XAO OpenIR  > 射电天文研究室  > 理论天体物理研究团组
星系尺度上的玻色暗物质研究进展
Alternative TitleResearch Progresses on Galactic Scale Boson Dark Matter
沙艾德·艾力1,2; 唐宇航2,3; 杨术银2,3; 吾尔尼沙·依明尼亚孜1; 杨晓峰2,4
2024-09-01
Source Publication天文学进展
ISSN1000-8349
Volume42Issue:3Pages:443-459
Contribution Rank2
Abstract星系尺度上的暗物质研究通常涉及各种不同的暗物质模型。在这些模型中,冷暗物质模型(CDM模型)受到了广泛关注。基于该理论模型的研究,可以较好地解释星系尺度和宇宙大尺度结构中的一些问题。然而,在研究星系小尺度结构时,存在一些该模型无法解释的观测现象。近年来,玻色-爱因斯坦凝聚暗物质模型(BEC-DM模型)和模糊暗物质模型(FDM模型)作为CDM模型的替代方案,受到了广泛关注和大量研究。在BEC-DM模型中,暗物质粒子被假设为一种处于宏观量子态的玻色子;而FDM模型则将暗物质描述为一个具有波动特性和极小质量的粒子。研究这两种理论模型有助于了解不同理论模型对星系中暗物质密度分布和相关性质的影响。在这一背景下,对星系尺度上的玻色暗物质理论模型及其粒子探测进行了简要概述。回顾了暗物质研究的历史,介绍了暗物质候选粒子及对其的探测方法。重点介绍了BEC-DM模型和FDM模型作为传统CDM模型的替代方案,并探讨了它们在解决问题方面的优势。
Other AbstractIn the past years, the cold dark matter (CDM) model has been extensively studied and provided a theoretical frameworks which offers an excellent explanation for severa l issues related to galaxies and the large-scale structure of universe. However, there are few challenges currently from observational phenomena in small scale with galaxies in the CDM model’s frameworks. Alternative approaches to the CDM model have been proposed and obtained some considerable attention. These progresses include the Bose-Einstein condensate dark matter (BEC-DM) model and the fuzzy dark matter (FDM) model. In BEC-DM model, dark matter particles are assumed to be a kind of boson in a macroscopic quantum state. On the other hand, the FDM model describes the dark matter as a particle which has wave-like properties and assumes its mass is smaller. Studies on these two theoretical models help us to understand the effects of different theoretical models on the density distribution and related properties of galaxies. This paper reviews the historical developments of dark matter research, introduces several dark matter particle candidates and their detection methods. Particularly, we present a detailed review on detection experiments for axion-like particles.
Keyword玻色-爱因斯坦凝聚暗物质模型 模糊暗物质模型 冷暗物质模型 类轴子
DOI10.3969/j.issn.1000-8349.2024.03.03
URL查看原文
Indexed ByCSCD ; 中文核心期刊要目总览
Language中文
WOS IDCSCD:7834202
CSCD IDCSCD:7834202
Citation statistics
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/7591
Collection射电天文研究室_理论天体物理研究团组
Affiliation1.新疆大学物理科学与技术学院,乌鲁木齐 830046;
2.中国科学院新疆天文台,乌鲁木齐 830011;
3.西华师范大学物理与天文学院,南充 637000;
4.中国科学院大学,北京 100049
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
沙艾德·艾力,唐宇航,杨术银,等. 星系尺度上的玻色暗物质研究进展[J]. 天文学进展,2024,42(3):443-459.
APA 沙艾德·艾力,唐宇航,杨术银,吾尔尼沙·依明尼亚孜,&杨晓峰.(2024).星系尺度上的玻色暗物质研究进展.天文学进展,42(3),443-459.
MLA 沙艾德·艾力,et al."星系尺度上的玻色暗物质研究进展".天文学进展 42.3(2024):443-459.
Files in This Item:
File Name/Size DocType Version Access License
沙艾德·艾力-2024-星系尺度上的玻色(490KB)期刊论文出版稿开放获取CC BY-NC-SAView Application Full Text
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[沙艾德·艾力]'s Articles
[唐宇航]'s Articles
[杨术银]'s Articles
Baidu academic
Similar articles in Baidu academic
[沙艾德·艾力]'s Articles
[唐宇航]'s Articles
[杨术银]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[沙艾德·艾力]'s Articles
[唐宇航]'s Articles
[杨术银]'s Articles
Terms of Use
No data!
Social Bookmark/Share
File name: 沙艾德·艾力-2024-星系尺度上的玻色暗物质研究进展.pdf
Format: Adobe PDF
This file does not support browsing at this time
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.