相关实验视频
Updated: Jun 30, 2025

07:46
Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
8.6K
来自西弗特星系群的中微子信号
A Neronov1,2, D Savchenko1,3,4, D V Semikoz1
1Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France.
Physical review letters
|March 22, 2024
概括
研究人员发现了来自两个额外的赛弗特星系NGC 4151和NGC 3079中微子信号的证据. 这加强了西弗特星系是宇宙中微子的重要来源的假设.
科学领域:
- 天体物理学 天体物理学
- 粒子物理学 粒子物理学
- 宇宙中微子天文学
背景情况:
- 冰块中微子天文台此前曾探测到来自西弗特星系NGC 1068的中微子信号.
- 这一观察表明,赛弗特星系可能是高能中微子的常见来源.
研究的目的:
- 为了研究所有赛弗特星系都发射中微子的假设.
- 为了识别和测试其他附近的赛弗特星系作为潜在的中微子来源.
主要方法:
- 根据硬X射线特性选择候选中性子源.
- 对十年来公开可用的IceCube数据集的分析.
- 统计分析以评估观察到的中微子过量的重要性.
主要成果:
- 在NGC 4151和NGC 3079.9中发现了中微子信号 (约3西格玛) 的证据.
- 没有一个来源单独达到发现值.
- 包括NGC 1068在内的选定来源中观察这些过度的综合概率小于2.6x10^-7.
结论:
- 建立了赛弗特星系和中微子辐射之间的统计学意义上的相关性.
- 这些发现支持这样一个观点,即赛弗特星系是天体物理学中微子流的重要贡献者.
- 需要进一步的观测来确认个别的来源发现.
相关概念视频
Atomic Nuclei: Nuclear Spin State Population Distribution
974
Near absolute zero temperatures, in the presence of a magnetic field, the majority of nuclei prefer the lower energy spin-up state to the higher energy spin-down state. As temperatures increase, the energy from thermal collisions distributes the spins more equally between the two states. The Boltzmann distribution equation gives the ratio of the number of spins predicted in the spin −½ (N−) and spin +½ (N+) states.
974
Atomic Emission Spectroscopy: Interference
183
In atomic emission spectroscopy (AES), high-temperature atomizers excite a broad range of elements and molecules that generate complex emissions from sources such as oxides, hydroxides, and flame combustion products in the flame or plasma. Several strategies can be employed to minimize spectral interferences caused by overlapping emission lines or bands. These include increasing instrument resolution, choosing alternative emission lines, optimally placing the detector in low-background regions,...
183
Fermi Level Dynamics
245
The vacuum level denotes the energy threshold required for an electron to escape from a material surface. It is usually positioned above the conduction band of a semiconductor and acts as a benchmark for comparing electron energies within various materials.
Electron affinity in semiconductors refers to the energy gap between the minimum of its conduction band and the vacuum level and it is a critical parameter in determining how easily a semiconductor can accept additional electrons.
The work...
Electron affinity in semiconductors refers to the energy gap between the minimum of its conduction band and the vacuum level and it is a critical parameter in determining how easily a semiconductor can accept additional electrons.
The work...
245
Detection of Black Holes
2.2K
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...
2.2K
Atomic Nuclei: Larmor Precession Frequency
1.3K
The earth's gravitational field produces a 'twisting force' perpendicular to the angular momentum of a spinning mass (such as a spinning top) that causes the mass to 'wobble' around the gravitational field axis in a phenomenon called precession. Similarly, the magnetic moment (μ) of a spinning nucleus precesses due to an external magnetic field directed along the z-axis. The precession of the magnetic moment vector about the magnetic field is called Larmor precession,...
1.3K
Emission Spectra
52.4K
When solids, liquids, or condensed gases are heated sufficiently, they radiate some of the excess energy as light. Photons produced in this manner have a range of energies, and thereby produce a continuous spectrum in which an unbroken series of wavelengths is present.
52.4K

