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Ellipticity imaging for visualizing and quantifying long and short range correlations in laser speckle data II: phantom and animal studies

Exact solutions in multidimensional gravity with antisymmetric forms and the solutions with p-branes (e.g. Majumdar-Papapetrou-type, cosmological, spherically symmetric, black

Dilaton gravity, charged dust, and (quasi-) black holesWe consider Einstein-Maxwell-dilaton gravity with charged dust and interaction of the form P

Long-term multi-wavelength variability and correlation study of Markarian 421 from 2007 to 2009

Dilaton gravity, (quasi-) black holes, and scalar charge presented) ((Formula presented)) and (Formula presented). If (Formula presented), the classical Majumdar

Dilaton gravity, (quasi-) black holes, and scalar charge). If (Formula presented), the classical Majumdar–Papapetrou (MP) system is restored. We discuss solutions

Ultra-high energy collisions in static space-times: single versus multi-black hole cases $$E_{c.m.}$$Ec.m. Collisions in the electro-vacuum Majumdar–Papapetrou metric (several extremal black

Ultra-high energy collisions in static space-times: single versus multi-black hole cases $$E_{c.m.}$$Ec.m. Collisions in the electro-vacuum Majumdar–Papapetrou metric (several extremal black

Dilaton gravity, (quasi-) black holes, and scalar charge). If (Formula presented), the classical Majumdar–Papapetrou (MP) system is restored. We discuss solutions

Quasi-black holes: General features and purely field configurationsMajumdar-Papapetrou systems

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