tag:blogger.com,1999:blog-124350264510724511.post5118632513387045950..comments2024-01-15T16:21:42.238+02:00Comments on Unitary Flow: Black Hole Information Paradox 3. Look for the information where you lost itCristi Stoicahttp://www.blogger.com/profile/00577217435388643300noreply@blogger.comBlogger6125tag:blogger.com,1999:blog-124350264510724511.post-35073122586159991862014-01-28T17:24:17.006+02:002014-01-28T17:24:17.006+02:00Dear Rafael,
> Do the g_mu_nu = 0 "soluti...Dear Rafael,<br /><br />> Do the g_mu_nu = 0 "solutions" also play an important role in your densitized approach to GR ? Is your approach also able to incorporate that ( g_mu_nu = 0 ) solution and so explain dark matter as a topological effect?<br /><br />Yes, it works for g_mu_nu=0 solutions. I don't know yet if my approach explains dark matter. <br /><br />I read the paper you referenced (thank you), and I think it is very interesting, showing that the ground degenerate metric is a good candidate to explain dark matter. I plan to reread it more carefully. I found another paper which discusses dark matter as a 2+1 dimensional effect http://arxiv.org/abs/astro-ph/0008268. Maybe both can be connected with my paper http://arxiv.org/abs/1205.2586, in which I discuss the dimensional reduction effects of degenerate metric (needed for QG). Normally in QG one takes as ground metric a Minkowski one, but I think one should take g_mu_nu=0 indeed.<br /><br />I would like to discuss more about the relation between my approach and dark matter, but at this point I would only be able to speculate too much even for a blog :)<br /><br />Best regards,<br />CristiCristi Stoicahttps://www.blogger.com/profile/00577217435388643300noreply@blogger.comtag:blogger.com,1999:blog-124350264510724511.post-7643749116273169482014-01-28T15:32:21.004+02:002014-01-28T15:32:21.004+02:00Dear Cristi,
are you aware of this paper http://a...Dear Cristi,<br /><br />are you aware of this paper http://arxiv.org/abs/hep-th/0701169 ?<br /><br />Do the g_mu_nu = 0 "solutions" also play an important role in your densitized approach to GR ? Is your approach also able to incorporate that ( g_mu_nu = 0 ) solution and so explain dark matter as a topological effect?<br />If you could elaborate more on this theme, maybe as a blog entry it would be really great!<br /><br />Thanks beforehand by your answer.<br />Best<br /><br />RafaelAnonymoushttps://www.blogger.com/profile/16589243519941443450noreply@blogger.comtag:blogger.com,1999:blog-124350264510724511.post-36651547864446050732014-01-13T19:49:24.381+02:002014-01-13T19:49:24.381+02:00Thank you Robert!
Also thank you for writing a gr...Thank you Robert!<br /><br />Also thank you for writing a great book about the Standard Model (http://www.amazon.com/dp/0452287863), which I liked very much.Cristi Stoicahttps://www.blogger.com/profile/00577217435388643300noreply@blogger.comtag:blogger.com,1999:blog-124350264510724511.post-17886533356445930772014-01-13T18:48:09.679+02:002014-01-13T18:48:09.679+02:00Thanks for this series, Cristi! Beautifully explai...Thanks for this series, Cristi! Beautifully explained. Locating the missing information at the singularity makes so much more sense than locating it at the horizon.<br /><br />I wish you the best in continuing this research, and I hope that your graduation won't mean you stop blogging!Robert Oerterhttps://www.blogger.com/profile/09708981993708509662noreply@blogger.comtag:blogger.com,1999:blog-124350264510724511.post-36215631575651104452013-10-06T08:32:52.622+03:002013-10-06T08:32:52.622+03:00thanks, Ninithanks, NiniCristi Stoicahttps://www.blogger.com/profile/00577217435388643300noreply@blogger.comtag:blogger.com,1999:blog-124350264510724511.post-89291875197324757612013-10-05T21:10:28.602+03:002013-10-05T21:10:28.602+03:00omg, great finding... and now you finally get some...omg, great finding... and now you finally get some recognitionNinihttps://www.blogger.com/profile/03485172850076925319noreply@blogger.com