相关实验视频
Updated: Jul 8, 2026

07:46
Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
缺失的巴里翁和温暖的星系间介质
Fabrizio Nicastro1, Smita Mathur, Martin Elvis
1Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA. fnicastro@cfa.harvard.edu
概括
宇宙学家正在寻找缺失的巴里昂,这些巴里昂被认为存在于一个温暖的热的星系间介质中. 发现这些难以捉摸的宇宙成分是验证我们对宇宙的理解的关键.
科学领域:
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
- 星系间介质 星系间介质
背景情况:
- 可观测的宇宙只包含预期的一半的重子物质.
- 假设大多数重子存在于一个热热的星系间介质 (WHIM).
- 这种缺失的物质被认为是在宇宙结构形成过程中受到冲击加热.
研究的目的:
- 为了找到宇宙中缺失的 baryons.
- 为了创建一个完整的库存的baryonic物质.
- 为了测试标准宇宙学模型.
主要方法:
- 观测天文学是一种观测天文学.
- 宇宙学模拟的宇宙学模拟.
- 对星系间气体特性进行分析.
主要成果:
- 该研究的重点是缺失的巴里昂的理论分布.
- 它强调了温暖热的星系间介质的预期性质.
- 它强调了观察证据的必要性.
结论:
- 确认缺失的子的存在和分布至关重要.
- 这项研究影响了我们对标准宇宙学模型的验证.
- 需要进一步的观测努力来检测温暖热的星系间介质.
相关概念视频
Detection of Black Holes
Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
Real Gases: Effects of Intermolecular Forces and Molecular Volume Deriving Van der Waals Equation
Thus far, the ideal gas law, PV = nRT, has been applied to a variety of different types of problems, ranging from reaction stoichiometry and empirical and molecular formula problems to determining the density and molar mass of a gas. However, the behavior of a gas is often non-ideal, meaning that the observed relationships between its pressure, volume, and temperature are not accurately described by the gas laws.
Heat Capacities of an Ideal Gas II
For a system that undergoes a thermodynamic process at a constant volume condition, the heat absorbed is used only to increase the system's internal energy and not for doing any kind of work. While for a system undergoing a thermodynamic process under a constant pressure condition, the amount of heat absorbed is used not only for increasing the internal energy (as a function of temperature) but also for doing some work. The molar heat capacity is the amount of heat required to increase the...
Heat Capacities of an Ideal Gas III
The number of independent ways a gas molecule can move along straight line, rotate, and vibrate is called its degrees of freedom. Supposing d represents the number of degrees of freedom of an ideal gas, the molar heat capacity at constant volume of an ideal gas in terms of d is
Radiation: Applications
The average temperature of Earth is the subject of much current discussion. Earth is in radiative contact with both the Sun and dark space; it receives almost all its energy from the radiation of the Sun and reflects some of it into outer space. Dark space is very cold, about 3 K, so Earth radiates energy into it. For instance, heat transfer occurs from soil and grasses, the rate of which can be so rapid that frost can occur on clear summer evenings, even in warm latitudes.
The average...
The average...
Heat Capacities of an Ideal Gas I
Heat capacity is the ratio of heat absorbed by the substance corresponding to its temperature change. It is also called thermal capacity and the SI unit of heat capacity is J/K. Whereas, specific heat capacity is defined as the amount of heat necessary to change the temperature of 1 kg of a substance by 1 K and is also called massic heat capacity. Its SI unit is J/kg⋅K.
Molar heat capacity quantifies the ratio of the amount of heat added (or removed) to increase (or decrease) the temperature of...
Molar heat capacity quantifies the ratio of the amount of heat added (or removed) to increase (or decrease) the temperature of...

