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関連する概念動画

Emission Spectra02:39

Emission Spectra

52.3K
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.
52.3K
Nuclear Fusion02:45

Nuclear Fusion

19.6K
The process of converting very light nuclei into heavier nuclei is also accompanied by the conversion of mass into large amounts of energy, a process called fusion. The principal source of energy in the sun is a net fusion reaction in which four hydrogen nuclei fuse and ultimately produce one helium nucleus and two positrons.
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
19.6K
Detection of Black Holes01:10

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...
2.2K
Atomic Emission Spectroscopy: Overview01:20

Atomic Emission Spectroscopy: Overview

2.1K
Atomic emission spectroscopy (AES) is an analytical technique used to determine the elemental composition of a sample by analyzing the light emitted from excited atoms. In AES, atoms in a sample are excited to higher energy levels by thermal energy from high-temperature sources, such as plasma, arcs, or sparks. When these excited atoms return to lower energy states, they emit light at specific wavelengths characteristic of each element. The resulting atomic emission spectrum, which consists of...
2.1K
Schwarzschild Radius and Event Horizon01:21

Schwarzschild Radius and Event Horizon

2.0K
No object with a finite mass can travel faster than the speed of light in a vacuum. This fact has an interesting consequence in the domain of extremely high gravitational fields.
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape...
2.0K
Thomson's e/m Experiment01:19

Thomson's e/m Experiment

3.6K
In a beam of charged particles created by a heated cathode, the particles move at different speeds. However, many applications need a beam with uniform particle speeds. An arrangement known as a velocity selector uses electric and magnetic fields to pick particles with a particular speed from the beam.
A particle with charge q, speed v, and mass m enters an area from the top, where the magnetic and electric fields are perpendicular both to the particle's motion and to one another. The...
3.6K

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関連する実験動画

Updated: Jun 28, 2025

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
06:48

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves

Published on: May 10, 2020

3.5K

超新星 の 光 の 曲線 は 中心 の エンジン の 活動 を 示す

Ósmar Rodríguez1, Ehud Nakar2, Dan Maoz1

  • 1School of Physics and Astronomy, Tel-Aviv University, Tel-Aviv, Israel.

Nature
|April 17, 2024
PubMed
まとめ

超新星には非放射性エネルギー源がある. 54個の超新星を分析した結果 磁星を形成している 中央のエンジンが 爆発の原動力になっていることが分かりました

科学分野:

  • 天文学と天体物理学
  • スター進化
  • 超新星物理学

背景:

  • 脱落型超新星 (SESNe) は恒星の爆発が一般的である.
  • その輝きは主に放射性ニッケル崩壊に起因します
  • 以前の研究では,追加のエネルギー源が示唆されたが,統計的に有意でないか,モデルに依存していた.

研究 の 目的:

  • SESNeのエネルギー予算を調査する
  • SESNeの非放射性エネルギー源の観測証拠を見つけるために.
  • 中央エンジンの性質を制限する.

主な方法:

  • 54のよく観察されたSESNeのエネルギー予算の分析
  • モデル独立の観測比較
  • 可能なエネルギー源と体系的なエラーの評価

主要な成果:

  • ほとんどのSESNeでは非放射性エネルギー源の統計的に有意な証拠がある.
  • 爆発後10^3~10^6秒の 寿命が長い 中央エンジンから発生したものです
  • エンジンがマグネタールである場合,初期磁場は ~ 10 ^ 15 G で,回転周期は 1 ~ 100 ms です.

さらに関連する動画

Setting Limits on Supersymmetry Using Simplified Models
07:46

Setting Limits on Supersymmetry Using Simplified Models

Published on: November 15, 2013

8.6K
Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
11:20

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses

Published on: July 2, 2012

15.0K

関連する実験動画

Last Updated: Jun 28, 2025

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
06:48

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves

Published on: May 10, 2020

3.5K
Setting Limits on Supersymmetry Using Simplified Models
07:46

Setting Limits on Supersymmetry Using Simplified Models

Published on: November 15, 2013

8.6K
Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
11:20

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses

Published on: July 2, 2012

15.0K

結論:

  • SESNeは,放射性崩壊を超えた 中央エンジンを持っている可能性が高い.
  • このエンジンは磁星の形成に 責任があるかもしれません
  • このエンジンの性質をさらに研究することで 精錬できるでしょう