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Gravitation Between Spherically Symmetric Masses01:14

Gravitation Between Spherically Symmetric Masses

The gravitational potential energy between two spherically symmetric bodies can be calculated from the masses and the distance between the bodies, assuming that the center of mass is concentrated at the respective centers of the bodies.
Schwarzschild Radius and Event Horizon01:21

Schwarzschild Radius and Event Horizon

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 velocity with the...
Detection of Black Holes01:10

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...
Reduced Mass Coordinates: Isolated Two-body Problem01:12

Reduced Mass Coordinates: Isolated Two-body Problem

In classical mechanics, the two-body problem is one of the fundamental problems describing the motion of two interacting bodies under gravity or any other central force. When considering the motion of two bodies, one of the most important concepts is the reduced mass coordinates, a quantity that allows the two-body problem to be solved like a single-body problem. In these circumstances, it is assumed that a single body with reduced mass revolves around another body fixed in a position with an...
Rocket Propulsion in Gravitational Field - II01:03

Rocket Propulsion in Gravitational Field - II

A rocket's velocity in the presence of a gravitational field is decreased by the amount of force exerted by Earth's gravitational field, which opposes the motion of the rocket. If we consider thrust, that is, the force exerted on a rocket by the exhaust gases, then a rocket's thrust is greater in outer space than in the atmosphere or on a launch pad. In fact, gases are easier to expel in a vacuum.
A rocket's acceleration depends on three major factors, consistent with the equation for the...
Rocket Propulsion in Gravitational Field - I01:20

Rocket Propulsion in Gravitational Field - I

Rockets range in size from small fireworks that ordinary people use to the enormous Saturn V that once propelled massive payloads toward the Moon. The propulsion of all rockets, jet engines, deflating balloons, and even squids and octopuses are explained by the same physical principle: Newton's third law of motion. The matter is forcefully ejected from a system, producing an equal and opposite reaction on what remains.
The motion of a rocket in space changes its velocity (and hence its...

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Video Experimental Relacionado

Updated: May 11, 2026

Generation and Coherent Control of Pulsed Quantum Frequency Combs
06:42

Generation and Coherent Control of Pulsed Quantum Frequency Combs

Published on: June 8, 2018

Un púlsar masivo en un binario relativista compacto.

John Antoniadis1, Paulo C C Freire, Norbert Wex

  • 1Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, Bonn, Germany. jantoniadis@mpifr-bonn.mpg.de

Science (New York, N.Y.)
|April 27, 2013
PubMed
Resumen
Este resumen es generado por máquina.

Se midió un púlsar masivo de 2,01 masas solares que orbita una enana blanca. Su desintegración orbital coincide con la relatividad general, validando la teoría de Einstein en condiciones de gravedad extrema.

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Generation and Coherent Control of Pulsed Quantum Frequency Combs
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Área de la Ciencia:

  • La astrofísica es la astrofísica.
  • Relatividad general La relatividad general.
  • Las ondas gravitacionales son ondas gravitacionales.

Sus antecedentes:

  • Las extensiones de la relatividad general predicen desviaciones del espacio-tiempo alrededor de estrellas de neutrones masivas.
  • Probar la gravedad de campo fuerte requiere mediciones precisas en entornos extremos.

Objetivo del estudio:

  • Para medir la masa de un púlsar en un sistema binario compacto.
  • Para probar la validez de la relatividad general en un régimen de campo fuerte.
  • Para restringir las desviaciones de la relatividad general y las propiedades de la materia densa.

Principales métodos:

  • Astronomía observacional utilizando el tiempo de pulsar.
  • Análisis del decaimiento orbital en un sistema binario compuesto por un púlsar y una enana blanca.

Principales resultados:

  • Se determinó una masa de púlsar de 2,01 ± 0,04 masas solares.
  • El decaimiento orbital observado es consistente con las predicciones de la relatividad general.
  • Se establecieron restricciones a las desviaciones de la relatividad general.

Conclusiones:

  • La relatividad general sigue siendo válida bajo condiciones gravitatorias extremas.
  • Las plantillas basadas en GR son adecuadas para detectores de ondas gravitacionales.
  • El estudio proporciona información sobre la materia densa, la astrofísica estelar binaria y el reciclaje de los púlsares.