On black hole formation in higher dimensions

نویسندگان

چکیده

The two main processes of black hole formation are collapse a matter cloud under its own gravity and accretion onto an already existing gravitating centre. necessary condition for both the to operate is that overall force on collapsing fluid element or test accreting particles attractive. It turns out this not case in general higher dimensions greater than usual four having nonzero angular momentum. Thus, these cannot form rotating hole. only theory which pure Lovelock gravity, where could principle work holes.

برای دانلود رایگان 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

Accelerating a Black Hole in Higher Dimensions

Utilising the master equation with source for perturbations of the SchwarzschildTangherlini solution, we construct perturbative solutions representing a black hole accelerated by a string in higher dimensions. We show that such solutions can be uniquely determined by a single function representing the local tension of the string, under natural asymptotic and regularity conditions. We further st...

متن کامل

Black hole hair in higher dimensions

We study the property of matter in equilibrium with a static, spherically symmetric black hole in D-dimensional spacetime. It requires this kind of matter has an equation of state ω ≡ pr/ρ = −1/(1 + 2kn), k, n ∈ N, which seems to be independent of D. However, when we associate this with specific models, some interesting limits on space could be found: (i)D = 2 + 2kn while the black hole is surr...

متن کامل

Black Holes in Higher Dimensions

We review black-hole solutions of higher-dimensional vacuum gravity and higher-dimensional supergravity theories. The discussion of vacuum gravity is pedagogical, with detailed reviews of Myers-Perry solutions, black rings, and solution-generating techniques. We discuss black-hole solutions of maximal supergravity theories, including black holes in anti-de Sitter space. General results and open...

متن کامل

Black hole entropy in two dimensions.

Black hole entropy is studied for an exactly solvable model of two-dimensional gravity[1], using recently developed Noether charge techniques[2]. This latter approach is extended to accomodate the non-local form of the semiclassical effective action. In the two-dimensional model, the final black hole entropy can be expressed as a local quantity evaluated on the horizon. This entropy is shown to...

متن کامل

Multi-black hole solutions in five dimensions

Using a recently developed generalized Weyl formalism, we construct an asymptotically flat, static vacuum Einstein solution that describes a superposition of multiple five-dimensional Schwarzschild black holes. The spacetime exhibits a U(1)×U(1) rotational symmetry. It is argued that for certain choices of parameters, the black holes are collinear and so may be regarded as a five-dimensional ge...

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 D

سال: 2021

ISSN: ['1793-6594', '0218-2718']

DOI: https://doi.org/10.1142/s0218271821501200