Skip to main content
QUICK REVIEW

[Paper Review] Measurement of the Open Charm Cross-Section in $\sqrt{s_{NN}}$ = 200 GeV Cu+Cu Collisions at STAR

Stephen Baumgart|arXiv (Cornell University)|Sep 26, 2007
High-Energy Particle Collisions Research4 citations
TL;DR

This study measures the mid-rapidity open charm cross-section in $√{s_{NN}}$ = 200 GeV Cu+Cu collisions at RHIC using direct reconstruction of $D^0$ and $\overline{D^0}$ via the $K\pi$ decay channel. The measured charm cross-section per binary collision is $1.30 \pm 0.25$ mb, confirming binary scaling and indicating production via initial hard scattering processes, with implications for FONLL model under-prediction.

ABSTRACT

We present the mid-rapidity $(D^{0} + \bar{D^{0}})/2$ yield measured in $\sqrt{s_{NN}}$ = 200 GeV Cu+Cu collisions at RHIC via direct reconstruction through the $Kπ$ decay channel. A charm cross-section is reported and compared to theoretical predictions and to previous RHIC experimental results.

Motivation & Objective

  • To measure the open charm cross-section in $√{s_{NN}}$ = 200 GeV Cu+Cu collisions at RHIC using direct reconstruction of $D^0$ and $\overline{D^0}$ via the $K\pi$ decay channel.
  • To test whether charm production scales with the number of binary nucleon-nucleon collisions, as expected for initial hard scattering processes.
  • To compare the measured charm cross-section with theoretical FONLL predictions and previous RHIC measurements from STAR and PHENIX.
  • To investigate discrepancies between experimental data and FONLL calculations, which may indicate missing physics in current models.

Proposed method

  • Reconstruct $D^0$ and $\overline{D^0}$ via the $K\pi$ decay channel using invariant mass reconstruction with the formula $m_{D^0} = \sqrt{m_\pi^2 + m_K^2 + 2(E_\pi E_K - |p_\pi||p_K|\cos\theta)}$.
  • Apply rotational background subtraction by rotating one kaon-pion pair in momentum space every 5° from 150° to 210° to estimate and subtract uncorrelated background.
  • Use a Gaussian function plus a first-order polynomial to fit the invariant mass spectrum, achieving a 4.6σ significance for the $D^0+\overline{D^0}$ peak.
  • Correct for detector efficiency and acceptance using detailed GEANT simulations of the STAR TPC and apply a branching ratio correction of $3.80 \pm 0.07\%$.
  • Fit the transverse momentum spectrum with an $m_t - m_0$ exponential function to extract the $dN_{D^0}/dy$ yield.
  • Convert the $dN_{D^0}/dy$ yield to a cross-section per binary collision using the formula $\sigma_{c\overline{c}}^{NN} = (dN_{D^0}/dy) \times (\sigma_{pp}^{inelastic}/N_{bin}^{CuCu}) \times (f/R)$, with $\sigma_{pp}^{inelastic} = 42$ mb, $N_{bin}^{CuCu} = 51.5^{+1.0}_{-2.9}$, $f = 4.7 \pm 0.7$, and $R = 0.54 \pm 0.05$.

Experimental results

Research questions

  • RQ1Does charm production in Cu+Cu collisions at $\sqrt{s_{NN}}$ = 200 GeV scale with the number of binary nucleon-nucleon collisions, as expected for initial hard scattering processes?
  • RQ2How does the measured open charm cross-section in Cu+Cu collisions compare to theoretical FONLL predictions at this energy?
  • RQ3Are the discrepancies between previous STAR and PHENIX charm cross-section measurements statistically significant or consistent with systematic uncertainties?
  • RQ4Does the observed charm cross-section in Cu+Cu collisions support the hypothesis of charm production via gluon fusion in early-stage collisions?

Key findings

  • The $D^0 + \overline{D^0}$ invariant mass peak was observed with a statistical significance of 4.6σ after background subtraction using the rotational method.
  • The mid-rapidity $dN_{D^0}/dy$ yield was measured to be $0.184 \pm 0.035$ (statistical uncertainty) from the $m_t - m_0$ exponential fit to the transverse momentum spectrum.
  • The preliminary charm cross-section per binary collision in Cu+Cu collisions is $1.30 \pm 0.25$ mb, consistent with binary scaling observed in previous STAR data from p+p to central Au+Au.
  • The measured cross-section exceeds the FONLL prediction of $0.256^{+0.400}_{-0.146}$ mb, indicating a potential under-prediction by current theoretical models.
  • The result supports the interpretation that charm quarks are produced in initial hard scattering processes, consistent with perturbative QCD expectations.

Better researchstarts right now

From reading papers to final review, dramatically reduce your research time.

No credit card · Free plan available

This review was created by AI and reviewed by human editors.