REGULAR R–R AND NS–NS BPS BLACK HOLES

نویسندگان
چکیده

برای دانلود باید عضویت طلایی داشته باشید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Nonextremal black holes are BPS

Extremal charged black holes are BPS solutions. It is commonly thought that their nonextremal counterparts are not. Further, experience with BPS solutions in flat spacetime suggests that all BPS solutions are supersymmetric; i.e. that they are invariant under some supersymmetry charges of either the original field theory or an appropriately extended version thereof. Using nonextremal Reissner-N...

متن کامل

BPS Black Holes 3 M -

Classical black holes are solutions of Einstein’s equations of general relativity that exhibit an event horizon. From inside this horizon, nothing (and in particular, no light) can escape. The region inside the horizon is therefore not in the backward lightcone of future timelike infinity. However, since the discovery of Hawking radiation [1], it has become clear that many of the classical feat...

متن کامل

From BPS to Non-BPS Black Holes Canonically

We describe the “action-angle” integrable system underlying the structure of double-extremal black holes. This implies the existence of a canonical transformation from BPS to non-BPS black holes. We give examples of such canonical transformation for STU and for E7(7)-invariant black holes. ∗ Email: [email protected]

متن کامل

Regular Black Holes and Black Universes

We give a comparative description of different types of regular static, spherically symmetric black holes (BHs) and discuss in more detail their particular type, which we suggest to call black universes. The latter have a Schwarzschild-like causal structure, but inside the horizon there is an expanding Kantowski-Sachs universe and a de Sitter infinity instead of a singularity. Thus a hypothetic...

متن کامل

Exact Attractive Non-BPS STU Black Holes

We develop some properties of the non-BPS attractive STU black hole. Our principle result is the construction of exact solutions for the moduli, the metric and the vectors in terms of appropriate harmonic functions. In addition, we find a spherically-symmetric attractor carrying p0 (D6 brane) and qa (D2 brane) charges by solving the non-BPS attractor equation (which we present in a particularly...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: International Journal of Modern Physics A

سال: 2000

ISSN: 0217-751X,1793-656X

DOI: 10.1142/s0217751x0000207x