Temperature of Black Holes and Minimum Wavelength of Radio Waves

Authors

  • C. Ganesa Moorthy  Department of Mathematics, Alagappa University, Karaikudi, India
  • G. Udhaya Sankar  Department of Physics, Alagappa University, Karaikudi, India
  • G. RajKumar  Department of Electrical and Electronics Engineering, Nehru College of Engineering and Research Centre, Pampady, India

Keywords:

Electromagnetic Waves, Cosmic Microwave Background, Black Holes.

Abstract

The temperature for a black hole is identified as the temperature of the cosmic microwave background. The exact separating value for wavelength is found to classify electromagnetic waves into electric field waves and magnetic field waves. The maximum possible diameter of molecules in our universe is found. A Chandrasekhar’s limit for black holes is used to guess somewhat reasonable values of radii for electrons, protons and neutrons.

References

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  4. Moorthy, C. Ganesa, G. Udhaya Sankar, and G. RajKumar. "A Design for Charging Section of Electrostatic Precipitators by Applying a Law for Electric Field Waves." Imperial Journal of Interdisciplinary Research 3.6 (2017). (http://imperialjournals.com/index.php/IJIR/article/view/5233/5036)
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    (http://www.imperialjournals.com/index.php/IJIR/article/view/5856/5625)
  6. Moorthy, C. Ganesa, G. Udhaya Sankar, and G. RajKumar. "LIGOs Detected Magnetic Field Waves; not Gravitational Waves." Imperial Journal of Interdisciplinary Research 3.8 (2017).
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    (http://ijsrset.com/paper/2061.pdf)

International Journal of Scientific Research in Science, Engineering and Technology

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Published

2018-04-30

Issue

Volume 4, Issue 4, March-April-2018

Section

Research Articles

License

Copyright (c) IJSRSET

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This work is licensed under a Creative Commons Attribution 4.0 International License.

How to Cite

[1]
C. Ganesa Moorthy, G. Udhaya Sankar, G. RajKumar, " Temperature of Black Holes and Minimum Wavelength of Radio Waves, International Journal of Scientific Research in Science, Engineering and Technology(IJSRSET), Print ISSN : 2395-1990, Online ISSN : 2394-4099, Volume 4, Issue 4, pp.1104-1107, March-April-2018.