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Radio Astronomy and Cosmology

Radio Astronomy and Cosmology

J. E. Baldwin (auth.), David L. Jauncey (eds.)
এই বইটি আপনার কতটা পছন্দ?
ফাইলের মান কিরকম?
মান নির্ণয়ের জন্য বইটি ডাউনলোড করুন
ডাউনলোড করা ফাইলগুলির মান কিরকম?

337 F(e) = (z) where the angle between the directions III and 112 is equal to 8. r is the angular diameter effective distance of the epoch for recombination. F (8) ~ve have F(e) : f (e) ~ (S" ) e. . ~ is a Bessel function. It is assumed here that the spectrum of gravitational waves takes the form 1\ hI'::: hoK for all relevant wavelengths, a is beam width of the radio antenna, d\= d~, and ~ is the duration of the process of recombinations in \-time. The results for different beam widths are shown in Fig. 1. 338 I. D. NOVIKOV 1-. . . -__ 0. 5 1 1. 5 2 e' 0. 5 o and for a l' (solid line) and Fig. 1. The function f(8) for n for a = 2' (dotted line). These formula should be used in analysing the implications of future observations. Comparison with the observational data now available enables us to establish an upper limit for the energy density of long gravitational waves. This method is most sensitive for gravitational waves with A ~ ct The fluctuations ~; due to these waves have scale ~ 0. 03 GW rec 4 radian. If, according to modern observations, we take ~; < 10- , then 8 26 ~GW/Ey < 10- for those gravitational waves which have A = 5. 10 cm GW today where Ey is the energy density of relict radiation. The fluctuations ~TT due to long gravitational waves with A = ct .

ক্যাটাগোরিগুলো:
সাল:
1977
সংস্করণ:
1
প্রকাশক:
Springer Netherlands
ভাষা:
english
পৃষ্ঠা:
416
ISBN 10:
9401012601
ISBN 13:
9789401012607
বইয়ের সিরিজ:
International Astronomical Union / Union Astronomique Internationale 74
ফাইল:
PDF, 15.41 MB
IPFS:
CID , CID Blake2b
english, 1977
কপিরাইট ধারকের অভিযোগের কারণে এই বইটির ডাউনলোড অনুপলব্ধ

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Pravin Lal

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