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Physics & Astronomy
Physics and astronomy have shared new results on arXiv for over thirty years. This page shows the newest papers ReadSearch has read there, from astrophysics and condensed matter to particle, quantum and applied physics, with papers OpenAlex files under the same subjects.
The newest 1,000 papers, from 29 October 2026 to 5 November 2026: 1,000 arXiv preprints.
Newest papers, page 42
Time-Domain Multiplexing for Resource-Efficient Heralded GKP State Preparation
Gottesman-Kitaev-Preskill (GKP) states are key resources for fault-tolerant photonic quantum computing, but their conditional preparation via Gaussian boson sampling involves a trade-off between…Stellar Bars Reshape the Spatial Distribution of UV-bright Clumps in Nearby Galaxies
Stellar bars redistribute gas and angular momentum in disk galaxies, but whether they mainly change the amount or the spatial organization of recent star formation remains uncertain.Non-Hermitian Spectral Topology Shaped by Memory
Non-Hermitian spectral topology has transformed our understanding of bulk--boundary correspondence in open systems, yet its exploration has largely remained within the Markovian regime of…Loss-aware optimization of realistic GKP gid states
Realistic preparation of Gottesman-Kitaev-Preskill (GKP) states, the prime candidates for quantum computation with bosonic systems, is inevitably burdened by photon loss.Reconfigurable Generation of Terahertz Spiral Vector Beams Based on All-Dielectric Cascaded Metasurfaces
The reconfigurable generation of complex structured terahertz (THz) fields, and vector beams in particular, remains a significant challenge.Kinematic Map of the Galactic Bulge Using HST Proper Motions
Constraining the Galactic bulge's non-axisymmetric dynamics requires proper motions in deep fields across many sightlines, yet crowding and extinction limit such measurements.Distilling Knowledge from Search: Decoder Model Factory for Quantum LDPC Codes
We introduce GraphMP, a learning-based message-passing decoder for quantum low-density parity-check codes that transfers without fine-tuning across code families, code sizes, physical error rates…Helper-assisted quantum sensing with low dressed-state leakage
We study a two-qubit sensing protocol in which only a helper qubit is read out.Real-time BP decoding of a high-rate QEC code
We present a real-time FPGA decoder for a high-rate $[[512,174,8]]$ 3D product qLDPC code.Analytic level statistics of the quantum Rabi model
We derive an analytic expression for the distribution of level spacings in the quantum Rabi model.Resolving the Complex Line-Locking Structure in Quasar J004613+010425 with VLT/X-shooter Spectroscopy
Line-locking (LL) signatures in quasar absorption-line systems provide direct observational evidence for radiatively driven outflows.oracq: A Modular Framework for Implementing and Analyzing Quantum Scientific Computing Algorithms
Quantum algorithms for scientific computing are specified against access models such as block-encodings, sparse oracles, state preparations, and quantum random-access memories.Almost-Quantum Correlations Violate Information Causality
Information causality (IC) posits that communicating m classical bits cannot give the receiver access to more than m bits of information about the sender's independent data.An Unbounded Separation of Almost-Quantum and Commuting-Operator Correlations in Zero-Error Communication
Almost-quantum correlations form the $\mathtt{1+AB}$ level of the Navascués--Pironio--Acín hierarchy.Cryogenic Optical Characteristics of S-FPL51 and S-LAH71: Refractive index, Transmission and Thermal expansion
Several near-infrared instruments on upcoming extremely large telescopes use a combination of OHARA S-FPL51 and S-LAH71 glass prisms to correct for the atmospheric differential refraction.OASIS I: Spectroscopy of Mini-Quenched and Lulling Galaxies Constrains the Quiet Side of Bursty Star Formation at z > 4
JWST has revealed that star formation in early galaxies is bursty, including episodes of violent suppression, so-called mini-quenching.OASIS II: The Ionized Gas Traces Feedback-Driven Declines into the Quiet Side of Bursty Star Formation at z > 4
Models of bursty star formation in low-mass (10^8-10^9.5 Msun) galaxies at z>4 differ most in the suppressed phases: what drives the decline, how fast star formation falls, and how long it stays low.OASIS III: Bursty star formation drives observed galaxy sizes at $z\geq4$
We employ JWST/NIRSpec MSA PRISM spectroscopy together with NIRCam imaging to investigate the impact of star-formation variability on galaxy sizes for a representative sample of 51 galaxies at…As a matter of reconstruction -- varying the magnetic Prandtl number in implicit large eddy simulations
The magnetic Prandtl number ($\mathrm{Pm}$), the ratio of viscosity to magnetic diffusivity, spans many orders of magnitude in astrophysical plasmas.Characterization of Phase Transitions with the Annealed Importance Sampling Algorithm
We We explore the use of the Annealed Importance Sampling (AIS) algorithm as a numerical tool to study phase transitions and critical phenomena.
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