热双轻子辐射的极化

IF 4.5 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Physics Letters B Pub Date : 2025-02-01 Epub Date: 2025-01-16 DOI:10.1016/j.physletb.2025.139267
Florian Seck , Bengt Friman , Tetyana Galatyuk , Hendrik van Hees , Ralf Rapp , Enrico Speranza , Jochen Wambach
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引用次数: 0

摘要

高能重离子碰撞形成的火球辐射出的双轻子的不变质谱已成功地用于研究热致密QCD物质的性质。利用现实的介质电磁波谱函数模型,对极化观测值进行了预测,并与实验结果进行了比较。这使得首次对虚拟光子自能的纵向和横向分量进行独立测试成为可能。虽然低质量和高质量区域分别表现出横向和非极化光子的预期极限,但在ρ介子质量区域中重子驱动的介质效应产生了明显的纵向极化,并跃迁到夸克-胶子等离子体的大部分非极化发射中,从而提供了对QCD物质微观发射过程的敏感测试。对HADES和NA60实验在SIS和SPS能量下的可用数据的应用与我们的预测一致,并为FAIR和对撞机能量下的定量极化研究奠定了基础。
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Polarization of thermal dilepton radiation
The invariant mass spectra of dileptons radiated from the fireballs formed in high-energy heavy-ion collisions have been successfully used to investigate the properties of hot and dense QCD matter. Using a realistic model for the in-medium electromagnetic spectral function, we predict polarization observables and compare them to experiment. This allows, for the first time, independent tests of the longitudinal and transverse components of the virtual photon's selfenergy. While the low- and high-mass regions exhibit the expected limits of transverse and unpolarized photons, respectively, baryon-driven medium effects in the ρ-meson mass region create a marked longitudinal polarization that transits into a largely unpolarized emission from the quark-gluon plasma, thus providing a sensitive test of microscopic emission processes in QCD matter. Applications to available data from the HADES and NA60 experiments at SIS and SPS energies, respectively, are consistent with our predictions and set the stage for quantitative polarization studies at FAIR and collider energies.
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来源期刊
Physics Letters B
Physics Letters B 物理-物理:综合
CiteScore
9.10
自引率
6.80%
发文量
647
审稿时长
3 months
期刊介绍: Physics Letters B ensures the rapid publication of important new results in particle physics, nuclear physics and cosmology. Specialized editors are responsible for contributions in experimental nuclear physics, theoretical nuclear physics, experimental high-energy physics, theoretical high-energy physics, and astrophysics.
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