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Index: docs/paper/introduction.tex
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@@ -1,90 +1,90 @@
\section{Introduction}
\label{sec:introduction}
Decays of unstable heavy particles to multibody final states can in general occur through several different intermediate resonances.
Each decay channel can be represented quantum-mechanically by an amplitude, and the total density of decays across the phase space is represented by the square of the coherent sum of all contributing amplitudes.
Interference effects can lead to excesses or deficits of decays in regions of phase space where different resonances overlap.
Investigations of such dynamical effects in multibody decays are of great interest to test the Standard Model of particle physics and to investigate resonant structures.
The Dalitz plot (DP)~\cite{Dalitz:1953cp,Fabri:1954zz} was introduced originally to describe the phase space of $\KL \to \pi\pi\pi$ decays, but is relevant for the decay of any spin-zero particle to three spin-zero particles, $P \to d_{1} d_{2} d_{3}$.
In such a case, energy and momentum conservation give
\begin{equation}
m_P^2 + m_{d_{1}}^2 + m_{d_{2}}^2 + m_{d_{3}}^2 =
m^2(d_{1}d_{2}) + m^2(d_{2}d_{3}) + m^2(d_{3}d_{1}) \, ,
\end{equation}
where $m(d_id_j)$ is the invariant mass obtained from the two-body combination of the $d_i$ and $d_j$ four momenta.
Consequently, assuming that the masses of $P$, $d_1$, $d_2$ and $d_3$ are all known, any two of the $m^2(d_id_j)$ values -- subsequently referred to as Dalitz-plot variables -- are sufficient to describe fully the kinematics of the decay in the $P$ rest frame.
This can also be shown by considering that the 12 degrees of freedom corresponding to the four-momenta of the three final-state particles are accounted for by two DP variables, the three $d_i$ masses, four constraints due to energy-momentum conservation in the $P \to d_{1} d_{2} d_{3}$ decay, and three co-ordinates describing a direction in space which carries no physical information about the decay since all particles involved have zero spin.
A Dalitz plot is then the visualisation of the phase space of a particular three-body decay in terms of the two DP variables.\footnote{
The phrase ``Dalitz plot'' is often used more broadly in the literature.
In particular, it can be used to describe the projection onto two of the two-body invariant mass combinations of a three-body decay even when one or more of the particles involved has non-zero spin.
}
Analysis of the distribution of decays across a DP can reveal information about the underlying dynamics of the particular three-body decay, since the differential rate is
\begin{equation}
d\Gamma = \frac{1}{(2\pi)^3}\frac{1}{32\,m_P^3}\left| {\cal A} \right|^2 dm^2(d_{1}d_{3}) \, dm^2(d_{2}d_{3}) \, ,
\end{equation}
where ${\cal A}$ is the amplitude for the three-body decay.
Thus, any deviation from a uniform distribution is due to the dynamical structure of the amplitude.
Examples of the kinematic boundaries of a DP, and of resonant structures that may appear in this kind of decay, are shown in Fig.~\ref{fig:dpexample}.
\begin{figure}[!htb]
\centering
\includegraphics[width=0.49\textwidth]{figures/dalitz.pdf}
\includegraphics[width=0.49\textwidth]{figures/DP.pdf}\\
\includegraphics[width=0.32\textwidth]{figures/m12Sq.pdf}
\includegraphics[width=0.32\textwidth]{figures/m13Sq.pdf}
\includegraphics[width=0.32\textwidth]{figures/m23Sq.pdf}
\caption{
(Top left) kinematic boundaries of the three-body phase space for the decay $\Bs\to\Dzb\Km\pip$.
The insets indicate the configuration of the final-state particle momenta in the parent rest frame at various different DP positions.
(Top right) examples of the resonances which may appear in the Dalitz
plot for this decay: (red) $\D^*_2(2573)^-$, (orange) $\kaon^*(892)^0$,
(green) $\kaon\pion$ S-wave.
(Bottom) projections of this DP onto the squares of the invariant masses (from left to right): $m^2_{\Dzb\Km}$, $m^2_{\Dzb\pip}$, $m^2_{\Km\pip}$.
}
\label{fig:dpexample}
\end{figure}
The Dalitz-plot analysis technique, usually implemented with model-dependent descriptions of the amplitudes involved, has been used to understand hadronic effects in, for example, the $\pi^0\pi^0\pi^0$ system produced in $p\bar{p}$ annihilation~\cite{Amsler:1995bf}.
Recently, it has also been used to study three-body $\eta_c$ decays~\cite{Lees:2014iua,Lees:2015zzr}.
However, DP analyses have become particularly popular to study multibody decays of the heavy-flavoured $D$ and $B$ mesons.
Not only do the relatively large masses of these particles provide a broad kinematic range in which resonant structures can be studied but, since the decays are mediated by the weak interaction, there may be \CP-violating differences between the DP distributions for particle and antiparticle.
Studying these differences can test the Standard Model mechanism for \CP violation: if the asymmetries are not consistent with originating from the single complex phase in the Cabibbo-Kobayashi-Maskawa (CKM) quark mixing matrix~\cite{Cabibbo:1963yz,Kobayashi:1973fv} then contributions beyond the Standard Model must be present.
% as predicted for certain decay modes in various theories.
Until around the year 2000, most DP analyses of charm decays were focussed on understanding hadronic structures at low $\pi\pi$ or $K\pi$ mass.
In particular, pioneering analyses of $D \to K\pi\pi$ decays were carried out by experiments such as MARK-II, MARK-III, E687, ARGUS, E691 and CLEO~\cite{Schindler:1980ws,Adler:1987sd,Anjos:1992kb,Albrecht:1993jn,Frabetti:1994di,Kopp:2000gv}.
These analyses revealed the existence of a broad structure in the $K\pi$ S-wave that could not be well described with a Breit--Wigner lineshape.
In later analyses, it was shown that this contribution could be modelled in a quasi-model-independent way, in which the partial wave is fitted using splines to describe the magnitude and phase as a function of $m(K\pi)$~\cite{Aitala:2005yh}.
Subsequent uses of this approach include further studies of the $K\pi$ S-wave~\cite{Bonvicini:2008jw,Link:2009ng,delAmoSanchez:2010fd,Lees:2015zzr} as well as the $\Kp\Km$~\cite{Aubert:2007dc} and $\pip\pim$~\cite{Aubert:2008ao} S-wave{s}, in various processes.
Similarly, DP analyses of decays such as $\Dp \to \pip\pip\pim$~\cite{Aitala:2000xu,Muramatsu:2002jp,Link:2003gb,Bonvicini:2007tc} indicated the existence of a broad low-mass $\pi\pi$ S-wave known as the $\sigma$ pole~\cite{Pelaez:2015qba}.
With the advent of the $e^+e^-$ \B-factory experiments, \babar~\cite{Aubert:2001tu,TheBABAR:2013jta} and Belle~\cite{Abashian:2000cg}, DP analyses of \B meson decays became feasible.
The method was used to obtain insights into charm resonances through analyses of $\Bp\to \Dm\pip\pip$~\cite{Abe:2003zm,Aubert:2009wg} and $\Bz \to \Dzb\pip\pim$~\cite{Kuzmin:2006mw,delAmoSanchez:2010ad} decays.
Studies of \B meson decays to final states without any charm or charmonium particles also became possible~\cite{Garmash:2004wa,Aubert:2005sk,Aubert:2005ce}.
-Once baseline DP models were established, it was then possible to search for \CP violation effects, with results including the first evidence for \CP violation in the $\Bp \to \rho^0 \Kp$ decay~\cite{Garmash:2005rv,Aubert:2008bj}.
+Once baseline DP models were established, it was then possible to search for \CP violation effects, with results including the first evidence for \CP violation in the $\Bp \to \rho(770)^0 \Kp$ decay~\cite{Garmash:2005rv,Aubert:2008bj}.
Moreover, analyses that accounted for possible dependence of the \CP violation effect with decay time as well as with DP position were carried out for both $D$~\cite{Asner:2005sz,Abe:2007rd} and $B$ decays~\cite{Aubert:2007jn,Kusaka:2007dv,Kusaka:2007mj,Aubert:2007sd,:2008wwa,Aubert:2009me,Nakahama:2010nj,Lees:2013nwa}.
With the availability of increasingly large data samples at these experiments and, more recently, at the Large Hadron Collider experiments (in particular, LHCb~\cite{Alves:2008zz}), more detailed studies of these and similar decays become possible.
In addition, many ideas for DP analyses have been proposed, since they provide interesting possibilities to provide insight into hadronic structures, to measure \CP violation effects and to test the Standard Model.
These include methods to determine the angles $\alpha$, $\beta$ and $\gamma$ of the CKM Unitarity Triangle with low theoretical uncertainty from, respectively $\Bz \to \pip\pim\piz$~\cite{Snyder:1993mx}, $\Bz \to D\pip\pim$~\cite{Charles:1998vf,Latham:2008zs} and $\Bz \to D\Kp\pim$ decays~\cite{Gershon:2008pe,Gershon:2009qc}, among many other potential analyses.
Thus, it has become increasingly important to have a publicly available Dalitz-plot analysis package that is flexible enough both to be used in a range of experimental environments and to describe many possible different decays and types of analyses.
Such a package should be well validated and have excellent performance characteristics, in particular in terms of speed since complicated amplitude fits can otherwise have unacceptable CPU requirements.
This motivated the creation, and ongoing development, of the \laura\ package, which is described in the remainder of the paper.
\laura\ is written in the \cpp\ programming language and is intended to be as close as possible to being a standalone package, with a sole external dependency on the \root\ package~\cite{Brun:1997pa}.
In particular, \root\ is used to handle histogrammed quantities, and to implement minimisation of negative log-likelihood functions with \minuit~\cite{James:1975dr}.
Further documentation and code releases, distributed under the Boost Software License~\cite{boost}, are available from
\begin{center}
\href{http://laura.hepforge.org/}{\tt http://laura.hepforge.org/} \, .
\end{center}
The description of the software given in this paper corresponds to that
released in \laura\ version {\tt v3r2}.
In Sec.~\ref{sec:DalitzGeneralities}, a brief summary of the Dalitz-plot analysis formalism is given, and the conventions used in \laura\ are set out.
Section~\ref{sec:expt-effects} describes effects that must also be taken into account when performing an experimental analysis.
Sections~\ref{sec:signal},~\ref{sec:eff-resol} and~\ref{sec:backgrounds} then contain discussions of, respectively, the implementation of the signal model, efficiency and resolution effects, and the background components in \laura, including explicit classes and methods with high-level details given in Appendices.
These elements are then put together in Sec.~\ref{sec:workflow}, where the overall work flow in \laura\ is described.
The performance of the software is discussed in Sec.~\ref{sec:performance}, ongoing and planned future developments are briefly mentioned in Sec.~\ref{sec:future-devel}, and a summary is given in Sec.~\ref{sec:summary}.
Index: docs/paper/res-formulae.tex
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\section{Formulae for available lineshapes}
\label{sec:res-formulae}
This section presents the complete formulae for all resonance shapes implemented
in \laura. Table~\ref{tab:resForms} gives the list of shapes, together with
the corresponding \texttt{LauResonanceModel} enumeration integer that is required to
specify the resonance type for the \texttt{LauIsobarDynamics addResonance} function, as
well as the equation number(s) that provide the expression for the resonance
mass term $R(m)$ used in Eq.~(\ref{eq:ResDynEqn}).
The K-matrix shape is particularly complicated and is therefore described in a dedicated subsection.
\begin{table}[!hbt]
\caption{
List of the allowed resonance shape types.
The \texttt{LauResonanceModel} case-sensitive enumeration in the \texttt{LauAbsResonance}
abstract class specifies the integer that selects the resonance type for the \texttt{addResonance}
function. For example, the simple Breit--Wigner integer type is \texttt{LauAbsResonance::BW}.}
\centering
% Use small font for this table so that it fits the page width OK
\resizebox{\textwidth}{!}{
\begin{tabular}{lll}
\hline
Shape name & Enumeration & $R(m)$ Eq. \\
\hline
Simple Breit--Wigner & \texttt{BW} & (\ref{eq:SimpleBW}) \\
Relativistic Breit--Wigner (RBW) & \texttt{RelBW} & (\ref{eq:RelBWEqn}) \\
Modified Breit--Wigner from Gounaris--Sakurai (GS) & \texttt{GS} & (\ref{eq:GS}) \\
Flatt\'e or coupled--channel Breit--Wigner & \texttt{Flatte} & (\ref{eq:Flatte}) \\
$\sigma$ or $f_0(500)$ & \texttt{Sigma} & (\ref{eq:sigma}) \\
$\kappa$ or low--mass $K\pi$ scalar & \texttt{Kappa} & (\ref{eq:sigma}) \\
Low--mass $D\pi$ scalar & \texttt{Dabba} & (\ref{eq:dabba}) \\
LASS $K\pi$ S--wave & \texttt{LASS} & (\ref{eq:LASSEqn}) \\
Resonant part of $K\pi$ LASS & \texttt{LASS\_BW} & (\ref{eq:LASSEqn}) (2$^{\rm{nd}}$ term)\\
Non--resonant part of $K\pi$ LASS & \texttt{LASS\_NR} & (\ref{eq:LASSEqn}) (1$^{\rm{st}}$ term)\\
Form--factor description of the $K\pi$ S--wave & \texttt{EFKLLM} & (\ref{eq:efkllm}) \\
S--wave using $K$--matrix and $P$--vector & \texttt{KMatrix} & (\ref{eq:KMatProd})--(\ref{eq:prodPoleSVP}) \\
Uniform non--resonant (NR) & \texttt{FlatNR} & $R(m) \equiv 1$ \\
Theoretical NR model & \texttt{NRModel} & (\ref{eq:nrmodel}) \\
Empirical NR exponential & \texttt{BelleNR} & (\ref{eq:expnonres}) \\
Empirical NR power--law & \texttt{PowerLawNR} & (\ref{eq:nonrespower}) \\
Empirical NR exponential for symmetrised DPs & \texttt{BelleSymNR} & (\ref{eq:symnr}) \\
Empirical NR Taylor expansion for symmetrised DPs & \texttt{TaylorNR} & (\ref{eq:taylornr}) \\
Empirical NR polynomial & \texttt{PolNR} & (\ref{eq:polynr}) \\
Model-independent partial wave (magnitude \& phase) & \texttt{MIPW\_MagPhase} & (\ref{eq:mipw}) \\
Model-independent partial wave (real \& imaginary) & \texttt{MIPW\_RealImag} & (\ref{eq:mipw}) \\
Incoherent Gaussian shape & \texttt{GaussIncoh} & (\ref{eq:incohgauss}) \\
$\rho-\omega$ mixing: GS for $\rho$, RBW for $\omega$ & \texttt{RhoOmegaMix\_GS} & (\ref{eq:rhoomega}) \\
\hspace*{6em} neglecting $\Delta^2$ denominator term & \texttt{RhoOmegaMix\_GS\_1} & (\ref{eq:rhoomega}) \\
$\rho-\omega$ mixing: RBW for both $\rho$ and $\omega$ & \texttt{RhoOmegaMix\_RBW} & (\ref{eq:rhoomega}) \\
\hspace*{6em} neglecting $\Delta^2$ denominator term & \texttt{RhoOmegaMix\_RBW\_1} & (\ref{eq:rhoomega}) \\
\hline
\end{tabular}
}
\label{tab:resForms}
\end{table}
The simple Breit--Wigner lineshape is given by
%
\begin{equation}
\label{eq:SimpleBW}
R(m) = \frac{1}{m - m_0 - \frac{i}{2}\Gamma_0} \equiv
\frac{(m - m_0) + \frac{i}{2}\Gamma_0}{(m - m_0)^2 + \frac{\Gamma^2_0}{4}} \,,
\end{equation}
%
where $m_0$ is the pole mass and $\Gamma_0$ is the resonance width.
The more commonly used relativistic Breit--Wigner lineshape is described in Sec.~\ref{sec:lineshapes}.
We note here that the relativistic Breit--Wigner lineshape can also describe so-called virtual contributions, from resonances with masses outside the kinematically accessible region of the Dalitz plot, with one modification:
in the calculation of the momenta, the mass $m_0$ is set to a value $m_0^{\rm{eff}}$ within the kinematically allowed range.
This is accomplished with the {\it ad-hoc} formula
\begin{equation}\label{eq:effmass}
m_0^{\rm{eff}}(m_0) = m^{\rm{min}} + \frac{1}{2}(m^{\rm{max}} - m^{\rm{min}})
\left[ 1 + \tanh\left( \frac{m_0 - \frac{m^{\rm{min}}+m^{\rm{max}}}{2}}
{m^{\rm{max}}-m^{\rm{min}}} \right) \right]\, ,
\end{equation}
where $m^{\rm{max}}$ and $m^{\rm{min}}$ are the upper and lower limits of the kinematically allowed mass range.
For virtual contributions, only the tail of the RBW function enters the Dalitz plot.
The Gounaris--Sakurai form of the Breit--Wigner lineshape~\cite{GS} is usually used
as an alternative model for the $\rho$ resonance. It is given by
%
\begin{equation}
\label{eq:GS}
R(m) = \frac{1+D\cdot\Gamma_0/m_0}
{(m_0^2 - m^2) + f(m) - i\, m_0 \Gamma(m)} \,,
\end{equation}
%
where
%
\begin{equation}
\label{eq:GSfm}
f(m) = \Gamma_0 \,\frac{m_0^2}{q_0^3}\,
\left[\;
q^2 \left[h(m)-h(m_0)\right] +
\left(\,m_0^2-m^2\,\right)\,q^2_0\,
\frac{dh}{dm}\bigg|_{m_0}
\;\right] \,,
\end{equation}
%
$q$ is the magnitude of the momentum of one of the daughter particles
in the resonance rest-frame,
%
\begin{equation}
\label{eq:GShm}
h(m) = \frac{2}{\pi}\,\frac{q}{m}\,
\ln\left(\frac{m+2q}{2m_\pi}\right) \,,
\end{equation}
%
and
%
\begin{equation}
\label{eq:GSdh}
\frac{dh}{dm}\bigg|_{m_0} =
h(m_0)\left[(8q_0^2)^{-1}-(2m_0^2)^{-1}\right] \,+\, (2\pi m_0^2)^{-1} \,.
\end{equation}
%
The normalization condition at $R(0)$ fixes the parameter
$D=f(0)/(\Gamma_0 m_0)$, and is found to be~\cite{GS}
%
\begin{equation}
\label{eq:GSd}
D = \frac{3}{\pi}\frac{m_\pi^2}{q_0^2}\,
\ln\left(\frac{m_0+2q_0}{2m_\pi}\right)
+ \frac{m_0}{2\pi\,q_0}
- \frac{m_\pi^2 m_0}{\pi\,q_0^3} \,.
\end{equation}
%
The Flatt\'e~\cite{Flatte:1976xu}, or coupled two-channel Breit--Wigner, lineshape
is usually used to model $f_0(980)$, $K^{*}_0(1430)$ and $a_0(980)$ states:
%%
\begin{equation}
\label{eq:Flatte}
R(m) = \frac{1}{(m_0^2 - m^2) - i m_0 [\Gamma_1(m) + \Gamma_2(m)]} \,.
\end{equation}
%%
The decay widths in the two systems are given by:
%%
\begin{equation}
\label{eq:Gamma1}
\Gamma_1(m) = g_1 f_A \left(\frac{1}{3}\sqrt{1 - (m_{11} + m_{12})^2/m^2} +
\frac{2}{3}\sqrt{1 - (m_{13} + m_{14})^2/m^2} \right) \,,
\end{equation}
%%
\begin{equation}
\label{eq:Gamma2}
\Gamma_2(m) = g_2 f_A \left(\frac{1}{2}\sqrt{1 - (m_{21} + m_{22})^2/m^2} +
\frac{1}{2}\sqrt{1 - (m_{23} + m_{24})^2/m^2} \right) \,,
\end{equation}
%%
where the fractional coefficients come from isospin conservation,
$m_{ij}$ denotes the invariant mass of the daughter particle $j$ (1-4) in channel $i$ (1-2),
and $g_1$ and $g_2$ are coupling constants whose values are assumed to be those
provided in Table~\ref{tab:flattepars}.
The Clebsch-Gordan coefficients in Eqs.~\ref{eq:Gamma1} and~\ref{eq:Gamma2} are not guaranteed to be correct for every possible resonance that could be modelled with the Flatt\'e lineshape, but are appropriate for every case considered in Table~\ref{tab:flattepars}.
The expressions of the widths are continued analytically ($\Gamma \ra i |\Gamma|$) when $m$ is below any of the specific channel thresholds,
contributing to the real part of the amplitude, while the Adler-zero
term $f_A = (m^2 - s_A)/(m^2_0 - s_A)$ can be used to suppress false kinematic
singularities when $m$ goes below threshold~\cite{Bugg:2003kj}
(otherwise $f_A$ is set to unity).
%%
\begin{table}[!htb]
\caption{
The four daughter particles used for each channel term $m_{ij}$, as well as the coupling ($g_1$, $g_2$) and Adler-zero ($s_A$) constants for the Flatt\'e lineshapes.
Units of \gev\ for $g_{1,2}$ and \gevgevcccc\ for $s_A$ are implied.
}
\centering
\begin{tabular}{lllllll}
\hline
Resonance & Channel 1 & Channel 2 & $g_1$ & $g_2$ & $s_A$ & Reference \\
\hline
$f_0(980)$ & \piz,\piz,\pipm,\pipm & \Kpm,\Kpm,\Kz,\Kz & 0.165 & $4.21g_1$ & --- & \cite{Ablikim:2004wn} \\
-$K^{0*}_0(1430)$ & \Kz,\piz,\Kpm,\pipm & \Kz,\etapr,\Kz,\etapr & 0.304 & 0.380 & 0.234 & \cite{Bugg:2003kj} \\
-$K^{\pm*}_0(1430)$ & \Kpm,\piz,\Kz,\pipm & \Kpm,\etapr,\Kpm,\etapr & 0.304 & 0.380 & 0.234 & \cite{Bugg:2003kj} \\
-$a^0_0(980)$ & \etaz,\piz,\etaz,\piz & \Kpm,\Kpm,\Kz,\Kz & 0.353 & $1.03g_1$ & --- & \cite{Abele:1998qd} \\
-$a^{\pm}_0(980)$ & \etaz,\pipm,\etaz,\pipm & \Kpm,\Kz,\Kpm,\Kz & 0.353 & $1.03g_1$ & --- & \cite{Abele:1998qd} \\
+$K^{*}_0(1430)^0$ & \Kz,\piz,\Kpm,\pipm & \Kz,\etapr,\Kz,\etapr & 0.304 & 0.380 & 0.234 & \cite{Bugg:2003kj} \\
+$K^{*}_0(1430)^{\pm}$ & \Kpm,\piz,\Kz,\pipm & \Kpm,\etapr,\Kpm,\etapr & 0.304 & 0.380 & 0.234 & \cite{Bugg:2003kj} \\
+$a_0(980)^0$ & \etaz,\piz,\etaz,\piz & \Kpm,\Kpm,\Kz,\Kz & 0.353 & $1.03g_1$ & --- & \cite{Abele:1998qd} \\
+$a_0(980)^{\pm}$ & \etaz,\pipm,\etaz,\pipm & \Kpm,\Kz,\Kpm,\Kz & 0.353 & $1.03g_1$ & --- & \cite{Abele:1998qd} \\
\hline
\end{tabular}
\label{tab:flattepars}
\end{table}
%%
The $\sigma$ or $f_0(500) \ra \pi\pi$ and $\kappa$ or $K^*_0(800) \ra K\pi$
low--mass scalar resonances can be described using the form
%
\begin{equation}
\label{eq:sigma}
R(m) = \frac{1}{M^2 - s -iM\Gamma(s)} \,,
\end{equation}
%
where $M$ is the mass where the phase shift goes through 90$^{\circ}$ for real $s \equiv m^2$,
and the width
%
\begin{equation}
\label{eq:sigmawidth}
\Gamma(s) = \sqrt{1 - (m_1 + m_2)^2/s}\left(\frac{s - s_A}{M^2 - s_A}\right)(b_1 + b_2s)e^{-(s - M^2)/A} \,,
\end{equation}
%
where the square-root term is the phase space factor, which requires
the invariant masses of the daughter particles $m_1$ and $m_2$, $s_A$ is the Adler-zero constant,
while $b_1$, $b_2$ and $A$ are additional constants~\cite{Bugg:2003kj}.
Table~\ref{tab:sigmakappa} gives the default values of the parameters.
%%
\begin{table}[!htb]
\caption{Default values of the parameters for the $\sigma$ and $\kappa$ lineshapes
based on BES data~\cite{Bugg:2003kj}.}
\centering
\begin{tabular}{llllll}
\hline
Resonance & $M$ (\nbspgevcc) & $b_1$ (\nbspgevcc) & $b_2$ (\nbspgevcc) & $A$ (\nbspgevgevcccc) & $s_A$ \\
\hline
$\sigma$ & 0.9264 & 0.5843 & 1.6663 & 1.082 & $0.5m^2_{\pi}$ \\
$\kappa$ & 3.3 & 24.49 & 0.0 & 2.5 & $m^2_K - 0.5m^2_{\pi}$ \\
\hline
\end{tabular}
\label{tab:sigmakappa}
\end{table}
%%
The $D\pi$ S--wave can be parameterised using the form provided by Bugg~\cite{Bugg:2009tu},
who labels the pole state as ``dabba'':
%
\begin{equation}
\label{eq:dabba}
R(m) = \frac{1}{1 - \beta(m^2-s_0) - ib\rho(m^2-s_A)e^{-\alpha(m^2-s_0)}} \,,
\end{equation}
%
where $\rho$ is the Lorentz invariant phase space factor $\sqrt{1 - s_0/m^2}$,
$s_0$ is the square of the sum of the invariant masses of the $D$ ($m_D$) and
$\pi$ ($m_{\pi}$) daughters, $s_A$ is the Adler-zero term
$m^2_D - 0.5m^2_{\pi}$ that comes from chiral symmetry breaking~\cite{Adler:1965ga}, while
$b$ = 24.49, $\alpha$ = 0.1 and $\beta$ = 0.1.
The RBW function is a very good approximation for
narrow resonances well separated from any other resonant or nonresonant
contribution in the same partial wave.
This approximation is known to be invalid in the $K\pi$ S--wave, since the
$\Kstarbsubz(1430)$ resonance interferes strongly with a slowly varying
nonresonant term~\cite{Meadows:2007jm}.
The so-called LASS lineshape~\cite{lass} has been developed to combine these
amplitudes,
%
\begin{eqnarray}
\label{eq:LASSEqn}
R(m) & = & \frac{m}{q \cot{\delta_B} - iq} + e^{2i \delta_B}
\frac{m_0 \Gamma_0 \frac{m_0}{q_0}}
{(m_0^2 - m^2) - i m_0 \Gamma_0 \frac{q}{m} \frac{m_0}{q_0}}\, , \\
{\rm with} \ \cot{\delta_B} & = & \frac{1}{aq} + \frac{1}{2} r q \, ,
\end{eqnarray}
%
where $m_0$ and $\Gamma_0$ are now the pole mass and width of the $\Kstarbsubz(1430)$,
and $a$ and $r$ are parameters that describe the shape.
Most implementations of the LASS shape in amplitude analyses of \B meson
decays~\cite{Aubert:2004cp,Aubert:2005ce} apply a cut-off
to the slowly varying part close to the charm hadron mass ($\sim 1.7\gevcc$).
% with a constant nonresonant shape taking over at higher masses.
% {\bf check this with Tom -- after cut-off just get tail of RBW?}
An alternative representation of the $K\pi$ S--wave amplitude can be made using the
\texttt{EFKLLM} model described in Ref.~\cite{PhysRevD.79.094005} (the acronym comes
from the surnames of the authors of that paper), which uses a tabulated form--factor $f_0^{K\pi}(m^2)$
that is interpolated using two splines (one each for the magnitude and phase parts), multiplied by a
scaling power--law mass--dependence $m^{\ell}$, leading to
%
\begin{equation}
\label{eq:efkllm}
R(m) = f_0^{K\pi}(m^2) \cdot m^{\ell} \, ,
\end{equation}
%
where suggested values for the exponent $\ell$ are zero for $\kappa$ (this is also the default value)
and $-2$ for $\Kstarbsubz(1430)$.
Because of the large phase-space available in three-body \B meson decays, it
is possible to have nonresonant amplitudes (\ie\ contributions that are not associated
with any known resonance, including virtual states) that are not constant
across the Dalitz plot. One possible parameterisation, based on theoretical
considerations of final-state interactions in $\Bpm \to \Kpm\pip\pim$ decays~\cite{Bediaga:2008zz}, uses the form
%
\begin{equation}
\label{eq:nrmodel}
R(m) = \left[ m_{13}m_{23} f_1(m^2_{13}) f_2(m^2_{23}) e^{-d_0 m^4_{13}m^4_{23}} \right]^{\frac{1}{2}} \,,
\end{equation}
%
where
%
\begin{equation}
\label{eq:nrmodelf}
f_j(m^2) = \frac{1}{1 + e^{a_j(m^2 - b_j)}} \,,
\end{equation}
with the constant parameters $d_0 = 1.3232\times10^{-3}$\,GeV$^{-8}$,
$a_1 = 0.65$\,GeV$^{-2}$, $b_1 = 18$\,GeV$^2$, $a_2 = 0.55$\,GeV$^{-2}$
and $b_2 = 15$\,GeV$^2$ in natural units.
There are several empirical methods that can be used to model the nonresonant
contributions. One is to use an exponential form factor~\cite{Garmash:2004wa}
%
\begin{equation}
\label{eq:expnonres}
R(m) = e^{-\alpha m^2} \, ,
\end{equation}
while another form is simply a power-law distribution
%
\begin{equation}
\label{eq:nonrespower}
R(m) = m^{-2\alpha} \,,
\end{equation}
where in both cases $\alpha$ is a parameter that must be determined from the data.
For symmetric DPs, the exponential form is modified to
%
\begin{equation}
\label{eq:symnr}
R(m) = e^{-\alpha m^2_{13}} + e^{-\alpha m^2_{23}} \,,
\end{equation}
%
while a Taylor expansion up to first order can also be used:
\begin{equation}
\label{eq:taylornr}
R(m) = 1 + \frac{\alpha(m^2_{13} + m^2_{23})}{m^2_P} \,,
\end{equation}
%
where $m_P$ is the invariant mass of the parent $P$.
Another possible description for non-symmetric DPs is based
on the polynomial function~\cite{Lees:2012kxa}
%
\begin{equation}
\label{eq:polynr}
R(m) = \left[m - \frac{1}{2}\left(m_P + \frac{1}{3}(m_1 + m_2 + m_3)\right)\right]^n \,,
\end{equation}
%
where $m_k$ is the invariant mass of daughter particle $k$ and $n$ is
the integer order equal to 0, 1 or 2; a quadratic dependence in $m$ can be constructed
by using up to three polynomial $R(m)$ terms, one for each order along with
their individual $c_j$ amplitude coefficients.
We next come to the model that implements the $\rho-\omega$ mass mixing amplitude
described in Ref.~\cite{Rensing:259802}
%
\begin{equation}
\label{eq:rhoomega}
A_{\rho-\omega} = A_{\rho} \left[ \frac{1 + A_{\omega} \Delta|B| e^{i \phi_{B}}}{1 - \Delta^2 A_{\rho} A_{\omega}} \right],
\end{equation}
%
where $A_{\rho}$ is the $\rho$ lineshape, $A_{\omega}$ is the $\omega$ lineshape, $|B|$ and
$\phi_{B}$ are the relative magnitude and phase of the production amplitudes of
$\rho$ and $\omega$, and $\Delta \equiv \delta(m_{\rho} + m_{\omega})$, where $\delta$ governs
the electromagnetic mixing of $\rho$ and $\omega$ (with pole masses $m_{\rho}$ and $m_{\omega}$).
Here, the amplitude $A_{\omega}$ is always given by the RBW form of Eq.~(\ref{eq:RelBWEqn}), while
the amplitude $A_{\rho}$ can either be represented using
the Gounaris--Sakurai formula given in Eq.~(\ref{eq:GS}) or the RBW form; the required shape is
selected using either the \texttt{RhoOmegaMix\_GS} or \texttt{RhoOmegaMix\_RBW} enumeration integer
labels given in Table~\ref{tab:resForms}.
When ignoring the small $\Delta^2$ term in the denominator of Eq.~(\ref{eq:rhoomega}),
this is equivalent to the parameterisation described in Ref.~\cite{Akhmetshin:2001ig}; this option can be
chosen using either the \texttt{RhoOmegaMix\_GS\_1} or \texttt{RhoOmegaMix\_RBW\_1} enumeration labels,
depending on what lineshape is needed for the $\rho$ resonance.
From SU(3) symmetry, the $\rho$ and $\omega$ are expected to be
produced coherently, which gives the prediction $|B|e^{i\phi_B} = 1$.
To avoid introducing any theoretical assumptions, however, it is advisable that these
parameters are left floating in the fit. In general $\delta$ is complex, although the
imaginary part is small so this is neglected. The theory prediction for
$\delta$ is around $2 \mev$~\cite{PhysRev.134.B671}, and previous analyses
have found $|\delta|$ to be $2.15 \pm 0.35 \mev$~\cite{Rensing:259802} and
$1.57 \pm 0.16 \mev$, and $\rm{arg}~\delta$ to be $0.22 \pm 0.06$~\cite{Akhmetshin:2001ig}.
These parameters can be also be floated in the fit.
If the dynamical structure of the DP cannot be described by any of the
forms given above, then the \texttt{LauModIndPartWave} class can be used to define
a model-independent partial wave component, using splines
to produce an amplitude. It requires a series of mass points called ```knots'', in
ascending order, which sets the magnitude $r(m)$ and phase $\phi(m)$ at each point $m$ that
can be floated when fitted to data:
%
\begin{equation}
\label{eq:mipw}
R(m) = r(m)\left[\cos \phi(m) + i\sin \phi(m) \right] \,.
\end{equation}
The amplitude for points between knots is found using cubic spline interpolation, and
is fixed to zero at the kinematic boundary. There are two implementations for representing
the amplitudes: one uses magnitudes and phases (\texttt{MIPW\_MagPhase}), while the other
uses real and imaginary parts (\texttt{MIPW\_RealImag}).
Finally, the incoherent Gaussian lineshape form is given by
%
\begin{equation}
\label{eq:incohgauss}
R(m) = e^{-(m - m_0)^2/2G^2_0} \,,
\end{equation}
%
where $m_0$ is the mass peak and $G_0$ is the width. This can be used
to parameterise the amplitude for a very narrow resonance, where the measurement
of the width is dominated by experimental resolution effects, producing a lineshape
that is indistinguishable from a Gaussian distribution. The narrow width ensures that
the resonance will not interfere significantly with other resonances in the DP,
\ie\ it will be incoherent. This form could also be used to
parameterise narrow background resonance contributions that would otherwise be
excluded with mass vetoes, such as the $\Dz$ meson decay to $\Km \pip$ in the charmless mode
$\Bm \ra \Km \pip \pim$, when used with the \texttt{addIncoherentResonance} function of
\texttt{LauIsobarDynamics}.

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