Collaborative Research: A Comprehensive Theoretical Study of Cosmic Magnetic Fields, their Origin, Evolution, and Signatures

人们用指南针来了解他们的旅行方向。 这样的指南针之所以能工作，是因为它的微小磁针与地球的磁场对齐，并指示北方的方向。 在比地球大得多的尺度上，我们自己的银河系也有自己的磁场。 事实上，宇宙中的所有星系似乎都有磁场，这些磁场可以对星系的一生产生深远的影响。 通过一系列复杂的计算机模拟，该项目旨在解开星系中磁场的令人费解的起源。 完成后，这个项目可能会指出这些磁场的起源，与宇宙本身的诞生相吻合。 这样的结果可能会对我们目前对基础物理学的理解产生深远的影响，而对它的追求也符合美国在天体物理学领域发展科学领导地位的国家利益。 该项目还将通过直接培训普通和计算天体物理学的本科生和研究生来加强美国的科学劳动力。 项目计划还包括一个强有力的教育和公众宣传计划。更技术性地说，观测表明，星系的磁场中有一个分量在星系的很大一部分上是相干的，场强为微高斯量级。 这些领域被认为是从未知性质的初始弱种子磁场的放大。 它们的起源有两种情况：（1）自下而上的天体物理学情况，其中所需的种子场是在较小的尺度上产生的;（2）自上而下的宇宙学情况，其中种子场是在早期宇宙中星系形成之前在现在的大尺度上产生的。 根据目前的观察，本项目旨在区分这两种情况。 为了实现这一目标，宇宙磁场的演化和观测特征将在不同的天体物理环境，如星系团，星系和星际介质中进行研究。 数值模拟将模拟宇宙磁场在膨胀宇宙中的演化与时变耗散属性时，初始条件对应于不同的情况下的磁。 该项目分为以下相关部分：（i）磁生成机制的理论研究，包括宇宙学和天体物理学情景;（ii）大尺度磁场演化的数值模拟，以分析天体物理学机制是否能导致与下限相当的河外磁场强度;以及（iii）确定大尺度相干宇宙磁场的潜在可观测特征-包括宇宙结构形成、微波背景波动或超高能伽马射线传播。 该项目将寻找原始宇宙磁场的特征，以区分宇宙学种子和天体物理学来源。

People use a compass to learn their direction of travel. Such a compass works because its tiny magnetic needle aligns with the magnetic field of Earth and indicates the direction of North. On scales much larger than Earth, our own Milky Way Galaxy also has its own magnetic field. In fact, all galaxies in the Universe appear to have magnetic fields, and these magnetic fields can have profound effects on a galaxy's development throughout its lifetime. Through a series of sophisticated computer simulations, this project aims to unlock the puzzling origin of the magnetic fields found in galaxies. Upon completion this project might point to an origin of these magnetic fields that coincides with the birth of the Universe itself. Such a result could have a profound influence on our current understanding of fundamental physics, and its pursuit serves the national interest of developing US scientific leadership in astrophysics. This project will also strengthen the US science workforce by directly training undergraduate and graduate students in general and computational astrophysics. Project plans also include a vigorous education and public outreach program.More technically, observations show that galaxies have magnetic fields with a component that is coherent over a large fraction of the galaxy with field strengths of order microgauss. These fields are assumed to be from the amplification of initial weak seed magnetic fields of unknown nature. The two scenarios of their origin are (1) a bottom-up astrophysical one, where the needed seed field is generated on smaller scales and (2) a top-down cosmological scenario where the seed field is generated prior to galaxy formation in the early Universe on scales that are large now. Based on current observations, this project aims to distinguish between these two scenarios. To achieve this goal, the evolution and observational signatures of cosmic magnetic fields will be studied in different astrophysical environments such as clusters, galaxies, and interstellar medium. Numerical simulations will model the evolution of cosmic magnetic fields in the expanding Universe with time varying dissipative properties when initial conditions correspond to the different scenarios of the magnetogenesis. This project is divided into the following related parts: (i) theoretical studies of magnetogenesis mechanisms including the cosmological and astrophysical scenarios; (ii) numerical simulations of large-scale magnetic fields evolution to analyze whether astrophysical mechanisms can lead to extragalactic magnetic field strengths comparable with the lower bounds; and (iii) determining potentially observable signatures of cosmic magnetic fields coherent at large scales---including cosmic structure formation, microwave background fluctuations, or ultra high energy gamma-ray propagation. The project will search for signatures of primordial cosmic magnetic fields that distinguish cosmological seeds from astrophysical sources.