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Nuclear Fusion02:45

Nuclear Fusion

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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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Nuclear Transmutation03:20

Nuclear Transmutation

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Nuclear transmutation is the conversion of one nuclide into another. It can occur by the radioactive decay of a nucleus, or the reaction of a nucleus with another particle. The first manmade nucleus was produced in Ernest Rutherford’s laboratory in 1919 by a transmutation reaction, the bombardment of one type of nuclei with other nuclei or with neutrons. Rutherford bombarded nitrogen-14 atoms with high-speed α particles from a natural radioactive isotope of radium and observed...
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Atomic Nuclei: Larmor Precession Frequency01:11

Atomic Nuclei: Larmor Precession Frequency

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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,...
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Nuclear Fission02:50

Nuclear Fission

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Many heavier elements with smaller binding energies per nucleon can decompose into more stable elements that have intermediate mass numbers and larger binding energies per nucleon—that is, mass numbers and binding energies per nucleon that are closer to the “peak” of the binding energy graph near 56. Sometimes neutrons are also produced. This decomposition of a large nucleus into smaller pieces is called fission. The breaking is rather random with the formation of a large...
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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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Atomic Nuclei: Nuclear Relaxation Processes01:23

Atomic Nuclei: Nuclear Relaxation Processes

782
In the absence of an external magnetic field, nuclear spin states are degenerate and randomly oriented. When a magnetic field is applied, the spins begin to precess and orient themselves along (lower energy) or against (higher energy) the direction of the field. At equilibrium, a slight excess population of spins exists in the lower energy state. Because the direction of the magnetic field is fixed as the z-axis,  the precessing magnetic moments are randomly oriented around the z-axis.
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Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
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Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses

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Una fuente de radio transitoria consistente con una supernova de colapso del núcleo desencadenada por la fusión

D Z Dong1, G Hallinan1, E Nakar2

  • 1Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA 91125, USA.

Science (New York, N.Y.)
|September 13, 2021
PubMed
Resumen

Descubrimos un transitorio luminoso de radio de una potencial supernova impulsada por la fusión. Este evento muestra los primeros chorros relativistas y la interacción tardía, apoyando las teorías de explosiones estelares inducidas por binarios.

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Área de la Ciencia:

  • La astrofísica
  • Evolución estelar
  • Productos explosivos transitorios

Sus antecedentes:

  • Las supernovas de colapso del núcleo son el resultado del cese de la fusión nuclear en estrellas masivas.
  • Las fusiones de compañeras binarias se teorizan para interrumpir la fusión antes, desencadenando supernovas.
  • Los transitorios de radio ofrecen información sobre las eyecciones de supernovas y los entornos de interacción.

Objetivo del estudio:

  • Para reportar el descubrimiento y análisis de un transitorio luminoso de radio, VT J121001+495647.
  • Investigar el vínculo potencial entre las interacciones binarias y las características de la supernova.
  • Para probar las predicciones teóricas de explosiones de supernovas impulsadas por la fusión.

Principales métodos:

  • Utilizamos los datos del Very Large Array Sky Survey para detectar el transitorio de radio.
  • Analizó la emisión de radio para inferir las propiedades de las eyecciones de supernovas y la interacción con el material circundante.
  • Asocié el transitorio de radio con un transitorio de rayos X de archivo para identificar la actividad del chorro relativista.

Principales resultados:

  • Detectado un transitorio luminoso de radio, VT J121001+495647, exhibiendo una emisión consistente con la colisión con la cáscara de eyección.
  • La evidencia sugiere la presencia de una cubierta densa de material expulsado por la interacción binaria antes de la supernova.
  • La asociación con un transitorio de rayos X indica el lanzamiento de un chorro relativista durante la explosión.

Conclusiones:

  • El transitorio de radio observado y el evento de rayos X asociado apoyan la hipótesis de una supernova impulsada por la fusión.
  • La combinación de chorro relativista temprano y interacción densa tardía se alinea con los modelos teóricos de explosiones inducidas por binarios.
  • Este descubrimiento proporciona evidencia observacional de una vía alternativa para el colapso del núcleo de las supernovas.