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The Indirect Detection of Non-baryonic Dark Matter

非重子暗物质的间接探测

基本信息

批准号：
ST/G008094/1
负责人：
Daniel Cumberbatch
金额：
$ 29.15万
依托单位：
University of Sheffield
依托单位国家：
英国
项目类别：
Fellowship
财政年份：
2009
资助国家：
英国
起止时间：
2009 至无数据
项目状态：
已结题

来源：
https://gtr.ukri.org/projects?ref=ST%2FG008094%2F1
关键词：
Indirect Detection Non baryonic Dark

项目摘要

My proposed work specifically aims at identifying features within the high-precision spectra of cosmic-ray antiparticles and radiation, provided by both current and future indirect dark matter detection experiments, that cannot be simply understood within a conventional astrophysical scenario. In each of my proposed projects (outlined below), I will apply theoretical modelling and statistical analysis techniques to these spectra and infer constraints on the properties of particularly-suited species of dark matter particles whose annihilation or decay products could result in such features. 1. 'The effect of dark matter on the spatial distribution of the 21cm signal surrounding galaxies and clusters' In this project I plan to continue my investigation of the effect of dark matter on the 21cm hydrogen emission signal, resulting from electronic transitions from the 2p to 1s hyperfine levels of hydrogen atoms residing in the intergalactic medium. In my research I calculated the extent to which the energetic particles resulting from the annihilation of weakly interacting massive particles (or WIMPs) or light dark matter (LDM), assumed to constitute the dark matter thought to surround galaxies, heated, ionised and excited neutral hydrogen in the IGM when acknowledging several generations of dark matter structures. I demonstrated that such interactions could significantly alter the thermal and ionization history of the Universe, and calculated their effects on the global 21cm signal. It was deduced that for certain models of the evolution of dark matter structures, the effects on the global 21cm signal by WIMPs and LDM with certain properties could in principle be detectable by current radio-interferometers such as LOFAR. In my proposed project, instead of focusing on the global 21cm signature, I will now focus on the spatial distribution of the 21cm signal specifically around galaxies and clusters that are to be observed by current radio-interferometers such as LOFAR. The products of dark matter annihilations can significantly heat and ionise the surrounding hydrogen throughout a much larger region than if dark matter was absent, potentially making dark matter much easier to detect. 2. 'Indirect detection of disrupted dark matter substructure using FGST, and the implications for direct detection' Recent results from high-resolution simulations of dark matter halos imply that satellites of WIMP dark matter may be traversing through the Milky Way. WIMP annihilations within these satellites are predicted to yield unique elongated profiles of gamma-rays, acting as a smoking gun signature for satellites. Also, satellites disrupted by tidal forces are predicted to leave residual streams of dark matter in their wakes. Streams passing through the solar neighborhood could significantly enhance the annual signal modulation expected to be measured at direct detection experiments. By using the theoretical models that I have developed to calculate the energy spectra and spatial distribution of gamma-ray emissions resulting from WIMP annihilations within migrating satellites, together with a statistical analysis of the FGST all-sky gamma-ray map, scheduled for development in 2009, I will constrain the properties of WIMPs and make inferences on the lifetime of disrupted satellites. In addition, by using theoretical models for the trajectories of satellites and constraints from direct detection experiments, such as ZEPLIN-II, I will deduce constraints on the degree of mass-stripping suffered by satellites. 3. 'Alternative production mechanisms for sterile neutrino dark matter' My recent research disfavours a scenario where sterile neutrinos, generated through the Dodelson-Widrow mechanism (DWM), constitute all of the currently inferred dark matter abundance. Using new results from XMM and Chandra, I will investigate and deduce constraints on the properties of sterile neutrinos generated by mechanisms alternative to the DWM.

我提出的工作专门针对识别宇宙射线反粒子和辐射的高精度光谱内的特征，这些特征由当前和未来的间接暗物质探测实验提供，不能简单地在传统的天体物理学场景中理解。在我提出的每一个项目中（如下所述），我将对这些光谱应用理论建模和统计分析技术，并推断出对暗物质粒子的特殊合适种类的性质的约束，这些暗物质粒子的湮灭或衰变产物可能导致这种特征。1.“暗物质对周围星系和星系团的21厘米信号的空间分布的影响”在这个项目中，我计划继续研究暗物质对21厘米氢发射信号的影响，这是由于星系际介质中氢原子的2 p到1 s超精细能级的电子跃迁造成的。在我的研究中，我计算了弱相互作用大质量粒子（或WIMPs）或轻暗物质（LDM）湮灭产生的高能粒子的程度，假设构成被认为围绕星系的暗物质，在IGM中加热，电离和激发中性氢时承认几代暗物质结构。我证明了这种相互作用可以显著改变宇宙的热和电离历史，并计算了它们对全球21厘米信号的影响。据推断，对于暗物质结构演化的某些模型，具有某些性质的WIMP和LDM对全球21 cm信号的影响原则上可以通过现有的无线电干涉仪（如LOFAR）检测到。在我提议的项目中，我现在将重点关注21厘米信号的空间分布，而不是关注全球21厘米信号，特别是星系和星系团周围的21厘米信号，这些信号将被目前的无线电干涉仪（如LOFAR）观测到。暗物质湮灭的产物可以显着加热和电离周围的氢在一个更大的区域比如果暗物质不存在，可能使暗物质更容易检测。2.“使用FGST间接探测被破坏的暗物质子结构，以及直接探测的意义”最近对暗物质晕进行高分辨率模拟的结果表明，WIMP暗物质的卫星可能正在穿越银河系。预计这些卫星内的WIMP湮灭将产生独特的伽马射线拉长剖面，作为卫星的吸烟枪签名。此外，被潮汐力破坏的卫星预计会在尾流中留下残余的暗物质流。通过太阳附近的流可以显着增强预期在直接探测实验中测量的年度信号调制。通过使用的理论模型，我已经开发出计算的能量谱和空间分布的伽马射线辐射造成的WIMP湮灭内迁移的卫星，连同FGST的全天空伽马射线地图，定于2009年开发的统计分析，我将限制的WIMP的属性和中断卫星的寿命作出推断。此外，通过使用卫星轨道的理论模型和直接探测实验的约束条件，如ZEPLIN-II，我将推导出卫星所遭受的质量剥离程度的约束条件。3.我最近的研究不赞成这样一种情况，即通过Dodelson-Widrow机制（DWM）产生的无菌中微子构成了目前推断的所有暗物质丰度。利用XMM和钱德拉的新结果，我将调查和推导出的限制机制替代DWM产生的无菌中微子的属性。