Temperature of Black Holes and Minimum Wavelength of Radio Waves

Authors(3) :-C. Ganesa Moorthy, G. Udhaya Sankar, G. RajKumar

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.

Authors and Affiliations

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

Electromagnetic Waves, Cosmic Microwave Background, Black Holes.

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Publication Details

Published in : Volume 4 | Issue 4 | March-April 2018
Date of Publication : 2018-04-30
License:  This work is licensed under a Creative Commons Attribution 4.0 International License.
Page(s) : 1104-1107
Manuscript Number : IJSRSET11844387
Publisher : Technoscience Academy

Print ISSN : 2395-1990, Online ISSN : 2394-4099

Cite This Article :

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. Citation Detection and Elimination     |     
Journal URL : https://ijsrset.com/IJSRSET11844387

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