activity
20102026
most citedNeural Network Prediction of solar cycle 24

23 citations · 32 across the 8 of their papers we have counts for

collaborators

11 papers

astro-ph.HE2026

Angular structure of finite-field vacuum birefringence in magnetars

Shahram Abbassi, S. R. Valluri

Vacuum birefringence in a strong magnetic field is often modelled by combining the finite-field splitting for perpendicular propagation with the familiar angular factor.…

astro-ph.HE2026

Validating Inverse Fundamental-Plane IMBH Mass Estimates in the SKA/ngVLA Era

Shahram Abbassi, Samik Mitra, Ramananda Santra

The radio/X-ray/black-hole-mass Fundamental Plane (FP) is widely used to estimate masses of accreting intermediate-mass black hole (IMBH) candidates. Its inverse use is justified o…

astro-ph.HE2026

Thermal Stability of Radiation-Pressure-Dominated Accretion Disks Threaded by Net Vertical Magnetic Flux

Shahram Abbassi, Armin Memarian, Samik Mitra

The classical radiation-pressure instability predicts strong thermal variability in luminous black-hole accretion disks, whereas most disk-dominated X-ray binary soft states remain…

astro-ph.GA2026

Classifying Quasar Types Without a Spectrum

Adrien Hélias, Pauline Barmby, Sarah C. Gallagher +2

Distinguishing between Type 1 and Type 2 quasars is important because it helps us understand accretion regimes, black hole mass scaling, disk instabilities and feedback processes i…

astro-ph.HE2026

Braking indices as probes of r-mode spin-down in young pulsars

Shahram Abbassi, Armin Memarian, Evelyn Sophia Guest +1

We present a timing-based framework for interpreting braking-index measurements in young pulsars using a four-channel spin-down model that includes particle-wind, magnetic-dipole,…

astro-ph.SR2026

Early Stages of Protostellar Disk Evolution: A Link to the Initial Cloud Core

Majd Noel, Rahul Khanna, Shahram Abbassi +2

We study the structure and evolution of the very early protostellar disk (``protodisk'') just after protostar formation, where disk self-gravity dominates and the stellar contribut…

astro-ph.GA2026

Long Term (250 years) Hydrodynamical Simulation of the Supermassive Black Hole Binary OJ287

Ariel Chitan, Sarah C. Gallagher, Shahram Abbassi

With upcoming facilities capable of detecting photometric and gravitational wave signals from supermassive black hole (SMBH) binaries, studying their long-term accretion-driven var…

astro-ph.GA2024★ 1 cited

Prospects for Revealing Intermediate-Mass Black Holes in NGC 1399 using SKA

B. Karimi, P. Barmby, S. Abbassi

This study investigates the detectability of intermediate-mass black holes (IMBHs) within the mass range solar masses in the globular star clusters of NGC 1399 at a fre…

astro-ph.GA2024★ 6 cited

The redshift evolution of galactic bar pattern speed in TNG50

Asiyeh Habibi, Mahmood Roshan, Mohammad Hosseinirad +4

In this paper, the redshift evolution of the galactic bar properties, like the bar length, pattern speed, and bar fraction, has been investigated for simulated galaxies at stellar…

astro-ph.HE2023★ 2 cited

The Role of r-Modes in Pulsar Spin-down, Pulsar Timing, and Gravitational Waves

Xiyuan Li, Shahram Abbassi, Varenya Upadhyaya +2

We investigate the role of r-mode oscillations in pulsar spin-down and their implications for gravitational wave emission and pulsar timing analysis. Using a non-linear differentia…

astro-ph.SR2010★ 23 cited

Neural Network Prediction of solar cycle 24

A. Ajabshirizadeh, N. Masoumzadeh Jouzdani, S. Abbassi

The ability to predict the future behavior of solar activity has become of extreme importance due to its effect on the near Earth environment. Predictions of both the amplitude and…