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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.
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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...
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Detection of Black Holes01:10

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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...
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Atomic Emission Spectroscopy: Overview01:20

Atomic Emission Spectroscopy: Overview

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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...
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Schwarzschild Radius and Event Horizon01:21

Schwarzschild Radius and Event Horizon

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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...
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Thomson's e/m Experiment01:19

Thomson's e/m Experiment

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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...
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Las curvas de luz de supernova de envolvente despojado argumentan por la actividad del motor central

Ósmar Rodríguez1, Ehud Nakar2, Dan Maoz1

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

Nature
|April 17, 2024
PubMed
Resumen

Las supernovas de envoltura despojada pueden tener una fuente de energía no radiactiva. El análisis de 54 supernovas sugiere que un motor central, posiblemente formando magnetares, impulsa estas explosiones estelares.

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Área de la Ciencia:

  • Astronomía y astrofísica
  • Evolución estelar
  • Física de las supernovas

Sus antecedentes:

  • Las supernovas de envoltura despojada (SESNe) son explosiones estelares comunes.
  • Su luminosidad se atribuye principalmente a la desintegración radiactiva del níquel.
  • Estudios anteriores sugirieron fuentes de energía adicionales, pero carecían de significación estadística o dependían del modelo.

Objetivo del estudio:

  • Para investigar el presupuesto energético de SESNe.
  • Encontrar pruebas observacionales de fuentes de energía no radiactivas en SESNe.
  • Para limitar las propiedades de los potenciales motores centrales.

Principales métodos:

  • Análisis del presupuesto energético de 54 SESN bien observados.
  • Comparaciones observacionales independientes del modelo.
  • Evaluación de posibles fuentes de energía y errores sistemáticos.

Principales resultados:

  • Evidencia estadísticamente significativa de una fuente de energía no radiactiva en la mayoría de los SESNe.
  • Esta fuente de energía probablemente proviene de un motor central de larga duración (10^3-10^6 s después de la explosión).
  • Si el motor es un magnetar, los campos magnéticos iniciales son de ~ 10 ^ 15 G y los períodos de rotación son de 1-100 ms.

Conclusiones:

  • SESNe probablemente posee un motor central más allá de la descomposición radiactiva.
  • Este motor puede ser responsable de la formación de magnetares.
  • Investigaciones adicionales pueden refinar las propiedades de estos motores.