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Physics

arXiv preprints from January 1, 2026 through September 23, 2026 — 12:15:53 EST

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Posted in physics.atom-ph · 2026-01-13 · Kanta Asakawa, Naoki Tanabe, Oki Watanabe, Shuji Kamada, Keisuke Hara, Kaori Niki, Atsushi Hatakeyama

Light-induced spin-polarized desorption of Rb atoms from Co surfaces

The spin polarization of Rb atoms undergoing light-induced desorption from a spin-polarized Co (110) surface was investigated. Desorption induced by pulsed UV-light irradiation was driven by a non-thermal mechanism and the spins of the desorbed Rb atoms were polarized. This implies spin transfer between the surface and the adsorbate...

💬 0 commentsarXiv:2601.08442v2PDF
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Posted in nucl-th · 2026-01-13 · X. F. Jiang, Z. Z. Li, X. W. Sun, J. Meng

Dipole response in deformed halo nuclei $^{42}\mathrm{Mg}$ and $^{44}\mathrm{Mg}$

The quasiparticle finite amplitude method based on the deformed relativistic Hartree-Bogoliubov theory in continuum has been developed for the noncharge-exchange multipole response. Taking neutron-rich magnesium isotopes as examples, the isovector electric dipole response, especially in the low-lying region, is studied. It is found...

💬 0 commentsarXiv:2601.08438v2PDF
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Posted in physics.optics · 2026-01-13 · Yazhou Wang, Marcello Meneghetti, Manoj K. Dasa, Timothy Bate, J. E. Antonio-Lopez, Ian A. Davidson, Qiang Fu, Jaroslaw Rzegocki, Gregory T. Jasion, Francesco Poletti, Rodrigo Amezcua-Correa, Christos Markos

Tunable, high pulse energy and narrow linewidth gas-filled fiber laser across near- and mid-infrared

Wavelength widely tunable infrared fiber lasers that simultaneously deliver high pulse energies with narrow linewidths are critical for applications ranging from spectroscopy to nonlinear optics, yet achieving this combination has remained a long-standing challenge. Here, we demonstrate that gas-filled anti-resonant hollow-core fiber...

💬 0 commentsarXiv:2601.08433v1PDF
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Posted in astro-ph.GA · 2026-01-13 · Kai Wang, Peder Norberg, Azadeh Fattahi, Louis E. Strigari

Local Group analogues in a cosmological context -- I. Relating velocity structure to the cosmic web

Our Local Group, dominated in mass by the Milky Way (MW) and M31, provides a unique laboratory for testing $Λ$CDM cosmology on small scales owing to its proximity. However, its connection to the surrounding large-scale environment, which is essential for interpreting its properties, is inadequately understood. In this work, we explore...

💬 0 commentsarXiv:2601.08419v1PDF
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Posted in quant-ph · 2026-01-13 · Guillermo Currás-Lorenzo, Margarida Pereira, Kiyoshi Tamaki, Marcos Curty

Rigorous phase-error-estimation security framework for QKD with correlated sources

Practical QKD modulators introduce correlations between consecutively emitted pulses due to bandwidth limitations, violating key assumptions underlying many security proof techniques. Here, we address this problem by introducing a simple yet powerful mathematical framework to directly extend phase-error-estimation-based security...

💬 0 commentsarXiv:2601.08417v1PDF
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Posted in physics.acc-ph · 2026-01-13 · Hanxiang Yang, Zhangfeng Gao, Bingyang Yan, Wencai Cheng, Nanshun Huang, Haixiao Deng

High-power beyond extreme ultraviolet FEL radiation with flexible polarization at SHINE

Linac-based free-electron lasers (FELs) feature high brightness, narrow bandwidth, controllable polarization, and wide wavelength tunability. With the rapid development of superconducting radio-frequency technology, linacs can now operate at MHz-level repetition rates, enabling FELs with both high repetition rates and high average...

💬 0 commentsarXiv:2601.08413v2PDF
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Posted in cond-mat.mtrl-sci · 2026-01-13 · V. N. Jmerik, D. V. Nechaev, E. A. Evropeitsev, E. M. Roginskii, A. N. Semenov, M. A. Yagovkina, P. A. Alekseev, V. I. Kozlovsky, M. M. Zverev, N. A. Gamov, Tao Wang, Xinqiang Wang, T. V. Shubina, A. A. Toropov

Fractional-Monolayer 2D-GaN/AlN Structures: Growth Kinetics and UVC-emitter Applications

The paper reports on fundamental properties of the GaN/AlN quantum wells (QWs) with nominal subcritical thicknesses of 0.75-2 monolayers (MLs). They are grown by plasma-activated molecular beam epitaxy, varying either the nominal thickness or the gallium-to-nitrogen flux ratio. In situ monitoring reveals difference in 2D nucleation...

💬 0 commentsarXiv:2601.08410v3PDF
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Posted in physics.soc-ph · 2026-01-13 · Quantum Scientists for Disarmament

Quantum scientists for disarmament: a manifesto

We, as researchers in quantum science and technology, are publishing this manifesto to express our deep concerns about the current geopolitical situation and the global race to rearm. We firmly oppose all forms of militarization in our societies and, in particular, within the academic world. We categorically reject the use of our...

💬 0 commentsarXiv:2601.14282v1PDF
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Posted in astro-ph.IM · 2026-01-13 · M. Tsantaki, K. Biazzo, F. Zahra Majidi, G. Tautvaisiene, I. Busa

Planet-Host Stars Across the Galaxy in the 2040s

By the 2040s, the exoplanet field will have moved from the discovery of a few thousand planets to hundreds of thousands, thanks to Gaia DR5, TESS, PLATO, Roman, and their successors. At that stage, the key bottleneck will no longer be planet detection, but our ability to understand how planetary systems form, evolve, and diversify...

💬 0 commentsarXiv:2601.08890v1PDF
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Posted in physics.plasm-ph · 2026-01-13 · Eduardo Rodriguez, Gabriel G. Plunk

Near-axis quasi-isodynamic database

In this work, we investigate the landscape of quasi-isodynamic stellarators using the near-axis expansion of the magnetic field. Building on recent theoretical developments, we construct a database of more than 800,000 stable, approximately quasi-isodynamic vacuum magnetic configurations. These configurations span a range of field...

💬 0 commentsarXiv:2601.08400v3PDF
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Posted in astro-ph.IM · 2026-01-13 · Aurélie Magniez, Charlotte Z. Bond, Peter Wizinowich, TIm Morris, Kieran O'Brien

Polychromatic pyramid wavefront sensor with MKID technology for high contrast imaging

The high sensitivity of the pyramid wavefront sensor has made it the preferred sensor in high contrast adaptive optics systems. Future higher contrast systems, like the Extremely Large Telescope's Planetary Camera System, will require higher performance wavefront sensing. A further performance improvement could be achieved with a...

💬 0 commentsarXiv:2601.08398v1PDF
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Posted in astro-ph.EP · 2026-01-13 · Shohei Aoki, Yuka Fujii, Hideo Sagawa, Geronimo L. Villanueva, Ian Thomas, Bojan Ristic, Frank Daerden, Miguel Angel López-Valverde, Manish R. Patel, Jonathon Mason, Yannick Willame, Giancarlo Bellucci, Ann Carine Vandaele

Anatomy of Empirical Transit Spectra of Mars based on TGO/NOMAD

Transit spectroscopy is a powerful tool for probing atmospheric structures of exoplanets. Accurately accounting for the effects of aerosols is key to reconstructing atmospheric properties from transit spectra, yet this remains a significant challenge. To advance this effort, it is invaluable to examine the spectral features of...

💬 0 commentsarXiv:2601.08397v1PDF
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Posted in quant-ph · 2026-01-13 · Mir Alimuddin, Jaemin Kim, Antonio Acín, Leonardo Zambrano

Entanglement-swapping measurements for deterministic entanglement distribution

Entanglement swapping is a key primitive for distributing entanglement across nodes in quantum networks. In standard protocols, the outcome of the intermediate measurement determines the resulting state, making the process inherently probabilistic and requiring postselection. In this work, we fully characterize those measurements...

💬 0 commentsarXiv:2601.08581v1PDF
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Posted in physics.bio-ph · 2026-01-13 · Sebastian Westrich, Nimba Oshnik, Nina Thiele, Nina Burmeister, Yanis Abdedou, Nikhita Khera, Stefanie J. Müller-Schüssele, Elke Neu

FRET between NV centers in diamond and chlorophyll molecules: a novel resource for multimodal sensing and imaging in plant cells

This work demonstrates efficient Forster resonance energy transfer (FRET) between ensembles of shallow nitrogen-vacancy (NV) centers located 7 nm and 9 nm below a single-crystal diamond surface and a naturally occurring fluorophore, namely a mixture of chlorophyll a and b molecules extracted from Arabidopsis thaliana. The broad...

💬 0 commentsarXiv:2601.08580v1PDF
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Posted in quant-ph · 2026-01-13 · Xiaotong Wang, Shunlong Luo, Yue Zhang

Phase-sensitive superposition of quantum states

Although the principle of superposition lies at the heart of quantum mechanics and is the root of almost all quantum phenomena such as coherence and entanglement, its quantification, except for that related to the resource theory of coherence and interference, remains relatively less studied. In this work, we address quantification of...

💬 0 commentsarXiv:2601.08579v1PDF
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Posted in quant-ph · 2026-01-13 · Marvin Erdmann, Lukas Karch, Abhishek Awasthi, Caitlin Isobel Jones, Pallavi Bhardwaj, Florian Krellner, Jonas Stein, Claudia Linnhoff-Popien, Nico Kraus, Peter Eder, Sarah Braun, Tong Liu

Quantum Computing -- Strategic Recommendations for the Industry

This whitepaper surveys the current landscape and short- to mid-term prospects for quantum-enabled optimization and machine learning use cases in industrial settings. Grounded in the QCHALLenge program, it synthesizes hardware trajectories from different quantum architectures and providers, and assesses their maturity and potential...

💬 0 commentsarXiv:2601.08578v1PDF
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Posted in physics.bio-ph · 2026-01-13 · Tatsuaki Tsuruyama

Information-Thermodynamic Analysis of the DNA--RNA Polymerase Complex via Interface Dissipation: Based on Observer--Observed Swap Symmetry

RNA polymerase (RNAP) elongates RNA by walking along a DNA template and selectively incorporating ribonucleoside triphosphates (rNTPs). Rather than mechanically replicating the base sequence, RNAP conditions binding and chemistry on the currently read template nucleotide, converting sequence dependence into a bias in its stochastic...

💬 0 commentsarXiv:2601.08577v2PDF
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Posted in physics.optics · 2026-01-13 · Suman Mandal, Apuroop Vaidyam, Nishkarsh Kumar, Sujit Rajak, Shyamal Guchhait, Nirmalya Ghosh

Geometry Driven Spin Polarization Effects in Waveguiding Plasmonic Crystal

We investigated the modulation in the polarization-dependent optical behaviour of the waveguiding plasmonic crystal by varying the illumination and detection geometry. We employed the finite element method-based COMSOL simulation and Jones-Mueller formalisms to probe the variations in optical parameters by systematically varying the...

💬 0 commentsarXiv:2601.08572v1PDF
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Posted in physics.flu-dyn · 2026-01-13 · Manuel Noseda, Bernardo Luciano Español, Pablo Daniel Mininni, Pablo Javier Cobelli

Chirality tomography: measuring local helicity from trajectory linking

We present the first three-dimensional helicity maps of fully developed turbulence obtained through chirality tomography, a Lagrangian voxel-based method that reconstructs helicity density from particle trajectories. Our approach builds on an empirically established relation between helicity and trajectory linking, converting local...

💬 0 commentsarXiv:2601.08569v1PDF
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Posted in quant-ph · 2026-01-13 · K. Sai Mineesh Reddy, Navin Kashyap

Asymptotically good CSS codes that realize the logical transversal Clifford group fault-tolerantly

This paper introduces a framework for constructing Calderbank-Shor-Steane (CSS) codes that support fault-tolerant logical transversal $Z$-rotations. Using this framework, we obtain asymptotically good CSS codes that fault-tolerantly realize the logical transversal Clifford group (i.e., transversal single-qubit Clifford gates are...

💬 0 commentsarXiv:2601.08568v2PDF
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Posted in hep-ph · 2026-01-13 · Jun Jiang, Cong-Feng Qiao, Yu-Han Zhao

Where to find $X(17)$?

The Atomki anomaly puts forward the hypothesis of an $X(17)$ particle to explain its observation. Utilizing experimental results from the Atomki experiments, measurements of the electron's anomalous magnetic moment, beam dump experiments, the KLOE-2 experiment, the PADME experiment, and the parity-violating Møller scattering...

💬 0 commentsarXiv:2601.08567v5PDF
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Posted in astro-ph.GA · 2026-01-13 · Qian Wang, Aigen Li, Xuejuan Yang

On the Interstellar Extinction Curve toward HD 93222, A Sightline with an Exceedingly Narrow 2175 Angstrom Extinction Bump

The 2175 Angstrom extinction bump, the most prominent spectral feature superimposed on the interstellar extinction curve, is widely seen in the interstellar medium (ISM) of the Milky Way and external galaxies, both near and far. While its central wavelength is remarkably stable and independent with environment, its width shows...

💬 0 commentsarXiv:2601.08563v1PDF
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Posted in quant-ph · 2026-01-13 · Jhordan Santiago, Petr Steindl

Nonclassicality of multi-photon-added cat states

Multi-photon-added cat states are constructed by repeatedly applying the creation operator to a cat state. We study in detail their photon-number distribution, $Q$ parameter, squeezing properties, and Wigner function. We show that photon addition induces a $π$ phase shift in the original parity configuration whenever an odd number of...

💬 0 commentsarXiv:2601.08894v1PDF
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Posted in physics.chem-ph · 2026-01-13 · Luis Bonah, Marie-Aline Martin-Drumel, Olivier Pirali, Francesca Tonolo, Michela Nonne, Mattia Melosso, Luca Bizzocchi, Cristina Puzzarini, Jean-Claude Guillemin, Christian P. Endres, Stephan Schlemmer, Sven Thorwirth

High-Resolution Infrared Spectroscopy and ASAP Analysis of Cyclopentadiene: The Vibrational Modes below 860 cm$^{-1}$ and the $ν_{21}$ Mode at 961 cm$^{-1}$

The spectroscopic fingerprints of vibrationally excited states of astronomical molecules are interesting for multiple reasons. They are excellent temperature probes of the corresponding astronomical regions and are thought to be the origin of many unknown lines in astronomical survey spectra. Rovibrational spectra provide accurate...

💬 0 commentsarXiv:2601.08560v1PDF
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Posted in astro-ph.SR · 2026-01-13 · A. R. G. do Brito do Vale, K. Mužić, H. Bouy, V. Almendros-Abad, A. Bayo, D. Capela, A. Scholz, A. Bik, G. Suárez, L. Cieza, K. Peña Ramírez, E. Bertin, R. Schödel

Substellar population of the young massive cluster RCW 36 in Vela

The initial mass function (IMF) is a cornerstone of star formation studies, yet its universality remains debated. We investigate the IMF in the young massive cluster RCW 36, located in the Vela Molecular Ridge and comparable to the Orion Nebula Cluster in stellar density. Our goal is to build the most complete census of RCW 36 and...

💬 0 commentsarXiv:2601.08555v1PDF