Dear Djamel, here are some comments on the draft. I have tried to work a comprimise on Bjorken. I have also put in the more modern format for author list and added acknowledments. Yours Michael. The comments are listed here but they are also in the text file and attached. Dear Djamel, here are my comments. The insert of Fig 4 should have Sqrt(Snn) as the x label. It is something else on my printer. I think it is better to use the \affiliation for the author list since this letter search engines "harvest" the institute information. If there is space I would add a table of the 4pi yields. Michael At forward rapidities, where more net--baryons are observed~\cite{peter}, other production mechanisms, such as %MJM strangeness associated production associated production of strangeness may compete. BRAHMS consists of mid--rapidity (MRS) and forward spectrometers (FS) that measure the momentum, charge and mass of particles, and a set of global detectors for event characterization %MJM delete last line. \cite{nim}. \cite{nim,myself} Particle spectra have been obtained by combining several data sets, each set being characterized by a spectrometer setting (magnetic field and position), % MJM thus that is a given portion of the phase--space $(y,p_T)$. Change Yields $dN/dy$ were calculated by integrating the resulting fit functions over the whole $p_T$ range. to %MJM Yields The $dN/dy$ yields were calculated by integrating the resulting fit functions over the whole $p_T$ range. The difference between kaon and pion spectral shapes may be accounted for a contribution of resonance decays producing pions at low $p_T$. ==> he difference between kaon and pion spectral shapes may be accounted for %MJM a by the contribution of resonance decays producing pions at low $p_T$. Change a sum of Gaussian (G2) or Woods-Saxon (WS) distributions placed symmetrically around $y=0$. ==> a sum of two Gaussians %MJM or two Woods-Saxon distributions placed symmetrically around $y=0$. You don't need to name the functions since you never use them again. If you have the space it would be nice to have the 4pi yields as a table at the back. %MJM It does not matter if you systematic error depends upon y as long as % it is not so large that we cannot discriminate between a flat distribution % and a Gaussian one. Change Unfortunately, a non negligible fraction of our systematic error depends on $y$. Therefore, the present data cannot bring a definitive conclusion regarding the Bjorken picture. However, they exhibit a nearly Gaussian rapidity distribution. Widths are found to be $\sigma_{\pi^+} = 2.27 ==> While the Bjorken picture may work reasonably well for |y|<1 it certainly fails to describe the full rapidity region. Indeed our rapidity distributions are well represented by Gaussians. The widths are found to be Change This reminds of the old hydrodynamical expansion model proposed by L.~D.~Landau fifty years ago~\cite{landau}. ==> This is reminiscent of the old hydrodynamical expansion model proposed by L.~D.~Landau fifty years ago~\cite{landau}. Delete Eqn 1 and say the hydrodynamical equations, using the equation of state of a relativistic gas of massless particles, leads to a Gaussian dN/dy distribution. In a simplified ... Change Figure~\ref{fig:landau}(a) shows $dN/dy(\pi)$ and Landau's prediction for \snn{200} (using Eq.~\ref{eq:gaus} and \ref{eq:width} with the condition that the integrals of these Gaussians must be equal to the full--space yields estimated from the data). ==> Figure~\ref{fig:landau}(a) shows $dN/dy(\pi)$ and Landau's prediction for \snn{200} (using Eq.~ %MJM\ref{eq:gaus} and \ref{eq:width} with the condition that the integrals of these Gaussians must be equal to the full--space yields estimated from the data). The Gaussian distributions got a lot of press at QM04. I think that the last paragraph should be reordered and the link to Landau strengthened. In conclusion, BRAHMS has measured the transverse momentum spectra and inclusive invariant yields of charged meson $\pi^\pm$ and $K^\pm$. The particle yields show a maximum at mid--rapidity and decrease by more than a factor 3 at y$> 3$. The rapidity coverage allowed total yields to be estimated. It has been found that pion rapidity distributions are relatively well described by Gaussians, the width of which are not in complete disagreement with the Landau hydrodynamical model~\cite{landau,carut}. The gross agreement is valid at lower energies as well, in spite of the difference in the degree of transparency. The $K/\pi$ ratios are well reproduced by the hadron gas statistical model~\cite{braun} that assumes strangeness equilibration. The increasing difference between $K^+$ and $K^-$ yields at higher rapidities can be explained by a change of the baryo--chemical potential $\mu_B$ with increasing rapidity. This variation can be compared with the energy systematics of the $K/\pi$ ratios within such statistical context. =>> In conclusion, BRAHMS has measured the transverse momentum spectra and inclusive invariant yields of charged meson $\pi^\pm$ and $K^\pm$. The particle yields show a maximum at mid--rapidity and decrease by more than a factor 3 at y$> 3$. The rapidity coverage allowed total yields to be estimated. The $K/\pi$ ratios are well reproduced by the hadron gas statistical model~\cite{braun} that assumes strangeness equilibration. The increasing difference between $K^+$ and $K^-$ yields at higher rapidities can be explained by a change of the baryo--chemical potential $\mu_B$ with increasing rapidity. This variation can be compared with the energy systematics of the $K/\pi$ ratios within such statistical context. The pion rapidity distributions are well described by Gaussians, the width of which are within 5\% of the Landau hydrodynamical model~\cite{landau,carut}. At lower energies the difference between this model and the data are also ~5\% , in spite of the difference in the degree of transparency. _______________________________________________ Brahms-l mailing list Brahms-l@lists.bnl.gov http://lists.bnl.gov/mailman/listinfo/brahms-l
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