Frequency of Hawking Radiation of Black Holes

Frequency of Hawking Radiation of Black Holes

International Journal of Astrophysics and Space Science 2013; 1(4): 45-51 Published online October 30, 2013 (http://www.sciencepublishinggroup.com/j/ijass) doi: 10.11648/j.ijass.20130104.15 Frequency of Hawking radiation of black holes Dipo Mahto 1, Brajesh Kumar Jha 2, Krishna Murari Singh 1, Kamala Parhi 3 1Dept. of Physics, Marwari College, T.M.B.U. Bhagalpur-812007, India 2Deptartment of Physics, L.N.M.U. Darbhanga, India 3Dept. of Mathematics, Marwari College, T.M.B.U. Bhagalpur-812007, India Email address: [email protected](D. Mahto), [email protected](B. K. Jha), [email protected](K. M. Singh), [email protected] (K . Parhi) To cite this article: Dipo Mahto, Brajesh Kumar Jha, Krishna Murari Singh, Kamala Parhi. Frequency of Hawking Radiation of Black Holes. International Journal of Astrophysics and Space Science. Vol. 1, No. 4, 2013, pp. 45-51. doi: 10.11648/j.ijass.20130104.15 Abstract: In the present research work, we calculate the frequencies of Hawking radiations emitted from different test black holes existing in X-ray binaries (XRBs) and active galactic nuclei (AGN) by utilizing the proposed formula for the 8.037× 10 33 kg frequency of Hawking radiation f= Hz and show that these frequencies of Hawking radiations may be the M components of electromagnetic spectrum and gravitational waves. We also extend this work to convert the frequency of Hawking radiation in terms of the mass of the sun ( M ⊙ ) and then of Chandrasekhar limit ( M ch ), which is the largest unit of mass. Keywords: Electromagnetic Spectrum, Hawking Radiation, XRBs and AGN Starobinsky showed him that according to the quantum 1. Introduction mechanical uncertainty principle, rotating black holes A black hole is a solution of Einstein’s gravitational field should create and emit particles (Hawking, 1988). Before Hawking, in 1969, Leonard Parker obtained an equations in the absence of matter that describes the space expression for the average particle density as a function of time around a gravitationally collapsed star. Its gravitational time, and showed that particles creation is in pairs. The pull is so strong that even light cannot escape from it canonical creation and annihilation operators corresponding (Dabholkar 2005, Mahto et al. 2012&2013). The space-time having a black hole in it, first, has a singularity, and second, to physical particles during the expansion of the universe are has a horizon preventing an external observer from seeing it. specified and argued that in the present predominantly dust-filled universe, only massless particles of zero spin The singularity in GR is radically different from field theory might possibly be produced in significant amounts by the singularities because it is a property not of some field but of present expansion and also showed that massless particles of the space-time itself. The topology of space-time is changed when it acquires a black hole (Soloviev, 2005). arbitrary non-zero spin, such as photons or gravitons, are not In classical theory black holes can only absorb and not created by the expansion regardless of its form (Parker, 1969). emit particles. However, it is shown that quantum Hawking radiation arises for any test field on any mechanical effects cause black holes to create and emit Lorentzian geometry containing an event horizon regardless particles as if they were hot bodies with temperature of whether or not the Lorentzian geometry satisfies the κ h −6 M ⊙ dynamical Einstein equations of general relativity (Matt., ≈ 10 κ , where κ is surface gravity of 2π k M 1997). The outgoing wave packet is composed of wave vectors black holes and k is the Boltzmann constant. This thermal around K+s (and has positive Killing frequency) and arises emission leads to show a decrease in the mass of the black from a pair of packets composed of wave vectors around K+ hole and to its eventual disappearance: any primordial black and K– respectively which have positive and negative hole of mass less than about 10 15 gram would have free-fall frequency respectively (Corely and Jacobson 1998). evaporated by now (Hawking, 1975). Steven Corely and Ted Jacobson found that there are two Hawking’s work followed his visit to Moscow, where qualitatively different types of particle production in this Soviet scientists Yakov Zeldovich and Alexander 46 Dipo Mahto et al. : Frequency of Hawking radiation of black holes model: a thermal Hawking flux generated by “mode emit. The only length-scale in the problem is the size of the conversion” at the black hole horizon, and a non-thermal horizon. A photon with a wavelength ( λ ) equal to the radius spectrum generated via scattering off the background into of the black hole has energy equal to negative free-fall frequency modes. This second process has nothing to do with black holes and does not occur for the E= h ν (2) ordinary wave equation because such modes do not propagate outside the horizon with positive Killing The energy of a pair of virtual photons will be given by frequency (Corely and Jacobson 1996). the following equation Compact binaries (two neutron stars, two black holes, one BH and one NS, binary stars, rotating neutron stars, neutron E= 2 h ν (3) star instabilities, super nova, super massive black holes and stochastic background) are the sources emitting The energy of a photon of Hawking radiation is given by gravitational waves (Daniel Sigg, 1998). Gravitational wave the following equation (Hawking radiation, detection effects focus on four frequency bands (Curt and htt://library.thinkquest.org/c007571/English/printcore.htm, Thorne, 2002) (i) The extremely low frequency band (10 -15 2011) -18 to 10 Hz). 3 -7 -9 hc (ii) The very low frequency band (10 to 10 Hz). E = (4) (iii) The low frequency band (10 -4 to 1Hz). 16 πGM (iv) The high frequency band (1 to 10 4 Hz). In the present research paper, we have calculated the From equation (2) and (4), we have frequency of Hawking radiation of different types of the test 3 black holes existing in X-ray binaries (XRBs) and active c ν = (5) galactic nuclei (AGN) emitted by black holes and we have 16 πGM also tried to show that frequencies of Hawking radiations emitted by black holes may be the components of All the terms like gravitational constant (G), Planck electromagnetic spectrum. This work is further extended to constant (h) and velocity of light(c) on the right hand side of convert the frequency of Hawking radiation in terms of mass the equation (5) are constant except mass (M) of the black hole. These constants have vital role discussed as: of the sun and then in Chandrasekhar limit ( M ch ). The three fundamental constants of nature – the speed of light (c), Planck’s constant (h) and Newton’s gravitational 2. Theoretical Discussion constant (G) are present in the eq n (5). Planck’s constant (h) governs the law of quantum world. The speed of light (c) is Classically, the black holes are perfect absorbers and do the cornerstone of the special theory of relativity. The fact not emit anything; their temperature is absolute zero. that light is an electromagnetic wave travelling at the speed However, in quantum theory black holes emit Hawking of light (c) is very important consequences of Maxwell’s radiation with a perfect thermal spectrum. This allows a equations for electromagnetic field. In general relativity, consistent interpretation of the laws of black hole mechanics Newton’s gravitational constant G has an entirely new as physically corresponding to the ordinary laws of meaning. For Newton, G is the constant of proportionality thermodynamics (Wald 2001). that appears in inverse square law of gravitation, while for In quantum physics, the empty space is not empty at all. In Einstein; G is a constant that determines the degree to which it there are always particles flashing into existence and a given distribution of matter warps space and time disappear again. They always come in pairs; one particle and (Dabholkar, 2005). one anti-particle, like an electron and a positron, or a photon The equation (5) can be written as and another photon with opposite spin and impulse. These particles are called virtual particles. They only exist for a 1 very short time given by (Hawking radiation, ν ∝ (6) htt://library.thinkquest.org/c007571/English/printcore.htm, M 2011) If λ be the wavelength of Hawking radiation emitted 1 from the black hole, then we have ∆t = (1) 8π f λ ∝ M (7) where f is the frequency of radiation. If one virtual particle The relation (6) shows that the frequency of Hawking falls into the black hole and the other escapes, it escapes as radiation emitted by the black holes is inversely proportional Hawking radiation from black hole. This radiation shows the to the mass of the black hole, whereas from relation (7) it is same allocation as black body radiation. This assumes that clear that the wavelength of Hawking radiation emitted by black holes do have a temperature too. the black hole is directly proportional to the mass of the Once, we accept that black holes can radiate, then it is not black holes. This means that the heavier black hole will emit hard to estimate the wavelength of the radiation that they the Hawking radiation of lower frequency or longer International Journal of Astrophysics and Space Science 2013; 1(4): 45-51 47 wavelength and vice-versa. The most viable scenario for modeling of active galactic Putting the values of h, c, G and π in equation (5), we nuclei includes a super massive black hole with the mass have 6− 9 10 10 M ⊙ accreting the galaxian matter from its 8.037× 10 33 kg vicinity (Madejski, 2003).

View Full Text

Details

  • File Type
    pdf
  • Upload Time
    -
  • Content Languages
    English
  • Upload User
    Anonymous/Not logged-in
  • File Pages
    7 Page
  • File Size
    -

Download

Channel Download Status
Express Download Enable

Copyright

We respect the copyrights and intellectual property rights of all users. All uploaded documents are either original works of the uploader or authorized works of the rightful owners.

  • Not to be reproduced or distributed without explicit permission.
  • Not used for commercial purposes outside of approved use cases.
  • Not used to infringe on the rights of the original creators.
  • If you believe any content infringes your copyright, please contact us immediately.

Support

For help with questions, suggestions, or problems, please contact us