Add to ORKG© 2016 World Scientific Publishing Company We consider collision of two particles in rotating spacetimes without horizons. If the metric coefficient responsible for rotation of spacetime is big enough, the energy of collisions in the center of mass frame can be as large as one likes. This can happen in the ergoregion only. The results are model-independent and apply both to relativistic stars and wormholes
International audienceThe most widely accepted model of Solar System formation, known as the Nebular...
© 2017 World Scientific Publishing CompanyIf two particles collide inside the ergosphere, the energy...
The rotating regular Hayward’s spacetime, apart from mass (M) and angular momentum (a), has an addit...
© 2016 World Scientific Publishing Company.We consider collision of two particles in rotating spacet...
© 2016, Springer Science+Business Media New York.We consider generic axially symmetric rotating spac...
© 2014 World Scientific Publishing Company. We consider collision of two particles in the axially sy...
Bañados et al. (BSW) found that Kerr black holes can act as particle accelerators with collisions at...
AbstractWe study the collision of two particles with the different rest masses moving in the equator...
© 2016 World Scientific Publishing Company.We consider collision of two geodesic particles near the ...
© 2018 American Physical Society. We consider collision of particles in a wormhole near its throat. ...
© 2017, Springer Science+Business Media New York. Properties of particles in Kerr metric are compare...
In this article, we have investigated collisional Penrose process (CPP) using spinning particles in ...
We study the collision of two geodesic particles in the accelerating and rotating black hole spaceti...
Ultrahigh energy particles in cosmic rays observed on the Earth can have their origin in the ergosph...
International audienceThe most widely accepted model of Solar System formation, known as the Nebular...
© 2017 World Scientific Publishing CompanyIf two particles collide inside the ergosphere, the energy...
The rotating regular Hayward’s spacetime, apart from mass (M) and angular momentum (a), has an addit...
© 2016 World Scientific Publishing Company.We consider collision of two particles in rotating spacet...
© 2016, Springer Science+Business Media New York.We consider generic axially symmetric rotating spac...
© 2014 World Scientific Publishing Company. We consider collision of two particles in the axially sy...
Bañados et al. (BSW) found that Kerr black holes can act as particle accelerators with collisions at...
AbstractWe study the collision of two particles with the different rest masses moving in the equator...
© 2016 World Scientific Publishing Company.We consider collision of two geodesic particles near the ...
© 2018 American Physical Society. We consider collision of particles in a wormhole near its throat. ...
© 2017, Springer Science+Business Media New York. Properties of particles in Kerr metric are compare...
In this article, we have investigated collisional Penrose process (CPP) using spinning particles in ...
We study the collision of two geodesic particles in the accelerating and rotating black hole spaceti...
Ultrahigh energy particles in cosmic rays observed on the Earth can have their origin in the ergosph...
International audienceThe most widely accepted model of Solar System formation, known as the Nebular...
© 2017 World Scientific Publishing CompanyIf two particles collide inside the ergosphere, the energy...
The rotating regular Hayward’s spacetime, apart from mass (M) and angular momentum (a), has an addit...