Excitation of High-Spin States by Inelastic Proton Scattering

This work was supported by National Science Foundation Grant PHY 76-84033 and Indiana Universit

Excitation of High-Spin States by Inelastic Proton Scattering

This work was supported by National Science Foundation Grant PHY 75-00289 and Indiana Universit

Energy Dependence of Inelastic Proton Scattering to One-Particle One-Hole States in 28-Si

This work was supported by the National Science Foundation Grant NSF PHY 81-14339 and by Indiana Universit

Studies of Excited States in 208-Pb by Inelastic Proton Scattering at 100 MeV

This work was supported by the National Science Foundation Grant NSF PHY 78-22774 A02 & A03 and by Indiana Universit

Energy Dependence of Proton Inelastic Scattering Between 80 and 180 MeV

This work was supported by the National Science Foundation Grants NSF PHY 78-22774 A03, NSF PHY 81-14339, and by Indiana Universit

Studies of Excited States in 208-Pb by Inelastic Proton Scattering at 135 and 100 MeV

Supported by the National Science Foundation and Indiana Universit

Analyzing Power Measurements for the Excitation of States in 28-Si and 24-Mg by Inelastic Scattering of Polarized Protons

Supported by the National Science Foundation and Indiana Universit

Non-extremal black holes from the generalised r-map

We review the timelike dimensional reduction of a class of five-dimensional theories that generalises 5D, N = 2 supergravity coupled to vector multiplets. As an application we construct instanton solutions to the four-dimensional Euclidean theory, and investigate the criteria for solutions to lift to static non-extremal black holes in five dimensions. We focus specifically on two classes of models: STU-like models, and models with a block diagonal target space metric. For STU-like models the second order equations of motion of the four-dimensional theory can be solved explicitly, and we obtain the general solution. For block diagonal models we find a restricted class of solutions, where the number of independent scalar fields depends on the number of blocks. When lifting these solutions to five dimensions we show, by explicit calculation, that one obtains static non-extremal black holes with scalar fields that take finite values on the horizon only if the number of integration constants reduces by exactly half.Comment: 22 pages. Based on talk by OV at "Black Objects in Supergravity School" (BOSS2011), INFN, Frascati, Italy, 9-13 May, 201