{"title":"Magnetic field in relativistic heavy-ion collisions: Testing the classical approximation","authors":"I. Danhoni, F. Navarra","doi":"10.1103/PHYSREVC.103.024902","DOIUrl":null,"url":null,"abstract":"It is believed that in non-central relativistic heavy ion collisions a very strong magnetic field is formed. There are several studies of the effects of this field, where $\\vec{B}$ is calculated with the expressions of classical electrodynamics. A quantum field may be approximated by a classical one when the number of field quanta in each field mode is sufficiently high. This may happen if the field sources are intense enough. In heavy ion physics the validity of the classical treatment was not investigated. In this work we propose a test of the quality of the classical approximation. We calculate an observable quantity using the classical magnetic field and also using photons as input. If the results of both approaches coincide, this will be an indication that the classical approximation is valid. More precisely, we focus on the process in which a nucleon is converted into a delta resonance, which then decays into another nucleon and a pion, i.e., $ N \\to \\Delta \\to N' \\pi$. In ultra-peripheral relativistic heavy ion collisions this conversion can be induced by the classical magnetic field of one the ions acting on the other ion. Alternatively, we can replace the classical magnetic field by a flux of equivalent photons, which are absorbed by the target nucleons. We calculate the cross sections in these two independent ways and find that they differ from each other by $\\simeq 10$ \\% in the considered collision energy range. This suggests that the two formalisms are equivalent and that the classical approximation for the magnetic field is reasonable.","PeriodicalId":8457,"journal":{"name":"arXiv: High Energy Physics - Phenomenology","volume":"25 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2020-10-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"3","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv: High Energy Physics - Phenomenology","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1103/PHYSREVC.103.024902","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 3
Abstract
It is believed that in non-central relativistic heavy ion collisions a very strong magnetic field is formed. There are several studies of the effects of this field, where $\vec{B}$ is calculated with the expressions of classical electrodynamics. A quantum field may be approximated by a classical one when the number of field quanta in each field mode is sufficiently high. This may happen if the field sources are intense enough. In heavy ion physics the validity of the classical treatment was not investigated. In this work we propose a test of the quality of the classical approximation. We calculate an observable quantity using the classical magnetic field and also using photons as input. If the results of both approaches coincide, this will be an indication that the classical approximation is valid. More precisely, we focus on the process in which a nucleon is converted into a delta resonance, which then decays into another nucleon and a pion, i.e., $ N \to \Delta \to N' \pi$. In ultra-peripheral relativistic heavy ion collisions this conversion can be induced by the classical magnetic field of one the ions acting on the other ion. Alternatively, we can replace the classical magnetic field by a flux of equivalent photons, which are absorbed by the target nucleons. We calculate the cross sections in these two independent ways and find that they differ from each other by $\simeq 10$ \% in the considered collision energy range. This suggests that the two formalisms are equivalent and that the classical approximation for the magnetic field is reasonable.
据信,在非中心相对论性重离子碰撞中,会形成一个非常强的磁场。有几个研究这个场的影响,其中$\vec{B}$是用经典电动力学的表达式计算的。当每个场模式中的场量子数足够高时,可以用经典场来近似量子场。如果磁场源足够强,就可能发生这种情况。在重离子物理学中,经典处理的有效性没有得到研究。在这项工作中,我们提出了经典近似质量的检验。我们使用经典磁场和光子作为输入来计算一个可观察的量。如果两种方法的结果一致,这将表明经典近似是有效的。更准确地说,我们关注的是一个核子转化为δ共振的过程,δ共振然后衰变为另一个核子和一个介子,即$ N \to \Delta \to N' \pi$。在超外围相对论性重离子碰撞中,这种转换可以由一个离子作用于另一个离子的经典磁场引起。或者,我们可以用等效光子的通量代替经典磁场,这些光子被目标核子吸收。我们用这两种独立的方法计算截面,发现它们在考虑的碰撞能量范围内相差$\simeq 10$ %。这表明这两种形式是等价的,并且磁场的经典近似是合理的。