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From MIT coating thermal noise experiment results: * https://dcc.ligo.org/LIGO-G2000880 and LMA 2020 paper: * https://iopscience.iop.org/article/10.1088/1361-6382/ab77e9
From MIT coating thermal noise experiment results: * https://dcc.ligo.org/LIGO-G2000880 and LMA 2020 paper: * https://iopscience.iop.org/article/10.1088/1361-6382/ab77e9
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ifo.yaml 11.50 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:
pressure: 4.0e-7 # Pa
mass: 3.35e-27 # kg; Mass of H_2 (ref. 10)
polarizability: 7.8e-31 # m^3
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
#
# This expression can be expanded to 2nd order and is given by
# S= s_cc P_coat^2 + 2*s_cs*P_coat*P_subst + s_ss*P_subst^2
# s_cc, s_cs and s_ss were calculated analytically by Phil Willems (4/2007)
s_cc: 7.024 # Watt^-2
s_cs: 7.321 # Watt^-2
s_ss: 7.631 # Watt^-2
# The hardest part to model is how efficient the TCS system is in
# compensating this loss. Thus as a simple Ansatz we define the
# TCS efficiency TCSeff as the reduction in effective power that produces
# a phase distortion. E.g. TCSeff=0.99 means that the compensated distortion
# of 1 Watt absorbed is equivalent to the uncompensated distortion of 10mWatt.
# The above formula thus becomes:
# S= s_cc P_coat^2 + 2*s_cs*P_coat*P_subst + s_ss*P_subst^2 * (1-TCSeff)^2
#
# To avoid iterative calculation we define TCS.SCRloss = S as an input
# and calculate TCSeff as an output.
# TCS.SRCloss is incorporated as an additional loss in the SRC
SRCloss: 0.00
Seismic:
Site: 'LHO' # LHO or LLO (only used for Newtonian noise)