New Insights into Physical Science Vol. 12

  • Home
  • About
  • Books
  • Testimonials
  • Editors
  • Charges
  • Submission
  • Contact
Advanced Search
  1. Home
  2. Books
  3. New Insights into Physical Science Vol. 12
  4. Chapters


Frequency/Wavelength as the Characteristics of Black Holes

  • Dipo Mahto
  • Rakesh Paswan
  • Santosh Kumar

New Insights into Physical Science Vol. 12, 19 February 2021 , Page 155-165
https://doi.org/10.9734/bpi/nips/v12/5939D Published: 2021-02-19

  • View Article
  • Cite
  • Share

Abstract

A model for the wavelength/frequency of Hawking radiation emitted by non-spinning black holes in terms of the radius of event horizon \((\lambda=8\pi R_{s} \;\&\;  v=c/8\pi R_{s}\))  is proposed using quantum theory of radiation ( \(E=h\nu)\), energy of Hawking radiation and the radius of event horizon of non-spinning black holes ( \(R_{s}=2GM/c^{2})\). This can be used as the characteristics of non-spinning black holes. Data for the frequencies and wavelengths of Hawking radiation emitted from black holes have been calculated with the help of rest masses for stellar-mass black holes (M~5-20 MO)  in X-ray binaries and for the super massive black holes (M~ 106 – 109.5 MO) in active galactic nuclei using the model given by \(\lambda=8\pi R_{s} \;\&\;  v=c/8\pi R_{s}\) of the research work entitled: Frequency of Hawking radiation from black holes by Mahto et al.(Dec.2013). The astrophysical objects emitting the radiations of frequencies (8.092x102Hz to 2.023x102Hz) or wavelengths (3.707x105 m to 14.828x105m) in X-ray binaries and frequencies ( 4.046X10-3Hz to 0.809X10-6Hz) or wavelengths (7.414X1010m to 37.070X1013m) in active galactic nuclei may be classified as non-spinning black holes. These frequencies or wavelengths may be regarded as the characteristics of black holes in addition to the mass, spin and charge.

Keywords:
  • Frequency
  • wavelength
  • spin and angular momentum

How to Cite

Mahto, D. ., Paswan, R. ., & Kumar, S. . (2021). Frequency/Wavelength as the Characteristics of Black Holes. New Insights into Physical Science Vol. 12, 155–165. https://doi.org/10.9734/bpi/nips/v12/5939D
  • ACM
  • ACS
  • APA
  • ABNT
  • Chicago
  • Harvard
  • IEEE
  • MLA
  • Turabian
  • Vancouver
  • Endnote/Zotero/Mendeley (RIS)
  • BibTeX
  • Linkedin
  • Twitter
  • Facebook
  • WhatsApp
  • Telegram

© B P International