Flavor hierarchy of parton energy loss in quark-gluon plasma from a Bayesian analysis
Abstract: The quenching of light and heavy flavor hadrons in relativistic heavy-ion collisions probes the color and flavor dependences of parton energy loss through a color-deconfined quark-gluon plasma (QGP), and thus reveals the properties of QCD matter at extremely high density and temperature. By combining a next-to-leading order perturbative QCD calculation of parton production, a general ansatz of parton energy loss functions and parton fragmentation functions, we calculate the nuclear modification of various hadron species -- charged hadrons, $D$ mesons and $B$-decayed $J/\psi$ -- over a wide transverse momentum regime. Comparing our calculations to the experimental data using the Bayesian statistical analysis, we perform a first simultaneous extraction of the energy loss functions of gluons ($g$), light quarks ($q$), charm quarks ($c$) and bottom quarks ($b$) inside the QGP. We find that the average parton energy loss at high energies follows the expected hierarchy of $\langle \Delta E_g \rangle > \langle \Delta E_q \rangle \sim \langle \Delta E_c \rangle > \langle \Delta E_b \rangle$, while the parton energy loss distribution can further test the QCD calculations of parton interaction with the dense nuclear matter. We also find that the reduction of experimental uncertainties can significantly improve the precision of the extracted parton energy loss functions inside the QGP.
- X.-N. Wang and M. Gyulassy, Phys. Rev. Lett. 68, 1480 (1992).
- J. D. Bjorken, FERMILAB-PUB-82-059-THY (1982).
- E. Braaten and M. H. Thoma, Phys. Rev. D44, 2625 (1991).
- M. Djordjevic, Phys. Rev. C 74, 064907 (2006), arXiv:nucl-th/0603066.
- G.-Y. Qin et al., Phys. Rev. Lett. 100, 072301 (2008), arXiv:0710.0605.
- Phys. Lett. B345, 277 (1995), arXiv:hep-ph/9411409.
- Nucl. Phys. B483, 291 (1997), hep-ph/9607355.
- B. G. Zakharov, JETP Lett. 63, 952 (1996), arXiv:hep-ph/9607440.
- Nucl. Phys. B571, 197 (2000), arXiv:hep-ph/9907461.
- U. A. Wiedemann, Nucl. Phys. B588, 303 (2000), arXiv:hep-ph/0005129.
- JHEP 06, 030 (2002), hep-ph/0204343.
- Nucl. Phys. A696, 788 (2001), arXiv:hep-ph/0102230.
- ATLAS, G. Aad et al., Phys. Rev. Lett. 114, 072302 (2015), arXiv:1411.2357.
- CMS, V. Khachatryan et al., JHEP 04, 039 (2017), arXiv:1611.01664.
- ALICE, S. Acharya et al., JHEP 11, 013 (2018), arXiv:1802.09145.
- S. A. Bass et al., Phys. Rev. C79, 024901 (2009), arXiv:0808.0908.
- Y. He et al., Phys. Rev. C99, 054911 (2019), arXiv:1809.02525.
- Phys. Lett. B 805, 135424 (2020), arXiv:1906.00413.
- Phys. Rev. Lett. 122, 252301 (2019), arXiv:1903.01993.
- JETSCAPE, A. Kumar et al., Phys. Rev. C 107, 034911 (2023), arXiv:2204.01163.
- ATLAS, G. Aad et al., Phys. Rev. Lett. 105, 252303 (2010), arXiv:1011.6182.
- Phys. Rev. Lett. 98, 212301 (2007), arXiv:nucl-th/0701045.
- G.-Y. Qin and B. Muller, Phys. Rev. Lett. 106, 162302 (2011), arXiv:1012.5280, [Erratum: Phys. Rev. Lett.108,189904(2012)].
- Phys. Lett. B773, 672 (2017), arXiv:1607.01932.
- CMS, S. Chatrchyan et al., Phys. Lett. B 718, 773 (2013), arXiv:1205.0206.
- Phys. Rev. C80, 054909 (2009), arXiv:0906.3280.
- Phys. Lett. B 777, 86 (2018), arXiv:1704.03648.
- Phys. Lett. B782, 707 (2018), arXiv:1803.06785.
- Phys. Rev. C98, 021901 (2018), arXiv:1804.11041.
- CMS, S. Chatrchyan et al., JHEP 10, 087 (2012), arXiv:1205.5872.
- CMS, S. Chatrchyan et al., Phys. Lett. B 730, 243 (2014), arXiv:1310.0878.
- ATLAS, G. Aad et al., Phys. Lett. B 739, 320 (2014), arXiv:1406.2979.
- STAR, M. S. Abdallah et al., Phys. Rev. C 105, 044906 (2022), arXiv:2109.09793.
- Phys. Rev. C94, 024902 (2016), arXiv:1603.01920.
- Phys. Rev. C95, 044909 (2017), arXiv:1701.07951.
- Phys. Lett. B801, 135181 (2020), arXiv:1906.09562.
- JETSCAPE, Y. Tachibana et al., arXiv:2301.02485 (2023), arXiv:2301.02485.
- Phys. Lett. B 837, 137638 (2023), arXiv:2109.14314.
- Nucl. Phys. A 1005, 121934 (2021).
- C. Sirimanna et al., Phys. Rev. C 108, 014911 (2023), arXiv:2211.15553.
- A. Majumder and M. Van Leeuwen, Prog. Part. Nucl. Phys. 66, 41 (2011), arXiv:1002.2206.
- Int. J. Mod. Phys. E24, 1530014 (2015), arXiv:1511.00790.
- J.-P. Blaizot and Y. Mehtar-Tani, Int. J. Mod. Phys. E 24, 1530012 (2015), arXiv:1503.05958.
- S. Cao and X.-N. Wang, Rept. Prog. Phys. 84, 024301 (2021), arXiv:2002.04028.
- S. Cao and G.-Y. Qin, Ann. Rev. Nucl. Part. Sci. 73, 205 (2023), arXiv:2211.16821.
- JET, K. M. Burke et al., Phys. Rev. C 90, 014909 (2014), arXiv:1312.5003.
- Eur. Phys. J. C 76, 475 (2016), arXiv:1606.04837.
- Phys. Rev. D 103, L031901 (2021), arXiv:1907.11808.
- JETSCAPE, S. Cao et al., Phys. Rev. C 104, 024905 (2021), arXiv:2102.11337.
- Phys. Rev. C 108, L011901 (2023), arXiv:2206.01340.
- R. Baier, Nucl. Phys. A715, 209 (2003), arXiv:hep-ph/0209038.
- A. Majumder, Phys. Rev. C80, 031902 (2009), arXiv:0810.4967.
- Phys. Rev. Lett. 85, 3591 (2000), arXiv:hep-ph/0005044.
- A. Majumder, Phys. Rev. D85, 014023 (2012), arXiv:0912.2987.
- Phys. Rev. C 105, 024908 (2022), arXiv:2108.05329.
- arXiv:2208.14297 (2022), arXiv:2208.14297.
- F. Arleo, Phys. Rev. Lett. 119, 062302 (2017), arXiv:1703.10852.
- Nucl. Phys. B484, 265 (1997), arXiv:hep-ph/9608322.
- F. Arleo, JHEP 11, 044 (2002), arXiv:hep-ph/0210104.
- Phys. Rev. Lett. 122, 252302 (2019), arXiv:1808.05310.
- Sci. Bull. 68, 2003 (2023), arXiv:2208.08323.
- Nucl. Phys. B327, 105 (1989).
- Phys. Rev. D67, 054005 (2003), hep-ph/0211007.
- S. Kretzer, Phys. Rev. D 62, 054001 (2000), arXiv:hep-ph/0003177.
- Nucl. Phys. B 799, 34 (2008), arXiv:0712.0481.
- Phys. Rev. D 77, 014011 (2008), arXiv:0705.4392.
- CMS, A. M. Sirunyan et al., Phys. Lett. B 782, 474 (2018), arXiv:1708.04962.
- CMS, A. M. Sirunyan et al., Eur. Phys. J. C 78, 509 (2018), arXiv:1712.08959.
- J. Pumplin et al., JHEP 07, 012 (2002), arXiv:hep-ph/0201195.
- Nucl. Phys. A 1005, 121829 (2021).
- Y.-F. Liu et al., Phys. Rev. C 105, 044904 (2022), arXiv:2107.01522.
- JHEP 0904, 065 (2009), arXiv:0902.4154.
- Phys. Lett. B735, 445 (2014), arXiv:1401.3817.
- S. Y. F. Liu and R. Rapp, Phys. Rev. C97, 034918 (2018), arXiv:1711.03282.
- Phys. Lett. B 838, 137733 (2023), arXiv:2112.15062.
- Phys. Rev. Lett. 90, 202303 (2003), arXiv:nucl-th/0301087.
- S. Cao et al., Phys. Lett. B 807, 135561 (2020), arXiv:1911.00456.
- JHEP 0605, 026 (2006), arXiv:hep-ph/0603175.
- CMS, A. M. Sirunyan et al., Phys. Rev. Lett. 119, 152301 (2017), arXiv:1705.04727.
- J. Novak et al., Phys. Rev. C89, 034917 (2014), arXiv:1303.5769.
- Phys. Rev. Lett. 114, 202301 (2015), arXiv:1501.04042.
- J. E. Bernhard et al., Phys. Rev. C91, 054910 (2015), arXiv:1502.00339.
- Phys. Rev. C94, 024907 (2016), arXiv:1605.03954.
- Phys. Rev. C 97, 044905 (2018), arXiv:1706.03666.
- Nature Phys. 15, 1113 (2019).
- JETSCAPE, D. Everett et al., Phys. Rev. Lett. 126, 242301 (2021), arXiv:2010.03928.
- Phys. Rev. C97, 014907 (2018), arXiv:1710.00807.
- Phys. Lett. B 833, 137348 (2022), arXiv:2202.01998.
- Publications of the Astronomical Society of the Pacific 125, 306 (2013).
- Statistical Science 4, 409 (1989).
- Gaussian process for machine learning (The MIT Press, 2006).
- Phys. Rev. Lett. 93, 072301 (2004), arXiv:nucl-th/0309040.
- Phys. Lett. B777, 255 (2018), arXiv:1703.00822.
Paper Prompts
Sign up for free to create and run prompts on this paper using GPT-5.
Top Community Prompts
Collections
Sign up for free to add this paper to one or more collections.