© 2014 World Scientific Publishing Company. We consider collision of two particles in the axially symmetric black hole metric in the magnetic field. If the value of the angular momentum |L| of one particles grows unbound (but its Killing energy remains fixed) one can achieve unbound energy in the center-of-mass frame Ec.m. In the absence of the magnetic field, collision of this kind is known to happen in the ergoregion. However, if the magnetic field strength B is also large, with the ratio |L|/B being finite, large Ec.m. can be achieved even far from a black hole, in the almost flat region. Such an effect also occurs in the metric of a rotating star
© 2016 World Scientific Publishing Company.We consider collision of two geodesic particles near the ...
© 2016 World Scientific Publishing Company.We consider collision of two geodesic particles near the ...
© 2015 World Scientific Publishing Company. There are different versions of collisions of two partic...
© 2014 World Scientific Publishing Company. We consider collision of two particles in the axially sy...
© 2014 World Scientific Publishing Company. We consider collision of two particles in the axially sy...
© 2014 World Scientific Publishing Company. We consider collision of two particles in the axially sy...
We consider collision between two charged (or charged and neutral) particles near the black hole hor...
© 2015, The Author(s). We consider the behavior of the innermost stable circular orbit (ISCO) in the...
© 2015, The Author(s). We consider the behavior of the innermost stable circular orbit (ISCO) in the...
© 2015, The Author(s). We consider the behavior of the innermost stable circular orbit (ISCO) in the...
We consider collision between two charged (or charged and neutral) particles near the black hole hor...
We consider collision between two charged (or charged and neutral) particles near the black hole hor...
We consider collision between two charged (or charged and neutral) particles near the black hole hor...
We consider the behavior of the innermost stable circular orbit (ISCO) in the magnetic field near “d...
© 2015 World Scientific Publishing Company. There are different versions of collisions of two partic...
© 2016 World Scientific Publishing Company.We consider collision of two geodesic particles near the ...
© 2016 World Scientific Publishing Company.We consider collision of two geodesic particles near the ...
© 2015 World Scientific Publishing Company. There are different versions of collisions of two partic...
© 2014 World Scientific Publishing Company. We consider collision of two particles in the axially sy...
© 2014 World Scientific Publishing Company. We consider collision of two particles in the axially sy...
© 2014 World Scientific Publishing Company. We consider collision of two particles in the axially sy...
We consider collision between two charged (or charged and neutral) particles near the black hole hor...
© 2015, The Author(s). We consider the behavior of the innermost stable circular orbit (ISCO) in the...
© 2015, The Author(s). We consider the behavior of the innermost stable circular orbit (ISCO) in the...
© 2015, The Author(s). We consider the behavior of the innermost stable circular orbit (ISCO) in the...
We consider collision between two charged (or charged and neutral) particles near the black hole hor...
We consider collision between two charged (or charged and neutral) particles near the black hole hor...
We consider collision between two charged (or charged and neutral) particles near the black hole hor...
We consider the behavior of the innermost stable circular orbit (ISCO) in the magnetic field near “d...
© 2015 World Scientific Publishing Company. There are different versions of collisions of two partic...
© 2016 World Scientific Publishing Company.We consider collision of two geodesic particles near the ...
© 2016 World Scientific Publishing Company.We consider collision of two geodesic particles near the ...
© 2015 World Scientific Publishing Company. There are different versions of collisions of two partic...