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Source: The Open Library

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1Atomic collisions in crystals

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“Atomic collisions in crystals” Metadata:

  • Title: Atomic collisions in crystals
  • Author:
  • Language: English
  • Number of Pages: Median: 260
  • Publisher: ➤  Gordon and Breach Science Publishers
  • Publish Date:
  • Publish Location: New York

“Atomic collisions in crystals” Subjects and Themes:

Edition Identifiers:

Access and General Info:

  • First Year Published: 1989
  • Is Full Text Available: No
  • Is The Book Public: No
  • Access Status: No_ebook

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Cherenkov radiation

anisotropy of the radiation and came to the conclusion that the bluish glow was not a fluorescent phenomenon. A theory of this effect was later developed

Greenhouse effect

aerosols absorb terrestrial radiation emitted by the Earth's surface and elsewhere in the atmosphere." The enhanced greenhouse effect describes the fact that

Hawking radiation

paired with one on the inside. The horizon allows one to escape in each direction. Hawking radiation is dependent on the Unruh effect and the equivalence

Yarkovsky effect

the effect: Diurnal effect: On a rotating body illuminated by the Sun (e.g. an asteroid or the Earth), the surface is warmed by solar radiation during

Unruh effect

obtain the Rindler metric. The Unruh effect would then be the near-horizon form of Hawking radiation. The Unruh effect is also expected to be present in

Poynting–Robertson effect

Poynting–Robertson effect, also known as Poynting–Robertson drag, named after John Henry Poynting and Howard P. Robertson, is a process by which solar radiation causes

Radiation therapy

Radiation therapy or radiotherapy (RT, RTx, or XRT) is a treatment using ionizing radiation, generally provided as part of cancer therapy to either kill

Radiation pressure

electromagnetic radiation of any wavelength that is absorbed, reflected, or otherwise emitted (e.g. black-body radiation) by matter on any scale (from

Ionizing radiation

Ionizing radiation, also spelled ionising radiation, consists of subatomic particles or electromagnetic waves that have enough energy per individual photon

YORP effect

due to the scattering of solar radiation off its surface and the emission of its own thermal radiation. The YORP effect is typically considered for asteroids