We consider collision between two charged (or charged and neutral) particles near the black hole horizon in the strong magnetic field B. It is shown that there exists a strip near the horizon within which collision of any two such particles leads to ultrahigh energy in the center-of-mass frame (CM frame). The results apply to generic (not necessarily vacuum) black holes. © 2014 World Scientific Publishing Company
© 2015 World Scientific Publishing Company. There are different versions of collisions of two partic...
We consider the behavior of the innermost stable circular orbit (ISCO) in the magnetic field near “d...
© 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...
© 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...
© 2014 World Scientific Publishing Company. We consider collision of two particles in the axially sy...
© 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...
© 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...
We consider the behavior of the innermost stable circular orbit (ISCO) in the magnetic field near “d...
© 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...
© 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...
© 2014 World Scientific Publishing Company. We consider collision of two particles in the axially sy...
© 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...
© 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...
We consider the behavior of the innermost stable circular orbit (ISCO) in the magnetic field near “d...
© 2015, The Author(s). We consider the behavior of the innermost stable circular orbit (ISCO) in the...