KOINOTNING KENGAYMASLIK NAZARIYASI VA UNING ILMIY IZLANISHLARDAGI O‘RNI

Authors

  • Jumaeva Ra’no To‘ychi qizi Termiz davlat pedagogika instituti Fizika kafedrasi o‘qituvchisi Author

Keywords:

Koinotning kengaymaslik nazariyasi, Katta portlash nazariyasi, kosmik mikroto‘lqin fon nurlanishi, koinotning tuzilishi, kosmologiya, koinotning evolyutsiyasi.

Abstract

Mazkur maqola koinotning kengaymaslik nazariyasiga (Steady State Theory) bag‘ishlangan bo‘lib, bu nazariyaning asosiy g‘oyalarini va uning tarixiy ahamiyatini o‘rganadi. Koinotning kengaymaslik nazariyasi 1940-yillarda Fred Hoyle, Hermann Bondi va Thomas Gold tomonidan ishlab chiqilgan va koinotning doimiy ravishda kengaymasligi, yangi materiya doimiy ravishda paydo bo‘lishi va koinotning umumiy tuzilishi o‘zgarmasligini ta’kidlaydi. Ushbu nazariya Katta portlash nazariyasiga qarshi ishlab chiqilgan bo‘lib, koinotning kengayishini va evolyutsiyasini boshqacha tushuntirishga harakat qiladi.

Maqolada stasionar holat nazariyasining asosiy tushunchalari, tarixiy konteksti, tanqidlar va zamonaviy ilmiy qarashlar batafsil keltirilgan. Shuningdek, Katta portlash nazariyasining stasionar holat nazariyasiga qarshi bo‘lgan dalillari, jumladan kosmik mikroto‘lqin fon nurlanishi va galaktikalar orasidagi masofalardagi o‘zgarishlar muhokama qilingan. Nazariya va uning rivojlanishi, ilmiy jamoa tomonidan qanday qabul qilinishi va uning bugungi ilmiy izlanishlarga ta’siri tahlil qilinadi.

References

1.Hoyle, F., Bondi, H., & Gold, T. (1948). The Steady State Theory of the Universe. Monthly Notices of the Royal Astronomical Society, 108(5), 372-382.

2.Penzias, A. A., & Wilson, R. W. (1965). A Measurement of Excess Antenna Temperature at 4080 Mc/s. The Astrophysical Journal, 142(3), 419-421.

3.Peebles, P. J. E. (1993). Principles of Physical Cosmology. Princeton University Press.

4.Weinberg, S. (1972). Gravitation and Cosmology: Principles and Applications of the General Theory of Relativity. Wiley.

5.Liddle, A. R., & Lyth, D. H. (2000). Cosmological Inflation and Large-Scale Structure. Cambridge University Press.

6.Guth, A. H. (1981). The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems. Physical Review D, 23(2), 347-356.

7.Hawking, S. W., & Ellis, G. F. R. (1973). The Large-Scale Structure of Space-Time. Cambridge University Press.

8.Bondi, H., & Gold, T. (1952). The Steady-State Theory of the Expanding Universe. Nature, 169(4296), 539-541.

9.Turner, M. S., & Riess, A. G. (2003). The Dark Energy Equation of State: Current Measurements and Constraints. The Astrophysical Journal, 576(2), 623-630.

Published

2024-11-19

How to Cite

Jumaeva Ra’no To‘ychi qizi. (2024). KOINOTNING KENGAYMASLIK NAZARIYASI VA UNING ILMIY IZLANISHLARDAGI O‘RNI. IQRO INDEXING, 12(02), 233-235. http://worldlyjournals.com/index.php/IFX/article/view/6993