2.94; 308 nm: 7.046 against 7.06) (2026-09-26). The constant follows from Eqs. (4)-(5) with R = 0.99 as 9.43e6 (0.6 % high)."
}
The peak steady-state gain of the Q(1) line of normal H2; ‘In the high-density limit, Delta nu = 52 rho MHz, and hence the peak Raman gain is independent of density’ (p. 681). 7.19e9 = nu_i^2 of Eq. (5) (nu_i = 8.48e4 cm^-1). The paper’s recommended formula: ‘correct gain coefficients for use in modeling applications can be calculated from Eq. (11)’ (p. 682).
bischel_1986b/cross_section_eq5#
{
"id": "cross_section_eq5",
"material": "H2",
"equation": "Eq. (5), p. 681",
"printed": "dsigma/dOmega (90 deg) = A nu_s^4/(nu_i^2 - nu_p^2)^2, A = 8.74 x 10^-28 cm^2 sr^-1, nu_i = 8.48 x 10^4 cm^-1",
"variable": "nu_s, nu_p: the Stokes and pump frequencies in cm^-1",
"state": "298 K (the Q-branch thermal average)",
"density": "unknown",
"range": "200-600 nm (Bischel and Black's measurements, Ref. 20)",
"coefficients": {
"A": "8.74e-28",
"nu_i": "8.48e4"
},
"reproduced_from": [
"bischel_1983"
],
"check": "Enters Eq. (11) (with R = 0.99): see gain_eq11."
}
The wavelength dependence of the H2 Q-branch (4155 cm-1) cross section, fitted with a single resonance by the authors (Ref. 20, W. K. Bischel and G. Black, Excimer Lasers-1983, AIP, 1983 = bischel_1983, re-pointed 2026-09-27: A and nu_i are that paper’s Table 1 H2 row, identical): the thermal average over the Q branch for linear pump polarization and no analyser (Eq. 7), multiplied by R = 0.99 to give the Q(1) cross section for parallel pump and Stokes polarizations (Eq. 6).
bischel_1986b/linewidth_eq8#
{
"id": "linewidth_eq8",
"material": "H2",
"equation": "Eq. (8), p. 681",
"printed": "Delta nu = (309/rho) (T/298)^0.92 + [51.8 + 0.152 (T - 298) + 4.85 x 10^-4 (T - 298)^2] rho",
"variable": "rho: the density in amagat; T: the temperature in K; Delta nu: the FWHM in MHz",
"state": "T as the variable",
"density": "ideal",
"range": "rho < 100 amagat (the text); 1-50 amagat, 77-500 K (p. 682)",
"coefficients": {
"A": "309",
"n_A": "0.92",
"B0": "51.8",
"B1": "0.152",
"B2": "4.85e-4",
"T0": "298"
},
"check": "At 298 K and 20 amagat gives 1051 MHz against the text's 1055 MHz at 20 amagat (p. 680); at 12.1 amagat 652 MHz against 'the true linewidth is 650 MHz' (p. 678) (2026-09-26)."
}
The Q(1) FWHM of normal H2 with the Dicke term, reproduced from Ref. 14 (bischel_1986, Phys. Rev. A 33, 3113), the original. The temperature exponent 0.92 applies to the Dicke term. Ottusch and Rockwell’s H2 law (ottusch_1988 linewidth_H2) is this at 298 K.
bischel_1986b/line_shift_eq9#
{
"id": "line_shift_eq9",
"material": "H2",
"equation": "Eq. (9), p. 681",
"printed": "nu_r(rho) = nu_r(0) + C rho + D rho^2; nu_r(0) = 4155.25 +- 0.01 cm^-1; C = -96 MHz/amagat at 298 K; D = 0.174 MHz amagat^-2",
"variable": "rho: the density in amagat",
"state": "298 K",
"density": "ideal",
"range": "the second-order term needed above 100 amagat (p. 681)",
"coefficients": {
"nu0_cm1": "4155.25",
"C_MHz_per_amagat": "-96",
"D_MHz_per_amagat2": "0.174"
},
"check": "Not a fit of this paper's data: its terms are quoted (nu_r(0) from Refs. 28-31, C from Ref. 14, D from Ref. 26)."
}
Reproduced: D from J. R. Murray and A. Javan, J. Mol. Spectrosc. 42, 1 (1972) (Ref. 26), curated as murray_1972 (2026-09-27). FINDING: 0.174 MHz amagat^-2 is Murray and Javan’s quadratic-fit b of the Q_1(0) line (0.0058 x 10^-3 cm-1/amagat^2, their Table III); their Q_1(1) b is 0.0045 x 10^-3 = 0.135 MHz amagat^-2 (bischel_1986’s Table II prints both, on their own lines). This Q(1) law therefore carries the Q(0) quadratic coefficient; at 100 amagat the difference is 390 MHz (0.013 cm-1).
bischel_1986b/line_shift_eq10#
{
"id": "line_shift_eq10",
"material": "H2",
"equation": "Eq. (10), p. 681",
"printed": "C = [nu_r(rho) - nu_r(0)] rho^-1 = [-96.1 + 0.777 (T - 298) - 8.82 x 10^-4 (T - 298)^2]",
"variable": "T: the temperature in K; C in MHz/amagat",
"state": "T as the variable",
"density": "ideal",
"range": "densities below 100 amagat (p. 681); 77-500 K",
"coefficients": {
"C0": "-96.1",
"C1": "0.777",
"C2": "-8.82e-4",
"T0": "298"
},
"check": "At 298 K gives -96.1 MHz/amagat, the text's C = -96 (2026-09-26)."
}
The temperature law of the Q(1) shift coefficient, reproduced from Ref. 14 (bischel_1986).
Corrections#
No dataset errata are recorded in this source record.
Formula corrections, where recorded, appear with their formulas above. Curation notes may also discuss corrections or unresolved interpretation. Consult the review register for the checks and decisions.