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Momentum And Radiation Pressure01:20

Momentum And Radiation Pressure

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An object absorbing an electromagnetic wave would experience a force in the direction of propagation of the wave. This force occurs because electromagnetic waves contain and transport momentum. The force accounts for the wave's radiation pressure exerted on the object. Maxwell's prediction was confirmed in 1903 by Nichols and Hull by precisely measuring radiation pressures with a torsion balance. The measuring instrument had mirrors suspended from a fiber kept inside a glass container.
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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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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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Radiation Pressure: Problem Solving01:09

Radiation Pressure: Problem Solving

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The radiation pressure applied by an electromagnetic wave on a perfectly absorbing surface equals the energy density of the wave. The wave's momentum also gets transferred to the surface when an electromagnetic wave is entirely absorbed by it. The rate at which momentum is transmitted to an absorbing surface perpendicular to the propagation direction equals the force on the surface.
The average value of the rate of momentum transfer divided by the absorbing area represents the average force...
771
Emission Spectra02:39

Emission Spectra

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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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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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Updated: Jan 9, 2026

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
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A cosmic-ray loaded nascent outflow driven by a massive star cluster.

Marianne Lemoine-Goumard1,1, Lucia Härer2, Lars Mohrmann3

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Massive star clusters may drive galactic outflows. This study reveals a cosmic-ray outflow from Westerlund 1, providing direct evidence for cosmic rays influencing galaxy evolution and potentially transporting them into galactic halos.

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Area of Science:

  • Astrophysics
  • Galaxy Evolution
  • High-Energy Astrophysics

Background:

  • Cosmic rays are theorized to drive galactic outflows, crucial for galaxy evolution.
  • Massive star clusters are increasingly recognized for their role in cosmic-ray acceleration.
  • Direct observational evidence linking cosmic rays to galactic outflows has been scarce.

Purpose of the Study:

  • To provide direct evidence of cosmic-ray driven outflows from a massive star cluster.
  • To investigate the role of massive star clusters in cosmic-ray transport and galaxy evolution.

Main Methods:

  • Observation of gigaelectronvolt (GeV) gamma-ray emission.
  • Mapping atomic hydrogen distribution to identify galactic cavities.
  • Spectral and spatial analysis of gamma-ray emission in relation to the star cluster Westerlund 1.

Main Results:

  • Discovery of a nascent outflow driven by the massive star cluster Westerlund 1.
  • Detection of GeV gamma-ray emission tracing relativistic electrons emerging from the Galactic Disc.
  • Identification of an energy density of cosmic rays significantly higher than the interstellar medium.

Conclusions:

  • The observed outflow provides direct evidence for cosmic-ray carrying outflows.
  • Massive star clusters likely generate cosmic-ray loaded outflows, influencing galaxy evolution.
  • These outflows may be a significant mechanism for cosmic-ray transport into galactic halos.