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We study ultra-high-energy particle collisions and optical effects in the extraordinary class of mining braneworld Kerr-Newman (KN) naked singularity spacetimes, predicting extremely high efficiency of Keplerian accretion, and compare the results to those related to the other classes of the KN naked singularity and black hole spacetimes.
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Z. Stuchlík and M. Calvani · 1991
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The Shell of Incoherent Charged Matter Falling onto a Charged Rotating Black Hole
Z. Stuchlík, J. Bičák, and V. Balek · 1999
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Z. Stuchlík and S. Hledík · 1999
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N. Dadhich, R. Maartens, P. Papadopoulos, and V. Rezania · 2000
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T. Shiromizu, K.-I. Maeda, and M. Sasaki · 2000
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Equatorial photon motion in the Kerr-Newman spacetimes with a non-zero cosmological constant
Z. Stuchlík and S. Hledík · 2000
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Stars in the braneworld
C. Germani and R. Maartens · 2001
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Equatorial circular motion in Kerr spacetime
D. Pugliese, H. Quevedo, and R. Ruffini · 2011
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Z. Stuchlík, S. Hledík, and K. Truparová · 2011
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Shadow of a rotating braneworld black hole
L. Amarilla and E. F. Eiroa · 2012
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Upper limits of particle emission from high-energy collision and reaction near a maximally rotating Kerr black hole
T. Harada, H. Nemoto, and U. Miyamoto · 2012
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Trapping of Neutrinos in Extremely Compact Stars and the Influence of Brane Tension on This Process
Z. Stuchlík, J. Hladík, and M. Urbanec · 2012
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Observational phenomena related to primordial Kerr superspinars
Z. Stuchlík and J. Schee · 2012
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Charged rotating black holes on a 3-brane
A. N. Aliev and A. E. Gümrükçüoǧlu · 2005
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