Free motion around black holes with discs or rings: Between integrability and chaos. VI. The Melnikov method
L Polcar, O Semerák - Physical Review D, 2019 - APS
Motivated by black holes surrounded by accretion structures, we consider in this series static
and axially symmetric black holes “perturbed” gravitationally as being encircled by a thin …
and axially symmetric black holes “perturbed” gravitationally as being encircled by a thin …
[PDF][PDF] Free motion around black holes with discs or rings: Between integrability and chaos. VI. The Melnikov method
L Polcar, O Semerák - PHYSICAL REVIEW D Phys Rev D, 2019 - utf.mff.cuni.cz
In astrophysical models of accreting black holes, the gravitational effect of the accreting
material is usually neglected, hence the space-time is being described by the Kerr or …
material is usually neglected, hence the space-time is being described by the Kerr or …
Free motion around black holes with discs or rings: Between integrability and chaos. VI. The Melnikov method
L Polcar, O Semerák - Phys. Rev. D, 2019 - inspirehep.net
Motivated by black holes surrounded by accretion structures, we consider in this series static
and axially symmetric black holes “perturbed” gravitationally as being encircled by a thin …
and axially symmetric black holes “perturbed” gravitationally as being encircled by a thin …
Free motion around black holes with discs or rings: Between integrability and chaos. VI. The Melnikov method
L Polcar, O Semerák - Physical Review D, 2019 - ui.adsabs.harvard.edu
Motivated by black holes surrounded by accretion structures, we consider in this series static
and axially symmetric black holes" perturbed" gravitationally as being encircled by a thin …
and axially symmetric black holes" perturbed" gravitationally as being encircled by a thin …
[PDF][PDF] Free motion around black holes with discs or rings: between integrability and chaos–VI. The Melnikov method
L Polcar, O Semerák - arXiv preprint arXiv:1911.09790, 2019 - researchgate.net
Motivated by black holes surrounded by accretion structures, we consider in this series static
and axially symmetric black holes “perturbed” gravitationally as being encircled by a thin …
and axially symmetric black holes “perturbed” gravitationally as being encircled by a thin …
Free motion around black holes with discs or rings: between integrability and chaos--VI. The Melnikov method
L Polcar, O Semerák - arXiv preprint arXiv:1911.09790, 2019 - arxiv.org
Motivated by black holes surrounded by accretion structures, we consider in this series static
and axially symmetric black holes" perturbed" gravitationally as being encircled by a thin …
and axially symmetric black holes" perturbed" gravitationally as being encircled by a thin …
[引用][C] Free motion around black holes with discs or rings: Between integrability and chaos. VI. The Melnikov method
L Polcar, O Semerák - Physical Review D, 2019 - cir.nii.ac.jp
Free motion around black holes with discs or rings: Between integrability and chaos. VI. The
Melnikov method | CiNii Research CiNii 国立情報学研究所 学術情報ナビゲータ[サイニィ] 詳細へ …
Melnikov method | CiNii Research CiNii 国立情報学研究所 学術情報ナビゲータ[サイニィ] 詳細へ …
[PDF][PDF] Free motion around black holes with discs or rings: Between integrability and chaos. VI. The Melnikov method
L Polcar, O Semerák - PHYSICAL REVIEW D Phys Rev D, 2019 - utf.mff.cuni.cz
In astrophysical models of accreting black holes, the gravitational effect of the accreting
material is usually neglected, hence the space-time is being described by the Kerr or …
material is usually neglected, hence the space-time is being described by the Kerr or …
[PDF][PDF] Free motion around black holes with discs or rings: between integrability and chaos–VI. The Melnikov method
L Polcar, O Semerák - researchgate.net
Motivated by black holes surrounded by accretion structures, we consider in this series static
and axially symmetric black holes “perturbed” gravitationally as being encircled by a thin …
and axially symmetric black holes “perturbed” gravitationally as being encircled by a thin …