... 13) Clearly, the parameter p # does enter T B A when m = 1. ... we can calculate the generalized Einstein equations by introducing some coupling constant # (m,n) and taking (13) as the source ...
... Here we will focus on so called skyrmion stars (SkyS) as they are ex 1 This range is based on the two estimates given in (Quaintrell et al. 2003): 1.88 ± 0.13 and 2.27 ± 0.17 M # . ...
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Ссылки http://xray.sai.msu.ru/~polar/html/publications/ouyed/skyrm_aa6.ps -- 1034.9 Кб -- 14.12.2004 Похожие документы
... More precisely, we admit m to fall with the growth of r. Let, for small r, m be approximately described as follows m = 1 - #r + #r 2 (12) where 0 < # # - dm dr # # # # # r=0 # 1, # # 1 2 d 2 m dr 2 # # # # # r=0 , (13) and |#| is of the order of # 2 . ...
... Rapidly rotating SkyS were discussed by Ouyed (2002, 2004), and for this case Mmax=3.45 M # and R = 1 This range is based on the two estimates given in Quaintrell et al. (2003): 1.88 ± 0.13 and 2.27 ± 0.17 M # . ...
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Ссылки http://xray.sai.msu.ru/~polar/html/publications/ouyed/skyrm_aa5.ps -- 1052.9 Кб -- 11.12.2004 Похожие документы