Реферат Свадковского

Moderators: Konstantin Belotsky, Maxim Khlopov

Реферат Свадковского

New postby Igor Svadkovsky on Mon 18 May 2009 09:32

PBHs.pdf
(91.85 KiB) Downloaded 487 times
Igor Svadkovsky
 
Posts: 3
Joined: Thu 30 Apr 2009 17:03


Re: Реферат Свадковского

New postby Maxim Khlopov on Tue 19 May 2009 00:03

Dear Igor,
Please discuss:
- mechanisms of PBH formation
- what kind of constraints on super high energy physics can be obtained from upper limits on PBHs?
- primordial clouds of massive PBHs as seeds of active galactic nuclei (AGN) of galaxies
Please add Conclusion and List of references
Regards
M.Yu.Khlopov
[i]Хлопов Максим Юрьевич
Maxim Khlopov[/i]
User avatar
Maxim Khlopov
Administrateur du site
 
Posts: 1934
Joined: Sat 9 Aug 2008 19:42
Location: Paris


Re: Реферат Свадковского

New postby Igor Svadkovsky on Thu 21 May 2009 13:24

Михаил Юрьевич, я постарался учесть Ваши замечания. Вот новый вариант.
Attachments
PBHs.pdf
(117.15 KiB) Downloaded 457 times
Igor Svadkovsky
 
Posts: 3
Joined: Thu 30 Apr 2009 17:03


Re: Реферат Свадковского

New postby Maxim Khlopov on Thu 21 May 2009 20:37

Dear Igor,
It is close to finish. If you mention papers by Zeldovich and Novikov, or by Hawking these papers should be present in Bibliography (which should be more than 3 references).
There also should be a title list
Regards
M.Yu.Khlopov
[i]Хлопов Максим Юрьевич
Maxim Khlopov[/i]
User avatar
Maxim Khlopov
Administrateur du site
 
Posts: 1934
Joined: Sat 9 Aug 2008 19:42
Location: Paris


Re: Реферат Свадковского

New postby Igor Svadkovsky on Fri 22 May 2009 08:27

Михаил Юрьевич, спасибо за замечания. Я внес некоторые исправления. Прошу прощения за свой титульный лист - он неудачно получился (некоторые проблемы с латехом).
Attachments
PBHs.pdf
(120.29 KiB) Downloaded 500 times
Igor Svadkovsky
 
Posts: 3
Joined: Thu 30 Apr 2009 17:03


Re: Реферат Свадковского

New postby Maxim Khlopov on Sat 23 May 2009 09:51

Dear Igor,
To complete your work on referat please add answer on the following question:
1. In bubble collisions at 1 order phase transition after inflation PBHs have typical mass of 1g, so they seem to evaporate very early. What additional condition is necessary to put stringent limits on such PBHs and corrrespondingly on 1 order phase transitions in early Unvierse?
Regards
M.Yu.Khlopov
[i]Хлопов Максим Юрьевич
Maxim Khlopov[/i]
User avatar
Maxim Khlopov
Administrateur du site
 
Posts: 1934
Joined: Sat 9 Aug 2008 19:42
Location: Paris



Return to КУРС ПО КОСМОМИКРОФИЗИКЕ 2008/2009

Who is online

Users browsing this forum: No registered users and 45 guests

cron