13-Modul. Magnit maydoni va uning xarakteristikalari




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Moddaning paydo bo‘lishi.
Koinot rivojlanishining radiatsion erasi juda muxim xioblanadi. Aynan shu davrda D. Mendeleev davriy sistemasini tashkil qiluvchi elementlarning asosi – og‘ir yadrolar paydo bo‘la boshlangan. Ushbu jarayon nukleosintez deb nomlanadi. Eng engil yadro – proton Koinot paydo boshlgandan 10 sekund o‘tib paydo bo‘lgan. Ushbu davrda Koinotning temperaturasi va zichligi deyteriy – ikkita nuklondan tashkil topgan yadroni sintezi uchun etarli katta bo‘lib, proton va neytronning to‘qnashishi natijasida paydo bo‘lgan.
p + n 2H + + Q.
Bu erda Q = 2.2 MeV – ushbu sintez reaksiyasida ajralib chiqadigan energiya. Keyin 10-15 minut vaqt ichida 2H deyteriyni 3H tritiyga aylanishi, so‘ngra deyteriy va tritiydan 3He geliy yadrosining paydo bo‘lish reaksiyalari sodir bo‘lgan13. Hisob natijalariga ko‘ra geliy barcha nuklonlar ichida 24 foizni tashkil qilgan. Xozirgi paytdagi kuzatuv natijalari ham shuni ta’kidlamoqda.





4-rasm. Yulduzlardagi nukleosintezning sxematik ko‘rinishi.




1 Arnab Rai Choudhuri, Astrophysics for Physics, Cambridge University Press, 2010, 471 p.

2 James B. Hartle, Gravity: An Introduction to Einstein’s General Relativity, Pearson Education Ltd., 2013, 554 p.

3 Бочкарев Н.Г.б Магнитные поля в космосе, М.: Книжный дом «ЛИБРОКОМ», 2011. – 216 с.

4 Arnab Rai Choudhuri, Astrophysics for Physics, Cambridge University Press, 2010, 471 p.

5 Arnab Rai Choudhuri, Astrophysics for Physics, Cambridge University Press, 2010, 471 p.

6 Max Camenzind, Compact Objects in Astrophysics, Springer, 2007, 682 p.

7 L. Rezzolla, O. Zanotti, Relativistic Hydrodynamics, Oxford University Press, 2013, 752 p.

8 T. Padmanabhan, Theoretical Astrophysics, Volume I-III, Cambridge University Press, 2010.

9 T. Padmanabhan, Theoretical Astrophysics, Volume I-III, Cambridge University Press, 2010.

10 James B. Hartle, Gravity: An Introduction to Einstein’s General Relativity, Pearson Education Ltd., 2013, 554 p.

11 James B. Hartle, Gravity: An Introduction to Einstein’s General Relativity, Pearson Education Ltd., 2013, 554 p.

12 T. Padmanabhan, Theoretical Astrophysics, Volume I, Cambridge University Press, 2010

13 Фильченков М.Л., Гравитация, астрофизика, космология: дополнительные главы, «ЛИБРОКОМ», 2010.


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13-Modul. Magnit maydoni va uning xarakteristikalari

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