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Physics

arXiv preprints from January 1, 2026 through July 28, 2026 — 09:22:03 EST

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Posted in astro-ph.HE · 2026-01-02 · Olivia Aspegren, Daniel Kasen

The Emission and Suppression of Line Features in Luminous Transients

Featureless optical and ultraviolet (UV) spectra are a puzzling signature to emerge from recent observations of luminous fast blue optical transients (LFBOTs) and some tidal disruption events (TDEs). We describe the landscape of source and gas properties that are expected to form H, He I and He II emission lines, and map spectral...

💬 0 commentsarXiv:2601.00947v2PDF
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Posted in astro-ph.EP · 2026-01-02 · Kaitlyn T. Lane, Alexander P. Stephan, Melinda Soares-Furtado, Keivan G. Stassun, Ricardo Yarza

Observable Metal Pollution in Main-Sequence Stars: Simulations of Rocky Planets Engulfed by Stars in the $0.5$ to $1.4$ M$_\odot$ Range

The engulfment of planets by their host stars is an expected outcome of various dynamical processes and has been invoked to explain a variety of observed stellar properties, such as rapid rotation, chemical abundance abnormalities, and other transient phenomena. Recent observations support engulfment as the cause of such signatures;...

💬 0 commentsarXiv:2601.00949v1PDF
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Posted in astro-ph.GA · 2026-01-02 · Hayden R. Foote, Himansh Rathore, Gurtina Besla, Nicolás Garavito-Camargo, Ekta Patel, Michael S. Petersen, Martin D. Weinberg, Facundo A. Gómez, Chervin F. P. Laporte

Mapping the Distorted Dark Matter Distribution of the LMC-SMC System Prior to Milky Way Infall with Basis Function Expansions

The SMC orbits within the LMC's dark matter (DM) halo in a $\sim$1:10 mass-ratio encounter. The LMC:Milky Way (MW) interaction is also $\sim$1:10, and is expected to perturb the MW's DM distribution. However, no framework exists to quantify the severity of these perturbations over multiple pericenters and longer periods of time, such...

💬 0 commentsarXiv:2601.00946v2PDF
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Posted in hep-ph · 2026-01-02 · Henning Bahl, Jens Braun, Gudrun Heinrich, Tilman Plehn, Rebecca Revelli

How to Trust Learned Loop Amplitudes

Higher-order theory predictions are crucial for the precision LHC program, but the time-consuming amplitude evaluation challenges the corresponding Monte-Carlo simulations. Machine-learned amplitude surrogates can resolve this problem, if we can guarantee their precision over the entire phase space. First, we show that our surrogates...

💬 0 commentsarXiv:2601.00950v2PDF
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Posted in astro-ph.HE · 2026-01-02 · Ian Crawshaw, Tianlu Yuan, Emre Yildizci, Lu Lu, Anatoli Fedynitch

Probabilistic modeling of Cherenkov emission from particle showers

Subatomic particles can interact with target nuclei in matter or decay in flight, and an individual high-energy particle can induce a particle shower composed of numerous, lower-energy secondaries. These particle showers broadly exhibit universality across diverse media, including air, water, ice, and other materials, with their...

💬 0 commentsarXiv:2601.00944v3PDF
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Posted in astro-ph.SR · 2026-01-02 · Kareem El-Badry, Antonio C. Rodriguez, Matthew J. Green, Kevin B. Burdge

JWST observations of three long-period AM CVn binaries: detection of the donors and hints of magnetically truncated disks

We present JWST/NIRSpec high-cadence infrared spectroscopy of three long-period, eclipsing AM CVn binaries, Gaia14aae, SRGeJ0453, and ZTFJ1637. These systems have orbital periods of 50-62 minutes and cool donors that are undetectable in the optical. The data cover a wavelength range of 1.6-5.2 $μ$m at resolution $R=1000-2000$. We...

💬 0 commentsarXiv:2601.00945v2PDF
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Posted in astro-ph.HE · 2026-01-02 · Fatima Zaidouni, Erin Kara, Peter Kosec, Ehud Behar, Richard Mushotzky, Michael Koss, Anna Juráňová, Elias Kammoun, Laura W. Brenneman, Joheen Chakraborty, Ken Ebisawa, Megan E. Eckart, Andrew C. Fabian, Yasushi Fukazawa, Javier A. García, Liyi Gu, Megan Masterson, Shoji Ogawa, Takashi Okajima, Stéphane Paltani, Daniele Rogantini, Yuichi Terashima, Brian J. Williams, Satoshi Yamada

XRISM finds the Changing-Look AGN NGC 1365 in an extended low state: A dense, highly ionized outflow obscures the central source

We present the first XRISM/Resolve observations of the active galactic nucleus, NGC 1365, obtained in 2024 February and July. NGC 1365 is known for rapid transitions between Compton-thick and Compton-thin states, along with strong absorption from a highly ionized wind. During our observations, the source is found in a persistent...

💬 0 commentsarXiv:2601.00795v1PDF
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Posted in physics.optics · 2026-01-02 · Luca O. Trinchão, Alekhya Ghosh, Arghadeep Pal, Haochen Yan, Toby Bi, Shuangyou Zhang, Nathalia B. Tomazio, Flore K. Kunst, Lewis Hill, Gustavo S. Wiederhecker, Pascal Del'Haye

Color symmetry breaking in a nonlinear optical microcavity

Spontaneous symmetry breaking leads to diverse phenomena across the natural sciences, from the Higgs mechanism in particle physics to superconductors and collective animal behavior. In photonic systems, the symmetry of light states can be broken when two optical fields interact through the Kerr nonlinearity, as shown in early...

💬 0 commentsarXiv:2601.00792v1PDF
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Posted in hep-ph · 2026-01-02 · Ai-Yu Bai, Auttakit Chatrabhuti, Yin-Yuan Huang, Hiroshi Isono, Jian Tang

Dark Dimension Right-handed Neutrinos Confronted with Long-Baseline Oscillation Experiments

Right-handed neutrinos are naturally induced by dark extra dimension models and play an essential role in neutrino oscillations. The model parameters can be examined by the long-baseline neutrino oscillation experiments. In this work, we compute the predicted neutrino oscillation spectra within/without extra dimension models and...

💬 0 commentsarXiv:2601.00790v2PDF
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Posted in astro-ph.EP · 2026-01-02 · Teng Ee Yap, Konstantin Batygin

Callisto's Nonresonant Orbit as an Outcome of Circum-Jovian Disk Substructure

The Galilean moons of Io, Europa, and Ganymede exhibit a 4:2:1 commensurability in their mean motions, a configuration known as the Laplace resonance. The prevailing view for the origin of this three-body resonance involves the convergent migration of the moons, resulting from gas-driven torques in the circum-Jovian disk wherein they...

💬 0 commentsarXiv:2601.00786v1PDF
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Posted in cond-mat.mes-hall · 2026-01-02 · R. Johanna Zijderveld, Adam Yanis Chaou, Isidora Araya Day, Anton R. Akhmerov

Symmetric approximant formalism for statistical topological matter

The standard approach to characterizing topological matter, computing topological invariants, fails when the symmetry protecting the topological phase is preserved only on average in a disordered system. Because topological invariants rely on enforcing the symmetry exactly, they can overcount phases by incorrectly identifying certain...

💬 0 commentsarXiv:2601.00784v1PDF
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Posted in physics.optics · 2026-01-02 · J. Sumaya-Martinez, J. Mulia-Rodriguez

Achieving Extraordinary Acoustic Transmission in a Single Slit by Boundary Impedance Engineering

Extraordinary acoustic transmission is commonly associated with periodic or multi-aperture structures. In this work, we show that a single subwavelength slit can support strongly enhanced transmission when its boundary response is described by an effective impedance. Using a reduced analytical model together with numerical...

💬 0 commentsarXiv:2601.00778v1PDF
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Posted in gr-qc · 2026-01-02 · Juan F. Bravo, Leonardo Castañeda, Héctor J. Hortúa

A 3+1 Perturbative Approach to the Cosmic Dynamo Equation

In this work, we analyze the evolution of PMFs within a perturbed Friedmann-Lemaître-Robertson-Walker (FLRW) spacetime using the formalisms of Numerical Relativity (NR). We apply the 3+1 decomposition to first-order cosmological perturbations to derive the cosmological dynamo equation under the kinematic-dynamo approximation. Our...

💬 0 commentsarXiv:2601.00774v1PDF
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Posted in quant-ph · 2026-01-02 · Dietmar Dorninger, Helmut Länger

On orthoposets of numerical events in quantum logic

Let S be a set of states of a physical system and p(s) the probability of the occurrence of an event when the system is in state s in S. Such a function p from S to [0,1] is known as a numerical event or more accurately an S-probability. A set P of numerical events including the constant functions 0 and 1 and 1-p with every p in P...

💬 0 commentsarXiv:2601.00772v1PDF
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Posted in gr-qc · 2026-01-02 · Aonan Zhang, Qiang Wang, Yong Xiao

Extremalization approach to black hole thermodynamics: perturbations around higher-derivative gravities

When higher-derivative terms are added to a gravitational action, black hole solutions and their thermodynamic properties are generally corrected. Recent progress has shown that, by treating higher-derivative operators as perturbations, the first-order corrections to black hole thermodynamics can be obtained without explicit knowledge...

💬 0 commentsarXiv:2601.00771v2PDF
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Posted in astro-ph.CO · 2026-01-02 · Diego Garza, Brant Robertson, Piero Madau, Nick Gnedin, Matthew W. Abbruzo, Evan Schneider, Reuben D. Budiardja, James B. White, Robert Caddy, Bruno Villasenor

Dynamical Dark Energy Imprints in the Lyman-Alpha Forest

The nature of dark energy (DE) remains elusive, even though it constitutes the dominant energy-density component of the Universe and drives the late-time acceleration of cosmic expansion. By combining measurements of the expansion history from baryon acoustic oscillations, supernova surveys, and cosmic microwave background data, the...

💬 0 commentsarXiv:2601.00767v1PDF
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Posted in astro-ph.IM · 2026-01-01 · Vikram Seenivasan, Srinath Saikrishnan, Andrew Lizarraga, Jonathan Soriano, Bernie Boscoe, Tuan Do

Combining datasets with different ground truths using Low-Rank Adaptation to generalize image-based CNN models for photometric redshift prediction

In this work, we demonstrate how Low-Rank Adaptation (LoRA) can be used to combine different galaxy imaging datasets to improve redshift estimation with CNN models for cosmology. LoRA is an established technique for large language models that adds adapter networks to adjust model weights and biases to efficiently fine-tune large base...

💬 0 commentsarXiv:2601.00146v1PDF
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Posted in cond-mat.mtrl-sci · 2026-01-01 · Shuaiyang Guo, Yuan Wang, Wei Zhang

Machine-learned potential for amorphous Indium-Tin-Oxide alloys

Machine-learned potential-driven molecular dynamics (MLMD) simulations are of great value in guiding the design and optimization of memory devices. Amorphous indium-tin-oxide (ITO) is widely used as transparent conducting oxide for flat-panel display and solar cell applications, and also as a capping layer in...

💬 0 commentsarXiv:2601.00145v1PDF
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Posted in physics.plasm-ph · 2026-01-01 · Mangilal Choudhary, Vanshika, Surya

Transient spark dielectric barrier post-discharge plasma reactor with a liquid electrode for dye degradation: A primary study

The potential application of non-thermal plasma in treating textile industrial wastewater motivates researchers to develop innovative techniques at a laboratory scale to achieve the goal of wastewater mineralization. In line with this objective, a dielectric barrier post-discharge plasma reactor with a liquid electrode has been built...

💬 0 commentsarXiv:2601.00236v1PDF
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Posted in astro-ph.SR · 2026-01-01 · Atila Poro, Ehsan Paki, Fahri Alicavus, Raul Michel

Detailed Investigation of a W UMa Contact Binary with an Ultralow Mass Ratio and a Third-Body as a Potential Merger Candidate

The lower limit of the mass ratio in contact binaries remains uncertain, with observations suggesting systems exist below theoretical predictions. The stability of such very low mass ratio systems is still debated. Based on our review of systems within the mass ratio cutoff range, we reanalyzed TYC 3801-1529-1 and found it to have the...

💬 0 commentsarXiv:2601.00232v2PDF
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Posted in cond-mat.other · 2026-01-01 · Jayaseelan Dhakshinamoorthy, Hitesh Chhabra, Ajaya K Nayak

Deterministic Helicity Locking of Bloch Skyrmions in Centrosymmetric Systems

Magnetic skyrmions in centrosymmetric materials exhibit Bloch-type spin textures with degenerate helicity states due to the absence of Dzyaloshinskii Moriya interaction (DMI), resulting in random nucleation and uncontrolled chirality. Here, we present a comprehensive micromagnetic study demonstrating a fully DMI free strategy for...

💬 0 commentsarXiv:2601.00230v1PDF
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Posted in cond-mat.dis-nn · 2026-01-01 · Bibek Saha, Sthitadhi Roy

Anderson localisation in spatially structured random graphs

We study Anderson localisation on high-dimensional graphs with spatial structure induced by long-ranged but distance-dependent hopping. To this end, we introduce a class of models that interpolate between the short-range Anderson model on a random regular graph and fully connected models with statistically uniform hopping, by...

💬 0 commentsarXiv:2601.00220v2PDF
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Posted in quant-ph · 2026-01-01 · Yecheng Xue, Rui Yang, Zhiding Liang, Tongyang Li

DC-MBQC: A Distributed Compilation Framework for Measurement-Based Quantum Computing

Distributed quantum computing (DQC) is a promising technique for scaling up quantum systems. While significant progress has been made in DQC for quantum circuit models, there exists much less research on DQC for measurement-based quantum computing (MBQC), which is a universal quantum computing model that is essentially different from...

💬 0 commentsarXiv:2601.00214v1PDF
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Posted in cond-mat.mtrl-sci · 2026-01-01 · Paige Harford, Ezekiel Horsley, Subin Kim, Young-June Kim

Sample thickness dependence of structural and magnetic properties in $α$-RuCl$_3$

The layered transition metal trihalide $α$-RuCl$_3$ has been studied extensively in recent years as a promising candidate for a proximate Kitaev quantum spin liquid state. In high quality samples, a complete structural transition from room-temperature C2/m to low-temperature R$\bar{3}$ is consistently observed, with a single magnetic...

💬 0 commentsarXiv:2601.00210v1PDF
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Posted in physics.ao-ph · 2026-01-01 · Johannes Lawen, George Salman, Akshita Bhardwaj

Stratosphere Model Verification with Manufactured Geometry

We propose an exact solution for a stratosphere dynamical core formulated in geopotential/pressure coordinates with a time-evolving lower boundary supplied by the troposphere. Rather than constraining the stratospheric circulation via specified dynamics (``nudging'') to a reanalysis, we treat the tropopause as a moving geometric...

💬 0 commentsarXiv:2601.00206v1PDF