2017/11/28 by Z. Nekouee, Nekouee, Z., J. Sadeghi +4
Mathematics · Physics and Astronomy · #Advanced Differential Geometry Research #Commutative property #Computer science #Cosmology and Gravitation Theories #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #Geometry #High Energy Physics - Theory (hep-th) #Mathematical physics #Mathematics #Noncommutative and Quantum Gravity Theories #Physics #Pure mathematics #Relation (database) #Theoretical physics #gr-qc #hep-th
paper · pdf · doi:10.48550/arxiv.1711.10482
published in arXiv (Cornell University) (Cornell University) · 15 pages
openalex publication_date 2017/11/28 · arxiv created 2017/12/04 · arxiv updated 2017/12/05 · openalex created_date 2017/12/22 · openalex updated_date 2026/07/28
In this paper we employ the Horava-Lifshitz black holes solutions and obtain the corresponding Hamiltonian. It helps us to take new variables and it will be written by harmonic oscillator form. This leads us to apply non-commutative geometry to the new Hamiltonian and obtain the corresponding Lagrangian. And then, we take some information from Finsler geometry and write the Lagrangian of the different kinds of Horava-Lifshitz black holes. We show that the corresponding Lagrangian in non-commutative and Finsler geometry for above mentioned black holes completely coincidence together with some specification of parameters. But in case of rotation, the place of center of mass energy completely different, so the particle goes to inside of black hole rapidly without falling into singularity. So in that case, two Lagrangians cover each other at 0