activity
20132024
most citedQuantum gravity predictions for black hole interior geometry

85 citations · 256 across the 11 of their papers we have counts for

collaborators

11 papers

quant-ph2024★ 2 cited

Particle-conserving quantum circuit ansatz with applications in variational simulation of bosonic systems

Sina Bahrami, Nicolas Sawaya

Constrained problems are frequently encountered in classical and quantum optimization. Particle conservation, in particular, is commonly imposed when studying energy spectra of che…

hep-th2022★ 19 cited

Loop corrections in Minkowski spacetime away from equilibrium. Part II. Finite-time results

Spasen Chaykov, Nishant Agarwal, Sina Bahrami +1

Loop corrections to finite-time correlation functions in quantum field theories away from equilibrium can be calculated using the in-in path integral approach. In this paper, we ca…

hep-th2022★ 20 cited

Loop corrections in Minkowski spacetime away from equilibrium. Part I. Late-time resummations

Spasen Chaykov, Nishant Agarwal, Sina Bahrami +1

Loop corrections to unequal-time correlation functions in Minkowski spacetime exhibit secular growth due to a breakdown of time-dependent perturbation theory. This is analogous to…

gr-qc2020★ 29 cited

Asymptotically de Sitter Universe inside a Schwarzschild black hole

Emanuele Alesci, Sina Bahrami, Daniele Pranzetti

Extending our previous analysis, we study the interior of a Schwarzschild black hole derived from a partial gauge fixing of the full Loop Quantum Gravity Hilbert space, this time i…

gr-qc2019★ 85 cited

Quantum gravity predictions for black hole interior geometry

Emanuele Alesci, Sina Bahrami, Daniele Pranzetti

In a previous work we derived an effective Hamiltonian constraint for the Schwarzschild geometry starting from the full loop quantum gravity Hamiltonian constraint and computing it…

gr-qc2019★ 26 cited

Asymptotics with a positive cosmological constant: IV. The `no-incoming radiation' condition

Abhay Ashtekar, Sina Bahrami

Consider compact objects --such as neutron star or black hole binaries-- in \emph{full, non-linear} general relativity. In the case with zero cosmological constant , the gravita…