Intra cluster MAGnetic fields origiNATing from star formatION processes

星系团是宇宙中最大的准平衡物体，这使得它们对宇宙学和天体物理学来说非常有趣。在这些系统中，非热成分，如磁场和高能粒子，记录了从早期到现在的过程。这些成分通过控制星团大气内部的传输过程发挥关键作用，并且是额外压力和能量支持的来源。这项提议的目标是将ICM的播种与恒星形成过程和AGN活动驱动的磁场结合起来。磁场与冷却和恒星形成过程的耦合将使我们能够研究磁场在星团中心所谓的冷却流区域的动力学重要性，也可能在原始星系环境中，并将大大有助于我们对这些系统的全局动力学的理解。这将（第一次）在完全自洽的宇宙MHD模拟中完成。所得到的ICM的磁化强度也将与最近和即将到来的无线电波段观测结果进行比较。该项目是在一个已经实施的国际合作网络中进行的，也将允许博士生交换，作为他们培训的一部分，并将他们整合到这种国际合作中。

Galaxy clusters are the largest, quasi-equilibrium objects in the Universe, making them extraordinarily interesting for cosmology and astrophysics. In these systems, non-thermal components such as magnetic field and high energy particles keep a record of the processes acting since early times till now. These components play key roles by controlling transport processes inside the cluster atmosphere and are sources of additional pressure and energy support. The goal of this proposal is to incorporate the seeding of the ICM with magnetic fields driven by star formation processes and AGN activity. Coupling the magnetic field to the cooling and star formation processes will allow us to study the dynamical importance of magnetic fields in the so-called cooling flow regions in the centers of clusters but also potentially in the proto galactic environments and will significantly contribute to our understanding of the global dynamics of these systems. This will be done (for the first time) within fully self consistent, cosmological MHD simulations. The resulting magnetization of the ICM will also be compared with recent and forthcoming observations in radio band. The project is carried out within an already implemented, international network of collaborations and also will allow an exchange of PhD students as part of their training as well as to integrate them into such international collaborations.