Energy Extraction and Particle Acceleration in String-Inspired Rotating Einstein-Maxwell-Dilaton-Axion Black Hole

This paper demonstrates that negative dilaton hair in rotating Einstein-Maxwell-Dilaton-Axion black holes significantly enhances energy extraction efficiency and the rotational energy reservoir while expanding the parameter space for wave superradiance and preserving the Bañados-Silk-West divergence in particle collisions compared to standard Kerr black holes.

Arindam Kumar ChatterjeeMon, 09 Ma⚛️ gr-qc

Constraints on BMS Transformations via Energy Conditions and implications on black hole geometry

By expanding curvature tensors and recasting classical energy conditions as inequalities on metric perturbations, this study demonstrates that enforcing the strong, weak, null, and dominant energy conditions on a Schwarzschild background imposes significant angular restrictions on BMS supertranslations, thereby substantially reducing the space of physically admissible transformations despite their formal infinite dimensionality.

Nihar Ranjan Ghosh, Malay K. NandyMon, 09 Ma⚛️ gr-qc

Effects of Self-Interaction and of an Ideal Gas in Binary Mergers of Bosonic Dark Matter Cores

This study uses 3D simulations to demonstrate that while binary mergers of bosonic dark matter cores consistently produce stable solitonic remnants, the final mass retention is non-universal and critically depends on whether repulsive or attractive self-interactions are present, whereas the inclusion of an ideal gas component modifies the gravitational background without altering the intrinsic scaling of the bosonic core.

Carlos Tena-Contreras, Ivan Alvarez-Rios, Francisco S. Guzman, Jens NiemeyerMon, 09 Ma🔭 astro-ph

Disentangling the Galactic binary zoo: Machine learning classification of stellar remnant binaries in LISA data

This paper demonstrates that machine learning techniques, particularly gradient-boosting algorithms like XGBoost, can effectively classify and disentangle overlapping populations of stellar remnant binaries in simulated LISA data, achieving high recall rates for double white dwarf and high-mass systems while significantly outperforming statistical methods in identifying challenging neutron star-white dwarf binaries.

Irwin Khai Cheng Tay, Valeriya Korol, Thibault LechienMon, 09 Ma🔭 astro-ph

Spinor moving frame, type II superparticle quantization, hidden SU(8)SU(8) symmetry of linearized 10D supergravity, and superamplitudes

This paper utilizes a covariant spinor moving frame quantization of type IIA and IIB superparticles to reveal a hidden SU(8)SU(8) symmetry in linearized supergravity, demonstrating that both theories can be described by identical analytic on-shell superfields and superamplitudes while highlighting specific challenges in extending this formalism to include D0-branes.

Igor Bandos, Mirian TsulaiaMon, 09 Ma🔢 math

Quantum Big Bounce in Wheeler-DeWitt scattering theory: Ekpyrotic and LQC-like transitions

This paper presents a rigorous Wheeler-DeWitt scattering formulation of the Quantum Big Bounce for a closed isotropic universe with an ekpyrotic potential, demonstrating that while a LQC-like scenario requires regularization due to high-energy divergences, an ekpyrotic scenario with reversed internal time flow remains well-posed at all energy scales, thereby avoiding the cosmological singularity within standard quantum mechanics.

S. Lo Franco, G. MontaniMon, 09 Ma⚛️ gr-qc

Hybrid quantum-classical simulations of semiclassical gravity

This paper proposes and benchmarks a hybrid quantum-classical algorithm that iteratively simulates real-time dynamics of quantum fields coupled to classical fields to achieve self-consistent semiclassical backreaction, demonstrating its convergence and robustness in scalar-tensor modified gravity models relevant to cosmology.

Carlos Fulgado-Claudio, Daniel González-Cuadra, Jose Beltrán Jiménez, Alejandro BermudezMon, 09 Ma⚛️ quant-ph

Peeling of Dirac fields on Kerr spacetimes

This paper extends the study of peeling properties for scalar fields to Dirac fields on Kerr spacetimes by combining Penrose conformal compactification with geometric energy estimates to define peeling via Sobolev regularity near null infinity and establish optimal initial data spaces, confirming that decay and regularity assumptions in Kerr yield the same regularity across null infinity as in Minkowski space for all angular momentum values.

Pham Truong XuanFri, 13 Ma🔢 math-ph

Tidal deformability of black holes surrounded by thin accretion disks

This paper demonstrates that thin accretion disks can induce significant tidal Love numbers in black holes, potentially masking modified gravity effects and limiting tests of black-hole mimickers, while also showing that next-generation gravitational wave detectors like LISA and the Einstein Telescope could precisely measure these environmental tidal parameters.

Enrico Cannizzaro, Valerio De Luca, Paolo PaniFri, 13 Ma⚛️ gr-qc

Relational Dynamics with Periodic Clocks

This paper establishes a systematic framework for relational dynamics relative to periodic clocks in both classical and quantum theories, demonstrating the equivalence of three distinct quantization approaches, identifying limitations in the original Page-Wootters formalism for continuous spectra, and clarifying how periodic evolution with respect to one clock can coexist with monotonic evolution relative to another.

Leonardo Chataignier, Philipp A. Hoehn, Maximilian P. E. Lock, Fabio M. MeleFri, 13 Ma⚛️ gr-qc

Quintessential Implications of the presence of AdS in the Dark Energy sector

This paper utilizes joint cosmological observations to demonstrate that including a negative cosmological constant (AdS vacuum) in the dark energy sector provides a theoretically motivated mechanism that opens a finite non-phantom region in the Chevallier-Polarski-Linder parameter space while remaining consistent with current data and linking dark energy phenomenology to quantum gravity.

Purba Mukherjee, Dharmendra Kumar, Anjan A SenFri, 13 Ma⚛️ gr-qc

Systematic bias in LISA ringdown analysis due to waveform inaccuracy

This paper demonstrates that accurate parameter estimation for massive black hole binaries in the LISA band requires ringdown templates to include a specific minimum number of modes (ranging from 3–6 for typical systems to over 10 for high-SNR events) to prevent systematic biases caused by waveform truncation.

Lodovico Capuano, Massimo Vaglio, Rohit S. Chandramouli, Chantal L Pitte, Adrien Kuntz, Enrico BarausseFri, 13 Ma⚛️ gr-qc