Reissner

In other words, the approach to extremality is not continuous, as the non-extremal Reissner-Nordström solution splits into two spacetimes at extremality: an extremal black hole and a disconnected $AdS$ space.

Where Does the Entropy Go? Sean 2009

His romantic liaison with Larissa Reissner, his allegiance to Trotsky and later to Stalin, and his downfall following publication of a satire on Stalin, are treated in subsequent chapters.

Jim Tuck's homepage, biography and published works 2006

His romantic liaison with Larissa Reissner, his allegiance to Trotsky and later to Stalin, and his downfall following publication of a satire on Stalin, are treated in subsequent chapters.

Jim Tuck's homepage, biography and published works 2006

The Reissner-Nordström solution describes a black hole with electric charge, while the Kerr solution yields a rotating black hole.

the atomic uni-verse 2008

Why was he dissatisfied with the unification is apparent in, for example, the Reissner-Nordstorm solution?

Einstein’s Discovery of General Relativity, 1905-1915 cjohnson 2005

Recently, however, I discovered, in collaboration with Dr. Rosen, that the above mentioned simplest combination of the field equations of gravitation and electricity produces centrally symmetrical solutions which can be represented as free of singularity (the well known centrally symmetrical solutions of Schwarzschild for the pure gravitational field, and those of Reissner for the electric field with consideration of its gravitational action).

Out Of My Later Years Einstein, Albert, 1879-1955 1950

"Actually the question Nernst asked about curvature in 1916 was answered by Reissner in 1916 and ..."

Scientific Blogging 2010

All of them are almost exactly electrically neutral - so you don't need the Reissner-Nordström solutions if you're an astrophysicist.

The Reference Frame 2010

A fascinating property of a charged ( "Reissner-Nordström") black hole is that it has more than one event horizon.

Cosmic Variance 2009

In other words, the approach to extremality is not continuous, as the non-extremal Reissner-Nordström solution splits into two spacetimes at extremality: an extremal black hole and a disconnected $AdS$ space.

Cosmic Variance 2009