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Potential Due to a Polarized Object01:29

Potential Due to a Polarized Object

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A neutral atom consists of a positively charged nucleus surrounded by a negatively charged electron cloud. When placed in an external electric field, the external electric force pulls the electrons and nucleus apart, opposite to the intrinsic attraction between the nucleus and the electrons. The opposing forces balance each other with a slight shift between the center of masses of the nucleus and the electron cloud, resulting in a polarized atom. On the other hand, a few molecules, like water,...
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Momentum And Radiation Pressure01:20

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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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Shock Waves01:16

Shock Waves

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While deriving the Doppler formula for the observed frequency of a sound wave, it is assumed that the speed of sound in the medium is greater than the source's speed through it. When this condition is breached, a shock wave occurs.
When the source's speed approaches the speed of sound, constructive interference between successive wavefronts emitted by the source occurs immediately behind it. Initially, scientists believed that this constructive interference would result in such high...
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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...
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Group Polarization01:01

Group Polarization

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Group polarization is the strengthening of an original group attitude following the discussion of views within a group (Teger & Pruitt, 1967). That is, if a group initially favors a viewpoint, after discussion the group consensus is likely a stronger endorsement of the viewpoint. Conversely, if the group was initially opposed to a viewpoint, group discussion would likely lead to stronger opposition.
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Schwarzschild Radius and Event Horizon01:21

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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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Related Experiment Video

Updated: Aug 9, 2025

Scattering And Absorption of Light in Planetary Regoliths
11:34

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Polarized accretion shocks from the cosmic web.

Tessa Vernstrom1,2, Jennifer West3, Franco Vazza4,5,6

  • 1ICRAR, The University of Western Australia, 35 Stirling Hw, 6009 Crawley, Australia.

Science Advances
|February 15, 2023
PubMed
Summary
This summary is machine-generated.

Astronomers found evidence of particle acceleration in the cosmic web

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Area of Science:

  • Cosmic Microwave Background
  • Astrophysics
  • Cosmology

Background:

  • Galaxies form clusters connected by filaments, creating a cosmic web structure.
  • Radio emission is theoretically predicted from accretion shocks within this cosmic web.

Purpose of the Study:

  • To present the first observational evidence of Fermi-type acceleration in the cosmic web.
  • To investigate radio emission originating from shocks in cosmic web filaments and low-mass clusters.

Main Methods:

  • Utilized all-sky radio maps for analysis.
  • Employed stacking techniques on galaxy clusters and filaments.
  • Analyzed the polarization signature of synchrotron emission.

Main Results:

  • Detected synchrotron emission with polarization fractions of at least 20%.
  • Evidence suggests Fermi-type acceleration is active in cosmic web filaments and cluster peripheries.
  • Observed organization of magnetic fields by shock waves.

Conclusions:

  • The findings provide the first observational support for particle acceleration at shocks in the cosmic web.
  • The results align with theoretical predictions and cosmological simulations.
  • This study enhances our understanding of the energetic processes shaping the large-scale structure of the Universe.