Astrophysics

Physics / Stellar & Compact Objects

Stellar physics, compact objects, and high-energy astrophysical phenomena. Research spans black hole thermodynamics, stellar evolution, radiative processes, and accretion physics.

16 Indexed Papers
2 Sources
17 Jul Last Updated
INSPIREOpenAlex

High-Energy Physics Literature

from INSPIRE-HEP
#1

SPH methods in the modelling of compact objects

Rosswog, Stephan 2026-07-16

We review the current status of compact object simulations that are based on the Smoothed Particle Hydrodynamics (SPH) method. The first section of this review is dedicated to SPH as a numerical method for Newtonian, ideal gas dynamics and it should be fairly self-contained. It begins with the basic

#2

Black-Hole Spin Measurements from X-ray Reflection Spectroscopy: Quality Criteria and Community Recommendations

Garcia, Javier A., Connors, Riley, Brenneman, Laura W. et al. 2026-07-15

X-ray reflection spectroscopy provides one of the most powerful electromagnetic methods for measuring the dimensionless spin of accreting black holes. It has yielded spin constraints for stellar-mass black holes in X-ray binaries and supermassive black holes in active galactic nuclei, and is central

#3

Here, There and Everywhere: How AGN jets affect galaxy cluster environments

Rosenberg, Isaac, Lokken, Martine, Hložek, Renée et al. 2026-07-14

Active galactic nuclei (AGN) feedback via black hole-driven jets and winds plays a key role in redistributing matter across megaparsec scales. However, the implementation of jet feedback in cosmological simulations remains highly prescriptive, leading to uncertainties in the predicted state of the W

#6

Periodic line-of-sight velocity-driven modulations to gravitational waves emitted by compact binaries in Keplerian outer orbits

Tiwari, Avinash, Kapadia, Shasvath J., Vijaykumar, Aditya et al. 2026-07-10 1 citations

The centre of mass (CoM) of compact binary coalescences (CBCs) occurring in the vicinity of a supermassive black hole, through interaction with an arbitrary third body (e.g., of stellar mass), or in a dense stellar environment, will undergo a time-varying line-of-sight (LOS) velocity. This in turn l

#7

Low-hard to high-soft spectral state transitions in the faintest early-X-ray-detected optical tidal disruption event TDE 2025aarm

Baldini, Pietro, Rau, Arne, Merloni, Andrea et al. 2026-07-10

We report the X-ray and optical spectroscopic properties of TDE 2025aarm, the second closest tidal disruption event (TDE) discovered to date. The proximity of this source, combined with a deep and intense X-ray monitoring campaign spanning six months, allowed us to probe the source down to an unprec

#8

Radio and X-Ray Flux Rebrightening Six Years after Outburst in a Partially Obscured Extreme Changing-look Active Galactic Nucleus

Zhou, Tianyao, Shu, Xinwen, Yang, Lei et al. 2026-07-10 Astrophys.J.

SDSS J1548+2208 is a unique partially obscured nuclear transient that exhibits multiwavelength outbursts in mid-infrared, X-rays, and radio. We present the results from multiwavelength photometric and spectroscopic follow-up observations with a time span of ∼2500 days since its discovery. We find th

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#3

High-Resolution ($2560^3$) Simulation of Primordial Black Hole Lattice Stabilization: The 73-Resonance and the Mizaan State

Mohamad Samir Hamieh 2029-05-11 Zenodo (CERN European Organization for Nuclear Research)

Overview This dataset provides the results of a high-fidelity cosmological simulation exploring the non-linear dynamics of a universe dominated by Primordial Black Holes (PBHs). The simulation was executed on NVIDIA Blackwell (B200) hardware at a native resolution of $2560^3$ ($16.7$ billion voxels)

#4

GIFT 2.2 - Supplement S7: Dimensional Observables

de La Fournière, Brieuc 2028-11-28 Zenodo (CERN European Organization for Nuclear Research)

This supplement extends the dimensionless predictions of the main document to absolute mass scales and cosmological observables, addressing the dimensional transmutation problem. It bridges dimensionless topological predictions to physical mass scales in GeV.

#5

GIFT 2.2 - Supplement S7: Dimensional Observables

de La Fournière, Brieuc 2028-11-28 Zenodo (CERN European Organization for Nuclear Research)

This supplement extends the dimensionless predictions of the main document to absolute mass scales and cosmological observables, addressing the dimensional transmutation problem. It bridges dimensionless topological predictions to physical mass scales in GeV.

#6

Cosmological Mechanics in the Cosmological Thermosynthesis Theory v3.2: Non-Singular Cyclic Dynamics, Emergent Gravity, and Falsifiable Predictions for Multi-Messenger Observations

Adrian G. Fernandez 2028-04-11 Zenodo (CERN European Organization for Nuclear Research)

This work presents a rigorous mathematical formulation of cosmological mechanics within the Cosmological Thermosynthesis Theory v3.2 (TTC v3.2). The theory posits that spacetime and all fundamental interactions emerge from a primordial superfluid of ultralight scalar bosons termed etherions, with ma

#7

Kleinian Group Structure of the FCC Bond Map and an Apollonian Foam Cosmology

J.J. Way 2028-02-28 Zenodo (CERN European Organization for Nuclear Research)

The third paper in a four-paper series connecting FCC lattice cohomology, Apollonian circle packing, and post-quantum cryptography. Papers 1 and 2 proved that the FCC cycle space carries a natural V4 symmetry and that the FCC primitive cell is the symmetric Apollonian seed in R³’¹, with the directed

#8

Human Remains: Everest and the Ontological Afterlives of George Mallory and Andrew Irvine

Jonathan Westaway 2028-01-01 CLOK (University of Central Lancashire)

The philosopher Giorgio Agamben has argued that the ‘human/nonhuman distinction is the conceptual ground for any further ontological elaboration’, (Grieve-Carlson, 179) that humans must distinguish themselves from their environment and other beings before the work of culture can begin. However, obje