Non-minimally coupled scalar field dark sector of the universe: in-depth (Einstein frame) case study

Motivated by recent DESI DR2 results suggesting evolving dark energy, this study analyzes spatially flat FLRW cosmological models with non-minimally coupled scalar fields in the Einstein frame, employing dynamical system methods to examine the evolution and stability of five specific scalar field models under various coupling parameters to understand energy transfer between the scalar sector and matter.

Marcin PostolakThu, 12 Ma⚛️ gr-qc

Quiescent Big Bang formation in $2+1$ dimensions

This paper proves that (2+1)(2+1)-dimensional solutions to the Einstein scalar-field Vlasov system, initially close to FLRW spacetimes on closed surfaces of arbitrary genus, exhibit stable Big Bang singularities with quiescent, velocity-term-dominated asymptotics and C2C^2-inextendibility, thereby establishing the Strong Cosmic Censorship conjecture for a corresponding class of polarized U(1)U(1)-symmetric vacuum solutions.

Liam UrbanThu, 12 Ma⚛️ gr-qc

Existence of nonlinearly scalarized black holes in Einstein-scalar-Gauss-Bonnet theory with polynomial couplings

This paper investigates the existence and stability of nonlinearly scalarized black holes in Einstein-scalar-Gauss-Bonnet theory with polynomial couplings, demonstrating that while quartic-only couplings stabilize Schwarzschild black holes, specific higher-order polynomial couplings induce instability and transition to scalarized states above certain pulse thresholds, with the resulting solution branches exhibiting universal features in the probe limit but distinct dependencies on coupling strength when backreaction is included.

De-Cheng Zou, Xu Yang, Meng-Yun Lai, Hyat Huang, Bo Liu, Jutta Kunz, Yun Soo Myung, Rui-Hong YueThu, 12 Ma⚛️ gr-qc

Unexpectedly Weak General Relativistic Effects in Strongly Relativistic Tidal Disruption Events

Contrary to the prevailing belief that strong relativistic effects rapidly dissipate orbital energy to form prompt accretion disks, general relativistic hydrodynamic simulations reveal that even in strongly relativistic tidal disruption events, debris remains highly eccentric and extended with circularization occurring intrinsically slowly due to stream self-interactions that weaken relativistic shocks.

Ho-Sang Chan, Taeho Ryu, Julian Krolik, Tsvi PiranThu, 12 Ma⚛️ gr-qc

Kick matters: The impact of a new recoil model on the retention of hierarchical black-hole remnants in globular clusters

By employing a state-of-the-art recoil-kick model (gwModel_flow_prec) instead of traditional analytic approximations, this study demonstrates that the retention probability of hierarchical black-hole merger remnants in globular clusters is significantly higher, thereby altering the resulting mass and spin distributions and offering new insights into the formation of massive binaries like GW231123.

Tousif Islam, Digvijay Wadekar, Konstantinos KritosThu, 12 Ma🔭 astro-ph

Thermal enhancement of inflationary magnetic fields

This paper proposes that assuming a thermal initial state for gauge fields during inflation, rather than the standard vacuum, introduces a dissipative boost that enhances primordial magnetic fields by up to $10^{16}$, suggesting that embedding this mechanism in a warm inflation framework offers a promising path to inflationary magnetogenesis without requiring non-minimal couplings or modified electrodynamics.

Arjun Berera, Suddhasattwa Brahma, Zizang Qiu, Rudnei O. RamosThu, 12 Ma🔭 astro-ph

Production of Gravitational Waves in the Early Universe From turbulence triggered by first-order phase transitions

This paper investigates the production of primordial gravitational waves from first-order phase transitions in the early universe by modeling the resulting plasma turbulence with relativistic hydrodynamics and comparing two existing models against a new approach that incorporates freely decaying turbulence with a time-dependent de-coherence function.

Yashmitha KumaranThu, 12 Ma⚛️ gr-qc

Gauss-Bonnet scalarization of charged qOS-black holes

This paper investigates the Gauss-Bonnet scalarization of charged quantum Oppenheimer-Snyder black holes within Einstein-Gauss-Bonnet-scalar theory coupled to nonlinear electrodynamics, demonstrating that while positive coupling allows scalarization for specific parameters, negative coupling induces a distinct, linearly stable scalarization mechanism within a narrow range of the action parameter.

Hong Guo, Wontae Kim, Yun Soo MyungThu, 12 Ma⚛️ gr-qc

On the angular localization of gravitational-wave signals by pulsar timing arrays

This paper provides a comprehensive analytical study of gravitational-wave signal localization by pulsar timing arrays, deriving expressions for sky localization precision that reveal how the interplay between pulsar-source angular proximity and distance measurement accuracy determines whether improvements stem from tighter distance constraints or the strategic addition of nearby pulsars.

Stephen R. TaylorThu, 12 Ma🔭 astro-ph