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The Uncertainty Principle04:08

The Uncertainty Principle

Werner Heisenberg considered the limits of how accurately one can measure properties of an electron or other microscopic particles. He determined that there is a fundamental limit to how accurately one can measure both a particle’s position and its momentum simultaneously. The more accurate the measurement of the momentum of a particle is known, the less accurate the position at that time is known and vice versa. This is what is now called the Heisenberg uncertainty principle. He mathematically...
Mass and Weight01:19

Mass and Weight

Mass and weight are often used interchangeably in everyday conversation. For example,  medical records often show our weight in kilograms, but never in the correct units of newtons. In physics, however, there is an important distinction. Weight is the pull of the Earth on an object. It depends on the distance from the center of the Earth. Weight dramatically varies if we leave the Earth's surface, unlike mass, which does not vary with location. On the Moon, for example, the acceleration due to...
Newton's Law of Gravitation01:15

Newton's Law of Gravitation

Our everyday observation tells us that all objects close to the Earth naturally tend to fall to the ground. Early philosophers assumed that this downward force was unique to Earth. By the 16th century, Nicolaus Copernicus (1473-1543) put forward the heliocentric theory, which suggested that Earth and other planets orbited the sun, while the Moon orbited the Earth. However, it was Isaac Newton (1642-1727) who linked these two motions together in the 17th century. He reasoned that the force of...
Gravity between Spherical Bodies01:27

Gravity between Spherical Bodies

Newton's law of gravitation describes the gravitational force between any two point masses. However, for extended spherical objects like the Earth, the Moon, and other planets, the law holds with an assumption that masses of spherical objects are concentrated at their respective centers.
This assumption can be proved easily by showing that the expression for gravitational potential energy between a hollow sphere of mass (M) and a point mass (m) is the same as it would be for a pair of extended...
The Principle of Superposition and the Gravitational Field01:17

The Principle of Superposition and the Gravitational Field

The principle of superposition applies to gravitational forces of objects that are sufficiently far apart. It states that the net gravitational force on a point object is the vector sum of the gravitational forces on it due to various objects. The principle helps calculate the force by listing the individual forces and then vectorially summing them up. However, it should be noted that the principle of superposition is not always apparent. In the presence of a second force, the first force could...
Mass and Weight01:19

Mass and Weight

Mass and weight are often used interchangeably in everyday conversation. For example,  medical records often show our weight in kilograms, but never in the correct units of newtons. In physics, however, there is an important distinction. Weight is the pull of the Earth on an object. It depends on the distance from the center of the Earth. Weight dramatically varies if we leave the Earth's surface, unlike mass, which does not vary with location. On the Moon, for example, the acceleration due to...

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Video Experimental Relacionado

Updated: Jul 18, 2026

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
09:44

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System

Published on: June 5, 2014

Física de las astropartículas y cosmología.

Simon Mitton1

  • 1St Edmund's College, Cambridge CB3 0BN, UK. smitton@cambridge.org

Lancet (London, England)
|May 23, 2006
PubMed
Resumen

La física de las astropartículas conecta la física cuántica de partículas con la cosmología. Comprender el universo es entender el universo.

Área de la Ciencia:

  • Física de las astropartículas Física de las astropartículas
  • Cosmología Cosmología.
  • La mecánica cuántica es la mecánica cuántica.
  • La teoría de cuerdas es la teoría de cuerdas.

Sus antecedentes:

  • El Modelo Estándar de la física de partículas describe la materia usando quarks, leptones y fuerzas fundamentales.
  • Los modelos cosmológicos revelan que la materia ordinaria constituye sólo el 4% del universo.
  • La composición del universo está dominada por la materia oscura (23%) y la energía oscura (73%).

Objetivo del estudio:

  • Explorar las conexiones interdisciplinarias entre la física de partículas y la cosmología.
  • Investigar los constituyentes fundamentales de la materia y las propiedades a gran escala del universo.
  • Examinar los posibles marcos para unificar la mecánica cuántica y la gravedad.

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Principales métodos:

  • Revisión del Modelo Estándar de la física de partículas.
  • Análisis de modelos cosmológicos y sus implicaciones para la composición universal.
  • Exploración de marcos teóricos como la teoría de cuerdas para la unificación.

Principales resultados:

  • El Modelo Estándar explica con éxito las propiedades de las partículas a través de quarks y leptones.
  • Las observaciones cosmológicas indican un universo dominado por materia oscura y energía oscura.
  • La energía oscura se identifica como el motor de la expansión acelerada del universo.

Conclusiones:

  • La física de las astropartículas une los reinos cuántico y cósmico.
  • La composición del universo es en gran parte desconocida, ya que comprende materia oscura y energía oscura.
  • La teoría de cuerdas ofrece una vía potencial para unificar la física cuántica con la gravedad.