\documentclass[a4paper,12pt,openright,titlepage]{scrbook}
\usepackage[a4paper,top=3cm,bottom=3cm]{geometry}
\usepackage[T1]{fontenc}
\usepackage[utf8]{inputenc} 
\usepackage{palatino}
\usepackage[english]{babel} 
\usepackage{graphicx}
\usepackage[font=small,hang]{caption}
\usepackage{subfigure}
\usepackage{array}
\usepackage{color}
\usepackage{colortbl}
\usepackage{verbatim}
\usepackage{lscape}
\usepackage{amsmath,amssymb}
\linespread{2}
\title{Innovative perspectives for seismic isolation of gravitational waves detectors}
\author{Myself}
\date{}
\titlehead{A Thesis submitted for the degree of Doctor of Philosophy}
\publishers{School of Something\\University of Somewhere}

\begin{document}
\maketitle

\frontmatter
\tableofcontents

\chapter{Statement of originality}

\chapter{Abstract}

A brief summary of the project goes here, with main results.

\chapter{Introduction}
An introduction to frame the work and structure of the thesis go here.

\chapter{Notations}
Useful notations, constants and formulas go here.\\
Speed of light:\\
$c = 3 \times 10^8$ m/s\\
Gravitational constant:\\
$G = 6,67 \time 10^{-11}$ Nm$^2$/Kg$^2$\\
Gravitational wave amplitude:\\
$h \sim 10^{-21} $ $1/\sqrt{Hz}$\\
Solar mass:\\
$M_{\odot} = 10^{33}$ g

\chapter{Acronyms}
aLIGO = Advanced Laser Interferometric Gravitational-wave Observatory\\
BS = Beam Splitter\\
BSC = Basic Symmetric Chamber\\
BH = Black Hole\\
CARM = Common Arm length\\
CP = Compensation Plate\\
CPS = Capacitive Position Sensors\\
DARM = Differential Arm Length\\
ETM = End Test Mass\\
FIR = Finite Impulse Response\\
HAM = Horizontal Access Module\\
HEPI = Hydraulic External Pre-Isolator\\
HP = High Pass filter\\
ISI = Internal Seismic Isolation\\
ITM = Input Test Mass\\
LHO = LIGO Hanford Observaotry\\
LLO = LIGO Livingston Observatory\\
LP = Low Pass filter\\
LSC = Length Sensing and Control\\
MICH = Michelson length\\
NS = Neutron Star\\
PD = PhotoDiode\\
PR = Power Recycling\\
PRCL = Power Recycling Cavity Length\\
SC = Sensor Correction\\
SR = Signal Recycling\\
SRCL = Signal Recycling Cavity Length\\

\mainmatter

\include{Ch.1}

\include{Ch.2}

\include{Ch.3}

\include{Ch.4}

%\include{Ch.5}
%
%\include{Ch.6}
%
%\include{Ch.7}

\appendix
\include{A}
\include{B}

\backmatter

\listoffigures
\listoftables

\begin{thebibliography}{}

\bibitem{wei} S. Weinberg \textit{Gravitation and Cosmology: principles and applications of the General Theory of Relativity}, John Wiley \& Sons, Inc., 1972

\bibitem{nar} J. V. Narlikar \textit{An introduction to Relativity}, Cambridge University Press, 2011

\bibitem{mag} M. Maggiore \textit{Gravitational waves - Vol. 1: Theory and Experiments}, Oxford University Press, 2013

\bibitem{first} B. P. Abbott, \textit{Observation of Gravitational Waves from a Binary Black Hole Merger}, Phys. Rev. Lett. 116, 061102, 2016 

\bibitem{ligo} Advanced LIGO Systems Group, \textit{Advanced LIGO Systems Design}, DCC document T010075-v3, 2017

\bibitem{abb} B. P. Abbott et al, \textit{GW150914: The Advanced LIGO Detectors in the Era of First Discoveries}, Phys. Rev. Lett. 116, 131102, 2016

\bibitem{mar} D. Martynov et al., \textit{The Sensitivity of the Advanced LIGO Detectors at the
Beginning of Gravitational Wave Astronomy}

\bibitem{mat} F. Matichard et al, \textit{Seismic isolation of Advanced LIGO: Review of strategy, instrumentation and performance}, Class. Quantum Grav. 32 185003, 2015

\bibitem{lsc} K. Izumi, D. Sigg, \textit{Advanced LIGO: length sensing and control in a dual recycled interferometric gravitational wave antenna}, 2017 Class. Quantum Grav. 34 015001

\end{thebibliography}

\chapter{Acknowledgements}

\end{document}