Measurement of the impact-parameter dependent azimuthal anisotropy in coherent $ρ^0$ photoproduction in Pb$-$Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.02 TeV

This Letter presents the first measurement of the impact-parameter dependent angular anisotropy in the decay of coherently photoproduced $\rho^0$ mesons. The $\rho^0$ mesons are reconstructed through their decay into pion pairs. The measured anisotropy corresponds to the amplitude of the $\cos(2\phi)$ modulation, where $\phi$ is the angle between the two vectors formed by the sum and the difference of the transverse momenta of the pions, respectively. The measurement was performed by the ALICE Collaboration at the LHC using data from ultraperipheral Pb$-$Pb collisions at a center-of-mass energy of $\sqrt{s_{\mathrm{NN}}}~=~5.02$ TeV per nucleon pair. Different impact-parameter regions are selected by classifying the events in nuclear-breakup classes. The amplitude of the $\cos(2\phi)$ modulation is found to increase by about one order of magnitude from large to small impact parameters. Theoretical calculations describe the measured $\cos(2\phi)$ anisotropy and its impact-parameter dependence as the result of a quantum interference effect at the femtometer scale, arising from the ambiguity regarding which of the nuclei is the photon source in the interaction.

 

Phys. Lett. B 858 (2024) 139017
HEP Data
e-Print: arXiv:2405.14525 | PDF | inSPIRE
CERN-EP-2024-126
Figure group

Figure 1

Invariant-mass distribution of pion pairs, with superimposed S\"{o}ding (solid line) and Ross-Stodolsky (dotted line) fits, for the range $0\phi\pi/7$ in the 0n0n (left) and XnXn (right) neutron classes. The different components of the pion-pair production amplitude in the S\"{o}ding model are shown: the Breit--Wigner shape that describes the \rhoz (finer dotted line), the continuum process (dash-dotted line), and the interference between the \rhoz and the continuum (dash-dot-dot-dot line). The Breit--Wigner extracted from the Ross-Stodolsky model (finest dotted line) is also shown. In this example, the background contribution from misidentified muons is fixed to zero in the fit.

Figure 2

Example of a simultaneous fit to the \rhoz yield as a function of \phiz, used to extract the amplitude of the $\cos(2\phi)$ modulation in all neutron classes. The contribution of each physical class to the yield in all experimental classes is shown.

Figure 3

Amplitudes of the $\cos(2\phi)$ modulation of the \rhoz yield in Pb--Pb collisions at $\sqrt{s_{\rm{NN}}}$ = 5.02 \TeV in all neutron classes. The results are compared with the Xing et al.  and W. Zhao \etal  model predictions and, for the XnXn class, with the STAR results  in Au--Au and U--U collisions at RHIC. For all the experimental data points, statistical uncertainties are represented with a bar and systematic uncertainties with a box.