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Adds residual gas damping and additional molecular species to the residual gas calculations. The gas scattering and gas damping are now tracked separately for each species in an excess gas sub-budget. The damping calculation is done in the infinite volume limit by default but adds corrections for squeezed film damping if specified in the yaml file. H2, N2, H2O, and O2 are considered. The numbers for aLIGO are taken from the link in this commit. The numbers for Aplus and Voyager are copied from aLIGO. For the existing LIGO facilities the O2 numbers are unknown but are suspected to be low, and are therefore set 10x below the expected noise floor. Closes #63.
Adds residual gas damping and additional molecular species to the residual gas calculations. The gas scattering and gas damping are now tracked separately for each species in an excess gas sub-budget. The damping calculation is done in the infinite volume limit by default but adds corrections for squeezed film damping if specified in the yaml file. H2, N2, H2O, and O2 are considered. The numbers for aLIGO are taken from the link in this commit. The numbers for Aplus and Voyager are copied from aLIGO. For the existing LIGO facilities the O2 numbers are unknown but are suspected to be low, and are therefore set 10x below the expected noise floor. Closes #63.
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ifo.yaml 11.92 KiB
# GWINC aLIGO interferometer parameters
#
# parameters for quad pendulum suspension updated 3rd May 2006, NAR
# References:
# LIGO-T000012-00-D
# * Differentiate between silica and sapphire substrate absorption
# * Change ribbon suspension aspect ratio
# * Change pendulum frequency
# References:
# 1. Electro-Optic Handbook, Waynant & Ediger (McGraw-Hill: 1993)
# 2. LIGO/GEO data/experience
# 3. Suspension reference design, LIGO-T000012-00
# 4. Quartz Glass for Optics Data and Properties, Heraeus data sheet,
# numbers for suprasil
# 5. Y.S. Touloukian (ed), Thermophysical Properties of Matter
# (IFI/Plenum,1970)
# 6. Marvin J. Weber (ed) CRC Handbook of laser science and technology,
# Vol 4, Pt 2
# 7. R.S. Krishnan et al.,Thermal Expansion of Crystals, Pergamon Press
# 8. P. Klocek, Handbook of infrared and optical materials, Marcel Decker,
# 1991
# 9. Rai Weiss, electronic log from 5/10/2006
# 10. Wikipedia online encyclopedia, 2006
# 11. D.K. Davies, The Generation and Dissipation of Static Charge on
# dielectrics in a Vacuum, page 29
# 12. Gretarsson & Harry, Gretarsson thesis
# 13. Fejer
# 14. Braginsky
#
# Updated numbers March 2018: LIGO-T1800044
Infrastructure:
Length: 3995 # m
Temp: 290 # K
ResidualGas:
H2:
BeamtubePressure: 2.7e-7 # Pa
ChamberPressure: 2.7e-7 # Pa
mass: 3.35e-27 # kg; Mass of H_2 (ref. 10)
polarizability: 7.8e-31 # m^3
N2:
BeamtubePressure: 1.33e-8
ChamberPressure: 1.33e-8
mass: 4.65e-26
polarizability: 1.71e-30
H2O:
BeamtubePressure: 1.33e-8
ChamberPressure: 1.33e-8
mass: 2.99e-26
polarizability: 1.50e-30
O2:
BeamtubePressure: 1e-9
ChamberPressure: 1e-9
mass: 5.31e-26
polarizability: 1.56e-30
TCS:
# The presumably dominant effect of a thermal lens in the ITMs is an increased
# mode mismatch into the SRC, and thus an increased effective loss of the SRC.
# The increase is estimated by calculating the round-trip loss S in the SRC as
# 1-S = |<Psi|exp(i*phi)|Psi>|^2, where
# |Psi> is the beam hitting the ITM and
# phi = P_coat*phi_coat + P_subs*phi_subs
# with phi_coat & phi_subs the specific lensing profiles
# and P_coat & P_subst the power absorbed in coating and substrate
#