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Related Concept Videos

Radiation: Applications01:17

Radiation: Applications

The average temperature of Earth is the subject of much current discussion. Earth is in radiative contact with both the Sun and dark space; it receives almost all its energy from the radiation of the Sun and reflects some of it into outer space. Dark space is very cold, about 3 K, so Earth radiates energy into it. For instance, heat transfer occurs from soil and grasses, the rate of which can be so rapid that frost can occur on clear summer evenings, even in warm latitudes.
The average...
Momentum And Radiation Pressure01:20

Momentum And Radiation Pressure

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. Nichols...
Absorption of Radiation01:05

Absorption of Radiation

The rate of heat transfer by emitted radiation is described by the Stefan-Boltzmann law of radiation:
Interaction of EM Radiation with Matter: Spectroscopy01:12

Interaction of EM Radiation with Matter: Spectroscopy

Electromagnetic (EM) radiation can be considered an oscillating electric and magnetic field propagating through a medium that can interact with matter in its path. The electric field in the radiation can interact with electrical charges in the atoms or molecules in the matter. On the other hand, the magnetic field can interact with the magnetic field in the atomic nucleus. The study of the interaction between electromagnetic radiation and matter is termed spectroscopy. Spectroscopy is the study...
Radiation Pressure: Problem Solving01:09

Radiation Pressure: Problem Solving

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 per...
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...

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Related Experiment Video

Updated: May 9, 2026

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry
12:14

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry

Published on: August 12, 2013

Attractive optical forces from blackbody radiation.

M Sonnleitner1, M Ritsch-Marte, H Ritsch

  • 1Institute for Theoretical Physics, University of Innsbruck, Technikerstraße 25, A-6020 Innsbruck, Austria.

Physical Review Letters
|July 30, 2013
PubMed
Summary

Hot objects generate a "blackbody force" from radiation that can pull atoms, like hydrogen, towards surfaces, even overcoming gravity. This overlooked force is significant in astrophysical environments.

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Determination of the Excitation and Coupling Rates Between Light Emitters and Surface Plasmon Polaritons
07:39

Determination of the Excitation and Coupling Rates Between Light Emitters and Surface Plasmon Polaritons

Published on: July 21, 2018

Related Experiment Videos

Last Updated: May 9, 2026

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry
12:14

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry

Published on: August 12, 2013

Determination of the Excitation and Coupling Rates Between Light Emitters and Surface Plasmon Polaritons
07:39

Determination of the Excitation and Coupling Rates Between Light Emitters and Surface Plasmon Polaritons

Published on: July 21, 2018

Area of Science:

  • Atomic and Molecular Physics
  • Astrophysics
  • Quantum Optics

Background:

  • Blackbody radiation from hot objects causes AC Stark shifts in atomic and molecular energy levels.
  • These shifts are temperature-dependent and create forces that decay with distance.

Purpose of the Study:

  • To explicitly calculate the blackbody optical dipole force on ground state hydrogen atoms.
  • To investigate the conditions under which this force overcomes radiation pressure and gravity.

Main Methods:

  • Theoretical calculation of the blackbody optical dipole force.
  • Analysis of the force's dependence on temperature and distance.
  • Comparison with radiation pressure and gravitational forces.

Main Results:

  • The calculated attractive blackbody optical dipole force can exceed repulsive radiation pressure.
  • This force can pull hydrogen atoms towards a hot object, counteracting radiation flow.
  • The blackbody force is demonstrated to be stronger than gravity for hydrogen near hot dust particles.

Conclusions:

  • An overlooked attractive force, termed the "blackbody force," is significant in astrophysical scenarios.
  • This force has implications for the behavior of atoms and molecules near hot broadband radiation sources.
  • The findings are relevant for understanding atomic interactions in diverse cosmic environments.