collaborators

9 papers

astro-ph.EP2026

Size, shape, density, and atmospheric limit of (50000) Quaoar revealed from 14 years of stellar occultation

Giuliano Margoti, Felipe Braga-Ribas, José Luis Ortiz +173

We present results from 28 stellar occultations by the large Trans-Neptunian Object (50000) Quaoar registered between 2018 and 2025. By performing a joint analysis of this occultat…

gr-qc2026

Exciting the Vacuum: Non-Thermal Particle Bursts and Multi-Messenger Signals from Binary Black Holes

Sohrab Rahvar

We investigate particle production in the dynamical curved spacetime of a binary black hole system. Particle production is a well-known feature of quantum field theory in curved sp…

astro-ph.CO2026

Cosmological Tensions in a Gauge-Invariant Modified Gravity

Zahra Tabatabaei, Sohrab Rahvar, Shahin Rouhani

In this work, we investigate a gauge-invariant formulation of modified gravity (GIMOG) wherein the gravitational interaction emerges dynamically from a scalar field following a fir…

astro-ph.CO2026

The Oort Cloud as a Gravitational Detector for Primordial Black Holes

Sohrab Rahvar

Planetary systems can act as sensitive gravitational detectors for dark matter. We investigate the gravitational scattering of Oort cloud objects by primordial black holes (PBHs) a…

astro-ph.GA2026

Constraining the Lifespan of Intelligent Technological Civilization in the Galaxy

Sohrab Rahvar, Shahin Rouhani

In this work, we explore constraints on the emergence and longevity of technologically intelligent civilizations in our Galaxy, considering the Fermi paradox. We argue that under o…

astro-ph.CO2026

Addressing Dipole Tension via Clustering in CDM and beyond

Arefeh Daei Rasouli, Haniyeh S. Tadayyoni, Shant Baghram +1

The dipole in the angular distribution of the cosmic microwave background (CMB) is attributed to the Doppler effect and our motion relative to the CMB rest frame. It is expected th…