This is a mod of the AAK waveform in EMRI Kludge Suite (version 0.5.0) [1,2,3] https://github.com/alvincjk/EMRI_kludge_Suite. It computes quadrapole included augmented analytic kludge (QAAK) [4] waveforms for extreme-mass-ratio inspirals (EMRIs), where the system could possess arbitrary quadrapole moment deviation from Kerr value. The orbital frequency deviations caused by arbitrary quadrupoles are evaluated by the method in [5]. Note that the current version has removed the usage of AAK TDIs, AAK phases, Python interface of EMRI Kludge Suite.
— Miaoxin Liu, July 2021
Main:
src/exec/AAK_Waveform.ccCalculate the orbital frequency deviations from Kerr value, which correct the AAK mapping.src/inclecc/GKR.ccQuadrupole corrections in NK.src/suite/KSParMap.ccQuadrupole corrections in 3pn AK; The quadrupole won't be mapped to an unphysical value like spin in AAK mapping.src/suite/AAK.ccQuadrupole is included when calling the 3pn AK functions in KSParMap.cc.src/suite/GKTrajFast.ccQuadrupole is included when calling the GKR.src/suite/KSTools.ccThe quadrupole deviation from Kerr value q_q is added as an additional input parameter.
These header files are also modified:
include/AAK.hinclude/GKR.hinclude/GKTrajFast.hinclude/KSParMap.hinclude/KSTools.h
The following files have nothing to do with QAAK waveform, modified to avoid errors:
src/exec/AAK_Phase.ccsrc/exec/AAK_TDI.ccsrc/inclecc/GKTrajcc.ccsrc/suite/AAKPhase.ccsrc/suite/AAKpy.ccsrc/suite/AAKTDI.cc
- Orbital frequency deviations may be NaNs when p is too small, but it is safe for the position where they are needed to correct the mappings.
Miaoxin Liu
School of Physics and Astronomy, Sun Yat-sen University
liumx37@mail2.sysu.edu.cn
Jian-dong Zhang
TianQin Research Center for Gravitational Physics
zhangjd9@mail.sysu.edu.cn
We thank Alvin J. K. Chua and Yiming Hu for helpful discussion. This code makes use of the Black Hole Perturbation Toolkit.
[1] A. J. K. Chua & J. R. Gair. Improved analytic extreme-mass-ratio inspiral model for scoping out eLISA data analysis. Class. Quantum Grav. 32:232002, 2015.
[2] A. J. K. Chua, C. J. Moore & J. R. Gair. Augmented kludge waveforms for detecting extreme-mass-ratio inspirals. Physical Review D 96:044005, 2017.
[3] S. Babak, H. Fang, J. R. Gair, K. Glampedakis & S. A. Hughes. "Kludge" gravitational waveforms for a test-body orbiting a Kerr black hole. Physical Review D 75:024005, 2007.
[4] M. Liu & J. Zhang. Augmented analytic kludge waveform with quadrupole moment correction. e-Print: 2008.11396.
[5] S. J. Vigeland & S. A. Hughes. Spacetime and orbits of bumpy black holes. Physical Review D 81:024030, 2010.