Commit 2cf4bfcc by Parameswaran Ajith

added the tutorial material - chapter 1.

parents
Showing with 1831 additions and 0 deletions
@misc{mock-gw-data,
url = "home.icts.res.in/~ajith/Downloads/mock_gw_data.dat.gz"
}
@misc{ligo-data,
note = "Download the file L1-STRAIN\_4096Hz-815045078-256.txt.gz from",
url = "http://www.ligo.org/science/GRB051103/index.php"
}
@misc{rxte,
note = "RXTE is an X-ray timing satellite",
url = "https://heasarc.gsfc.nasa.gov/docs/xte/rxte.html"
}
@misc{rxte-data,
url = "http://home.icts.res.in/~ajith/Downloads/extracted_lightcurve_HerX-1.dat.gz"
}
@misc{rxte-data2,
url = "http://home.icts.res.in/~ajith/Downloads/4U1636-536_LC-extract.dat.gz"
}
@misc{nrdata,
url = "http://home.icts.res.in/~ajith/Downloads/nr_data.gz"
}
@misc{SXScatalog,
url = "http://www.black-holes.org/waveforms/"
}
@article{Porto:2010zg,
author = "Porto, Rafael A. and Ross, Andreas and Rothstein, Ira Z.",
title = "{Spin induced multipole moments for the gravitational
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journal = "JCAP",
volume = "1103",
pages = "009",
doi = "10.1088/1475-7516/2011/03/009",
year = "2011",
eprint = "1007.1312",
archivePrefix = "arXiv",
primaryClass = "gr-qc",
}
@article{Ajith:2011ec,
author = "Ajith, P.",
title = "{Addressing the spin question in gravitational-wave
searches: Waveform templates for inspiralling compact
binaries with nonprecessing spins}",
journal = "Phys. Rev. D",
volume = "84",
pages = "084037",
year = "2011",
eprint = "1107.1267",
archivePrefix = "arXiv",
primaryClass = "gr-qc",
}
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year = "2011",
note = "* Temporary entry *",
eprint = "1101.1459",
archivePrefix = "arXiv",
primaryClass = "gr-qc",
}
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}
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}
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}
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}
@Article{Ajith:2007qp,
author = "Ajith, Parameswaran and others",
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waveforms",
journal = "Class. Quant. Grav.",
volume = "24",
year = "2007",
pages = "S689--S699",
eprint = "",
SLACcitation = "%%CITATION = ARXIV:0704.3764;%%"
}
% eprint = "arXiv:0704.3764 [gr-qc]",
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}
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}
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}
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journal = {\apj},
keywords = {EQUATIONS OF STATE, PULSARS, RELATIVITY, STELLAR EVOLUTION, STELLAR MODELS, STELLAR ROTATION, ANGULAR MOMENTUM, BLACK HOLES (ASTRONOMY), COMPUTATIONAL GRIDS, COMPUTERIZED SIMULATION, EQUILIBRIUM METHODS, NUMERICAL ANALYSIS, STABILITY, STELLAR MASS},
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}
@UNPUBLISHED{Ajith:2011xx,
author = "Ajith, P.",
title = "Comparison of post-Newtonian templates for gravitational waveforms from spinning binaries",
year = "2011",
note = "{In preparation.}"
}
@article{0264-9381-27-8-084006,
author={Gregory M Harry and the LIGO Scientific Collaboration},
title={Advanced LIGO: the next generation of gravitational wave detectors},
journal={Classical and Quantum Gravity},
volume={27},
number={8},
pages={084006},
url={http://stacks.iop.org/0264-9381/27/i=8/a=084006},
year={2010},
abstract={The Advanced LIGO gravitational wave detectors are next generation instruments which will replace the existing initial LIGO detectors. They are currently being constructed and installed. Advanced LIGO strain sensitivity is designed to be about a factor 10 better than initial LIGO over a broad band and usable to 10 Hz, in contrast to 40 Hz for initial LIGO. This is expected to allow for detections and significant astrophysics in most categories of gravitational waves. To achieve this sensitivity, all hardware subsystems are being replaced with improvements. Designs and expected performance are presented for the seismic isolation, suspensions, optics and laser subsystems. Possible enhancements to Advanced LIGO, either to resolve problems that may arise and/or to allow for improved performance, are now being researched. Some of these enhancements are discussed along with some potential technology being considered for detectors beyond Advanced LIGO.}
}
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archivePrefix = "arXiv",
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doi = "10.1088/0264-9381/27/24/245007",
SLACcitation = "%%CITATION = 1005.5560;%%"
}
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}
%
% Note: Encoded in UTF-8! To use with TeX, adapt the encoding
% (with tools 'recode' or 'iconv') or use the ucs package
% (http://ctan.tug.org/tex-archive/macros/latex/contrib/unicode/)
%
@Article{Allen:2004gu,
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@Article{Ajith:2009fz,
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\title{ICTS Graduate Course: Numerical Methods (PHY410.5)}
\author{P.~Ajith}\email{ajith@icts.res.in}
\author{Prayush Kumar}\email{prayush@icts.res.in}
\affiliation{International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bangalore 560089, India.}
\bigskip
\date{\today}
\maketitle
\section{Numerical differentiation}
\input{diff.tex}
%\section{Lab 2}
%\input{rest.tex}
\bibliography{Lab}
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\subsection{Finite differencing, convergence, error estimates}
We derived the following finite-differencing approximants for the derivative of a function $f(x)$:
\begin{eqnarray}
\mathit{Forward~differencing:} & f'(x) \simeq \frac{f(x+h)-f(x)}{h} + \mathcal{O}\,(h) \\
\mathit{Backward~differencing:} & f'(x) \simeq \frac{f(x)-f(x-h)}{h} + \mathcal{O}\,(h) \\
\mathit{Central~differencing:} & f'(x) \simeq \frac{f(x+h)-f(x-h)}{2h} + \mathcal{O}\,(h^2)
\end{eqnarray}
\subsubsection*{Problems:}
\begin{enumerate}
\item Write a Python function to compute derivatives using these three finite differencing methods. Compute the derivative of the function $f(x) = e^x \, \sin(x)$ over the range $x = [0, 2\pi]$. Plot the numerically computed derivative $f_{(h)}'(x)$ for three different values of $h$.
\item Plot the error $\Delta f_{h}'(x) := |f_{h}'(x) - f'(x)|$ for three different values of $h$, and estimate the order of convergence $n$ of each finite-difference approximation. Plot $n(x)$, where
\begin{equation}
n(x) = \log_2 \frac{f'_{4h}(x) - f'_{2h}(x)}{f'_{2h}(x) - f'_{h}(x)}
\label{eq:order_convg}
\end{equation}
\item Reduce the step size $h$ successively. At what value of $h$ does the round-off error dominate the error budget?
%\item Derive a central differencing approximant for the first derivative $f'(x)$ that is accurate to $\mathcal{O}(h^4)$.
\end{enumerate}
\subsection{Richardson extrapolation}
We have seen that, if the order of the error in the numerical estimate of a function $f(x)$ is known, Richardson extrapolation provides a powerful way of improving the accuracy of the estimate. If we have two numerical estimates $f_{h}(x)$ and $f_{2h}(x)$ each having an error of $\mathcal{O}\,h^k$, a better estimate is given by
\begin{equation}
f(x) \simeq \frac{2 ~ 2^k\, f_{h}(x) - f_{2h}(x)}{2\,2^k -1 } + \mathcal{O}\,(h^{l}),
\end{equation}
where $l$ is the next-to-leading-order error term (for e.g., $l = k+2$ for central differencing, while $l = k+1$ for forward/backward differencing).
\subsubsection*{Problems:}
\label{sec:BBH_nr_data_fd}
\begin{enumerate}
\item Gravitational-waves (GWs) have two independent polarization states -- called ``plus'' and ``cross'' states. GW signals from the coalescence of black-hole binaries, in the simplest case, are circularly polarized:
\begin{eqnarray}
h_+(t) & = A(t) \, \cos \varphi(t), ~~~ h_\times(t) & = A(t) \, \sin \varphi(t).
\end{eqnarray}
Download the data file~\cite{nrdata} containing $h_+(t)$ and $h_\times(t)$. (This is the reduced form of the data produced by a numerical-relativity simulation of black-hole binaries performed by the SXS collaboration and is publicly available at~\cite{SXScatalog}). Compute the phase evolution $\varphi(t)$, the frequency evolution $\omega(t) := d\varphi(t)/dt$ and the rate of change of frequency $\dot{\omega}(t) := d\omega(t)/dt$ using second-order central difference approximation.
\item Estimate the order of convergence of the numerical computation of $\omega(t)$ and $\dot{\omega}(t)$.
\item Perform an extrapolation of $\omega(t)$ and $\dot{\omega}(t)$ to the next order using estimates of two different time-resolutions.
\item Derive an explicit expression for $f'(x)$ with error $\mathcal{O}(h^4)$ using Richardson extrapolation. This is the fourth-order finite differencing approximant for the derivative, which we will use later.
\end{enumerate}
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