Adrian William Romero Jorge, Elena Bratkovskaya, Taesoo Song, Laura Sagunski
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The analysis is based on the microscopic Parton–Hadron–String Dynamics (PHSD) transport model, which successfully reproduces the measured dilepton spectra in <span></span><math>\n <semantics>\n <mrow>\n <mi>p</mi>\n <mo>+</mo>\n <mi>p</mi>\n </mrow>\n <annotation>$$ p+p $$</annotation>\n </semantics></math>, <span></span><math>\n <semantics>\n <mrow>\n <mi>p</mi>\n <mo>+</mo>\n <mi>A</mi>\n </mrow>\n <annotation>$$ p+A $$</annotation>\n </semantics></math>, and <span></span><math>\n <semantics>\n <mrow>\n <mi>A</mi>\n <mo>+</mo>\n <mi>A</mi>\n </mrow>\n <annotation>$$ A+A $$</annotation>\n </semantics></math> collisions. Besides the dilepton channels resulting from interactions and decays of Standard Model particles (such as mesons and baryons), we extend the PHSD approach to include the decay of hypothetical <i>U</i>-bosons into dileptons, <span></span><math>\n <semantics>\n <mrow>\n <mi>U</mi>\n <mo>→</mo>\n <msup>\n <mi>e</mi>\n <mo>+</mo>\n </msup>\n <msup>\n <mi>e</mi>\n <mo>−</mo>\n </msup>\n </mrow>\n <annotation>$$ U\\to {e}^{+}{e}^{-} $$</annotation>\n </semantics></math>. The production of these <i>U</i>-bosons occurs via Dalitz decays of pions, <i>η</i>-mesons, <i>ω</i>-mesons, Delta resonances, as well as from the decays of vector mesons and <span></span><math>\n <semantics>\n <mrow>\n <msup>\n <mi>K</mi>\n <mo>+</mo>\n </msup>\n </mrow>\n <annotation>$$ {K}^{+} $$</annotation>\n </semantics></math> mesons. This analysis provides an upper limit on <span></span><math>\n <semantics>\n <mrow>\n <msup>\n <mi>ϵ</mi>\n <mn>2</mn>\n </msup>\n <mfenced>\n <msub>\n <mi>M</mi>\n <mi>U</mi>\n </msub>\n </mfenced>\n </mrow>\n <annotation>$$ {\\upvarepsilon}^2\\left({M}_U\\right) $$</annotation>\n </semantics></math> and offers insights into the accuracy required for future experimental searches for dark photons through dilepton experiments.</p>","PeriodicalId":55442,"journal":{"name":"Astronomische Nachrichten","volume":"346 3-4","pages":""},"PeriodicalIF":1.0000,"publicationDate":"2024-12-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1002/asna.20240132","citationCount":"0","resultStr":"{\"title\":\"Exploring Dark Photon Production and Kinetic Mixing Constraints in Heavy-Ion Collisions\",\"authors\":\"Adrian William Romero Jorge, Elena Bratkovskaya, Taesoo Song, Laura Sagunski\",\"doi\":\"10.1002/asna.20240132\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>Vector <i>U</i>-bosons, often referred to as “dark photons,” are potential candidates for mediating dark matter interactions. In this study, we outline a procedure to derive theoretical constraints on the upper bound of the kinetic mixing parameter <span></span><math>\\n <semantics>\\n <mrow>\\n <msup>\\n <mi>ϵ</mi>\\n <mn>2</mn>\\n </msup>\\n <mfenced>\\n <msub>\\n <mi>M</mi>\\n <mi>U</mi>\\n </msub>\\n </mfenced>\\n </mrow>\\n <annotation>$$ {\\\\upvarepsilon}^2\\\\left({M}_U\\\\right) $$</annotation>\\n </semantics></math> using dilepton data from heavy-ion from SIS to RHIC energies. The analysis is based on the microscopic Parton–Hadron–String Dynamics (PHSD) transport model, which successfully reproduces the measured dilepton spectra in <span></span><math>\\n <semantics>\\n <mrow>\\n <mi>p</mi>\\n <mo>+</mo>\\n <mi>p</mi>\\n </mrow>\\n <annotation>$$ p+p $$</annotation>\\n </semantics></math>, <span></span><math>\\n <semantics>\\n <mrow>\\n <mi>p</mi>\\n <mo>+</mo>\\n <mi>A</mi>\\n </mrow>\\n <annotation>$$ p+A $$</annotation>\\n </semantics></math>, and <span></span><math>\\n <semantics>\\n <mrow>\\n <mi>A</mi>\\n <mo>+</mo>\\n <mi>A</mi>\\n </mrow>\\n <annotation>$$ A+A $$</annotation>\\n </semantics></math> collisions. Besides the dilepton channels resulting from interactions and decays of Standard Model particles (such as mesons and baryons), we extend the PHSD approach to include the decay of hypothetical <i>U</i>-bosons into dileptons, <span></span><math>\\n <semantics>\\n <mrow>\\n <mi>U</mi>\\n <mo>→</mo>\\n <msup>\\n <mi>e</mi>\\n <mo>+</mo>\\n </msup>\\n <msup>\\n <mi>e</mi>\\n <mo>−</mo>\\n </msup>\\n </mrow>\\n <annotation>$$ U\\\\to {e}^{+}{e}^{-} $$</annotation>\\n </semantics></math>. The production of these <i>U</i>-bosons occurs via Dalitz decays of pions, <i>η</i>-mesons, <i>ω</i>-mesons, Delta resonances, as well as from the decays of vector mesons and <span></span><math>\\n <semantics>\\n <mrow>\\n <msup>\\n <mi>K</mi>\\n <mo>+</mo>\\n </msup>\\n </mrow>\\n <annotation>$$ {K}^{+} $$</annotation>\\n </semantics></math> mesons. This analysis provides an upper limit on <span></span><math>\\n <semantics>\\n <mrow>\\n <msup>\\n <mi>ϵ</mi>\\n <mn>2</mn>\\n </msup>\\n <mfenced>\\n <msub>\\n <mi>M</mi>\\n <mi>U</mi>\\n </msub>\\n </mfenced>\\n </mrow>\\n <annotation>$$ {\\\\upvarepsilon}^2\\\\left({M}_U\\\\right) $$</annotation>\\n </semantics></math> and offers insights into the accuracy required for future experimental searches for dark photons through dilepton experiments.</p>\",\"PeriodicalId\":55442,\"journal\":{\"name\":\"Astronomische Nachrichten\",\"volume\":\"346 3-4\",\"pages\":\"\"},\"PeriodicalIF\":1.0000,\"publicationDate\":\"2024-12-22\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://onlinelibrary.wiley.com/doi/epdf/10.1002/asna.20240132\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Astronomische Nachrichten\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://onlinelibrary.wiley.com/doi/10.1002/asna.20240132\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomische Nachrichten","FirstCategoryId":"101","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1002/asna.20240132","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
摘要
向量u -玻色子,通常被称为“暗光子”,是调解暗物质相互作用的潜在候选者。在这项研究中,我们概述了一个过程,利用SIS到RHIC重离子的双轻子数据推导出动力学混合参数ε 2 M U $$ {\upvarepsilon}^2\left({M}_U\right) $$上界的理论约束能量。该分析基于微观粒子-强子-弦动力学(PHSD)输运模型,该模型成功地再现了p + p $$ p+p $$, p + A $$ p+A $$,和A + A $$ A+A $$碰撞。除了由标准模型粒子(如介子和重子)的相互作用和衰变产生的双轻子通道外,我们还扩展了PHSD方法,将假设的u -玻色子衰变为双轻子,U→e + e−$$ U\to {e}^{+}{e}^{-} $$。这些u -玻色子的产生是通过介子、η介子、ω介子、δ共振的Dalitz衰变以及矢量介子和K + $$ {K}^{+} $$介子的衰变产生的。该分析提供了一个λ 2 M U $$ {\upvarepsilon}^2\left({M}_U\right) $$的上限,并为未来通过双轻子实验搜索暗光子所需的精度提供了见解实验。
Exploring Dark Photon Production and Kinetic Mixing Constraints in Heavy-Ion Collisions
Vector U-bosons, often referred to as “dark photons,” are potential candidates for mediating dark matter interactions. In this study, we outline a procedure to derive theoretical constraints on the upper bound of the kinetic mixing parameter using dilepton data from heavy-ion from SIS to RHIC energies. The analysis is based on the microscopic Parton–Hadron–String Dynamics (PHSD) transport model, which successfully reproduces the measured dilepton spectra in , , and collisions. Besides the dilepton channels resulting from interactions and decays of Standard Model particles (such as mesons and baryons), we extend the PHSD approach to include the decay of hypothetical U-bosons into dileptons, . The production of these U-bosons occurs via Dalitz decays of pions, η-mesons, ω-mesons, Delta resonances, as well as from the decays of vector mesons and mesons. This analysis provides an upper limit on and offers insights into the accuracy required for future experimental searches for dark photons through dilepton experiments.
期刊介绍:
Astronomische Nachrichten, founded in 1821 by H. C. Schumacher, is the oldest astronomical journal worldwide still being published. Famous astronomical discoveries and important papers on astronomy and astrophysics published in more than 300 volumes of the journal give an outstanding representation of the progress of astronomical research over the last 180 years. Today, Astronomical Notes/ Astronomische Nachrichten publishes articles in the field of observational and theoretical astrophysics and related topics in solar-system and solar physics. Additional, papers on astronomical instrumentation ground-based and space-based as well as papers about numerical astrophysical techniques and supercomputer modelling are covered. Papers can be completed by short video sequences in the electronic version. Astronomical Notes/ Astronomische Nachrichten also publishes special issues of meeting proceedings.