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Direct photon interferometry as tool to probe the space-time evolution of heavy-ion collisions

<!--HTML-->We investigate the measurement of Hanbury Brown-Twiss (HBT) photon correlations [1] as an experimental tool to discriminate different sources of photon production. To showcase that HBT correlations can distinguish between such sources, we consider two different scenarios in which we...

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Detalles Bibliográficos
Autor principal: Garcia-Montero, Oscar
Lenguaje:eng
Publicado: 2021
Materias:
Acceso en línea:http://cds.cern.ch/record/2749440
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author Garcia-Montero, Oscar
author_facet Garcia-Montero, Oscar
author_sort Garcia-Montero, Oscar
collection CERN
description <!--HTML-->We investigate the measurement of Hanbury Brown-Twiss (HBT) photon correlations [1] as an experimental tool to discriminate different sources of photon production. To showcase that HBT correlations can distinguish between such sources, we consider two different scenarios in which we enhance the yields from standard hydrodynamical simulations. In the first, additional photons are produced from the early pre-equilibrium stage computed from the ``bottom-up" thermalization scenario [2-4]. In the second, the thermal rates are enhanced close to the pseudo-critical temperature $T_c\approx 155\,\text{MeV}$ using a phenomenological ansatz [5]. We compute the correlators for relative momenta $q_o, \,q_s$ and $q_l$ for different transverse pair momenta, $K_\perp$, and find that the longitudinal correlation is the most sensitive to different photon sources. Our results also demonstrate that including anisotropic pre-equilibrium rates enhances non-Gaussianities in the correlators, which can be quantified using the kurtosis of the correlators. Finally, we study the feasibility of measuring a direct photon HBT signal in the upcoming high-luminosity LHC runs. Considering only statistical uncertainties, we find that with the projected $\sim 10^{10}$ heavy ion events a measurement of the HBT correlations for $K_\perp<1\, \text{GeV}$ is statistically significant. References [1] E. Frodermann and U. Heinz, Phys. Rev. C80, 044903 (2009), arXiv:0907.1292 [nucl-th] [2] J. Berges, K. Reygers, N. Tanji, and R. Venugopalan, Phys. Rev. C95, 054904 (2017), arXiv:1701.05064 [nucl- th]
 [3] R. Baier, A. H. Mueller, D. Schiff, and D. T. Son, Phys. Lett. B502, 51 (2001), arXiv:hep-ph/0009237 [hep-ph] [4] O. Garcia-Montero, (2019), arXiv:1909.12294 [hep-ph] [5] H. van Hees, M. He, and R. Rapp, Nucl. Phys. A933, 256 (2015), arXiv:1404.2846 [nucl-th]
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language eng
publishDate 2021
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spelling cern-27494402022-11-02T22:26:19Zhttp://cds.cern.ch/record/2749440engGarcia-Montero, OscarDirect photon interferometry as tool to probe the space-time evolution of heavy-ion collisionsInitial Stages 2021Conferences<!--HTML-->We investigate the measurement of Hanbury Brown-Twiss (HBT) photon correlations [1] as an experimental tool to discriminate different sources of photon production. To showcase that HBT correlations can distinguish between such sources, we consider two different scenarios in which we enhance the yields from standard hydrodynamical simulations. In the first, additional photons are produced from the early pre-equilibrium stage computed from the ``bottom-up" thermalization scenario [2-4]. In the second, the thermal rates are enhanced close to the pseudo-critical temperature $T_c\approx 155\,\text{MeV}$ using a phenomenological ansatz [5]. We compute the correlators for relative momenta $q_o, \,q_s$ and $q_l$ for different transverse pair momenta, $K_\perp$, and find that the longitudinal correlation is the most sensitive to different photon sources. Our results also demonstrate that including anisotropic pre-equilibrium rates enhances non-Gaussianities in the correlators, which can be quantified using the kurtosis of the correlators. Finally, we study the feasibility of measuring a direct photon HBT signal in the upcoming high-luminosity LHC runs. Considering only statistical uncertainties, we find that with the projected $\sim 10^{10}$ heavy ion events a measurement of the HBT correlations for $K_\perp<1\, \text{GeV}$ is statistically significant. References [1] E. Frodermann and U. Heinz, Phys. Rev. C80, 044903 (2009), arXiv:0907.1292 [nucl-th] [2] J. Berges, K. Reygers, N. Tanji, and R. Venugopalan, Phys. Rev. C95, 054904 (2017), arXiv:1701.05064 [nucl- th]
 [3] R. Baier, A. H. Mueller, D. Schiff, and D. T. Son, Phys. Lett. B502, 51 (2001), arXiv:hep-ph/0009237 [hep-ph] [4] O. Garcia-Montero, (2019), arXiv:1909.12294 [hep-ph] [5] H. van Hees, M. He, and R. Rapp, Nucl. Phys. A933, 256 (2015), arXiv:1404.2846 [nucl-th]oai:cds.cern.ch:27494402021
spellingShingle Conferences
Garcia-Montero, Oscar
Direct photon interferometry as tool to probe the space-time evolution of heavy-ion collisions
title Direct photon interferometry as tool to probe the space-time evolution of heavy-ion collisions
title_full Direct photon interferometry as tool to probe the space-time evolution of heavy-ion collisions
title_fullStr Direct photon interferometry as tool to probe the space-time evolution of heavy-ion collisions
title_full_unstemmed Direct photon interferometry as tool to probe the space-time evolution of heavy-ion collisions
title_short Direct photon interferometry as tool to probe the space-time evolution of heavy-ion collisions
title_sort direct photon interferometry as tool to probe the space-time evolution of heavy-ion collisions
topic Conferences
url http://cds.cern.ch/record/2749440
work_keys_str_mv AT garciamonterooscar directphotoninterferometryastooltoprobethespacetimeevolutionofheavyioncollisions
AT garciamonterooscar initialstages2021