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19912026
most citedSciPy 1.0--Fundamental Algorithms for Scientific Computing in Python

40.2k citations

Showing 2012 · gr-qcShow all

13 papers · 2 filters

gr-qc2012

Fully Characterizing Axially Symmetric Szekeres Models With Three Data Sets

Marie-Noëlle Célérier, Priti Mishra, Tejinder P. Singh

Inhomogeneous exact solutions of General Relativity with zero cosmological constant have been used in the literature to challenge the ΛCDM model. From one patch Lemaître-Tolman-Bon…

gr-qc2012★ 104 cited

An effectual template bank for the detection of gravitational waves from inspiralling compact binaries with generic spins

P. Ajith, N. Fotopoulos, S. Privitera +3

We report the construction of a three-dimensional template bank for the search for gravitational waves from inspiralling binaries consisting of spinning compact objects. The parame…

gr-qc2012★ 11 cited

Noise Kernel for Self-similar Tolman Bondi Metric: Fluctuations on Cauchy Horizon

Seema Satin, Kinjalk Lochan, Sukratu Barve

We attempt to calculate the point separated Noise Kernel for self similar Tolman Bondi metric, using a method similar to that developed by Eftekharzadeh et. al for ultra-static spa…

gr-qc2012★ 84 cited

Can strong gravitational lensing distinguish naked singularities from black holes?

Satyabrata Sahu, Mandar Patil, D. Narasimha +1

In this paper we study gravitational lensing in the strong field limit from the perspective of cosmic censorship, to investigate whether or not naked singularities, if at all they…

gr-qc2012★ 3 cited

Statistical analysis of entropy correction from topological defects in Loop Black Holes

Kinjalk Lochan, Cenalo Vaz

In this paper we discuss the entropy of quantum black holes in the LQG formalism when the number of punctures on the horizon is treated as a quantum hair, that is we compute the bl…

gr-qc2012★ 15 cited

Shell-crossings in Gravitational Collapse

Pankaj S. Joshi, Ravindra V. Saraykar

While studying the continual gravitational collapse of a massive matter cloud in general relativity towards examining collapse final states, an important issue is that of whether s…

gr-qc2012★ 7 cited

Modified gravity as a common cause for cosmic acceleration and flat galaxy rotation curves

Priti Mishra, Tejinder P. Singh

Flat galaxy rotation curves and the accelerating Universe both imply the existence of a critical acceleration, which is of the same order of magnitude in both the cases, in spite o…

gr-qc2012★ 14 cited

Hawking radiation from dynamical horizons

Ayan Chatterjee, Bhramar Chatterjee, Amit Ghosh

In completely local settings, we establish that a dynamically evolving black hole horizon can be assigned a Hawking temperature. Moreover, we calculate the Hawking flux and show th…

gr-qc2012★ 8 cited

Tunneling during Quantum Collapse in AdS Spacetime

Cenalo Vaz, Kinjalk Lochan

We extend previous results on the reflection and transmission of self-gravitating dust shells across the apparent horizon during quantum dust collapse to non-marginally-bound dust…

gr-qc2012★ 16 cited

Statistical thermodynamics for a non-commutative special relativity: Emergence of a generalized quantum dynamics

Kinjalk Lochan, Seema Satin, Tejinder P. Singh

There ought to exist a description of quantum field theory which does not depend on an external classical time. To achieve this goal, in a recent paper we have proposed a non-commu…

gr-qc2012★ 38 cited

Ultra-high energy particle collisions in a regular spacetime without blackholes or naked singularities

Mandar Patil, Pankaj S. Joshi

We investigate here the particle acceleration and collisions with extremely large center of mass energies in a perfectly regular spacetime containing neither singularity nor an eve…

gr-qc2012★ 6 cited

Canonical Partition function of Loop Black Holes

Kinjalk Lochan, Cenalo Vaz

We compute the canonical partition for quantum black holes in the approach of Loop Quantum Gravity (LQG). We argue that any quantum theory of gravity in which the horizon area is b…

gr-qc2012★ 240 cited

Recent developments in gravitational collapse and spacetime singularities

Pankaj S. Joshi, Daniele Malafarina

It is now known that when a massive star collapses under the force of its own gravity, the final fate of such a continual gravitational collapse will be either a black hole or a na…