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Physics

arXiv preprints from January 1, 2026 through September 6, 2026 — 06:18:30 EST

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Posted in astro-ph.GA · 2026-01-21 · Itzhak Goldman

Small scale turbulence alongside with large scale turbulence in a z~sim 2 star Forming Galaxy with outflowing wind, revealed by Multi-point structure functions

Recently, Goldman (2024) obtained evidence for a large scale compressible, Burgers turbulence in the ism of a gravitationally lensed, star-forming galaxy at $z = 1.87$, with an outflowing wind. The turbulent timescale on the largest spatial scale has been found to be ~500 Myr . This together with the large spatial scale of~ 6.4 kpc...

💬 0 commentsarXiv:2601.14887v1PDF
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Posted in physics.plasm-ph · 2026-01-21 · V. Fernández-Pacheco, J. L. Velasco, E. Sánchez, R. Gaur, J. M. García-Regaña, J. A. Alonso, I. Calvo, D. Carralero

Piecewise omnigenous magnetohydrodynamic equilibria as fusion reactor candidates

In piecewise omnigenous magnetic fields, charged particles remain perfectly confined in the abscence of collisions and turbulence. This concept extends the traditional notion of omnigenity, the theoretical principle upon which most of existing magnetic fusion reactor designs, including tokamaks, are based. While piecewise omnigenity...

💬 0 commentsarXiv:2601.14886v2PDF
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Posted in cond-mat.mtrl-sci · 2026-01-21 · Volodymyr Vasylkovskyi, Olga Trukhina, Patrick Dörflinger, Mykola Slipchenko, Wolf Gero Schmidt, Timur Biktagirov, Anastasiia Kultaeva, Yakov Kopelevich, Vladimir Dyakonov

Role of Defects in the Paramagnetism of Fe-doped Cs$_{2}$AgBiBr$_{6}$ Double Perovskite

Transition-metal doping enables the introduction of spin functionality into halide double perovskites, while simultaneously modifying optical properties. Here, we combine controlled single-crystal growth, optical characterization, comprehensive electron paramagnetic resonance (EPR) spectroscopy, and first-principles modeling to...

💬 0 commentsarXiv:2601.14885v1PDF
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Posted in nucl-ex · 2026-01-21 · STAR Collaboration, B. E. Aboona, J. Adam, G. Agakishiev, I. Aggarwal, M. M. Aggarwal, Z. Ahammed, A. Aitbayev, I. Alekseev, E. Alpatov, A. K. Alshammri, A. Aparin, S. Aslam, J. Atchison, G. S. Averichev, V. Bairathi, X. Bao, P. Barik, K. Barish, S. Behera, P. Bhagat, A. Bhasin, S. Bhatta, I. G. Bordyuzhin, J. D. Brandenburg, A. V. Brandin, C. Broodo, X. Z. Cai, H. Caines, M. Calderón~de~la~Barca~Sánchez, D. Cebra, J. Ceska, I. Chakaberia, Y. S. Chang, Z. Chang, A. Chatterjee, D. Chen, J. H. Chen, L. Chen, Q. Chen, W. Chen, Z. Chen, J. Cheng, Y. Cheng, W. Christie, X. Chu, S. Corey, H. J. Crawford, G. Dale-Gau, A. Das, D. De Souza Lemos, T. G. Dedovich, I. M. Deppner, A. A. Derevschikov, A. Deshpande, A. Dhamija, A. Dimri, P. Dixit, X. Dong, J. L. Drachenberg, E. Duckworth, J. C. Dunlop, Y. S. El-Feky, J. Engelage, G. Eppley, S. Esumi, O. Evdokimov, O. Eyser, B. Fan, Y. Fang, R. Fatemi, S. Fazio, H. Feng, Y. Feng, E. Finch, Y. Fisyak, F. A. Flor, B. Fu, C. Fu, T. Fu, T. Gao, Y. Gao, G. Garcia, F. Geurts, A. Gibson, A. Giri, K. Gopal, X. Gou, D. Grosnick, A. Gu, J. Gu, A. Gupta, A. Hamed, R. J. Hamilton, J. Han, X. Han, M. D. Harasty, J. W. Harris, H. Harrison-Smith, L. B. Havener, X. H. He, Y. He, C. Hu, Q. Hu, Y. Hu, H. Huang, H. Z. Huang, S. L. Huang, T. Huang, Y. Huang, Y. Huang, Y. Huang, M. Isshiki, W. W. Jacobs, A. Jalotra, C. Jena, Y. Ji, J. Jia, X. Jiang, C. Jin, Y. Jin, N. Jindal, X. Ju, E. G. Judd, S. Kabana, D. Kalinkin, J. Kang, K. Kang, A. R. Kanuganti, D. Kapukchyan, K. Kauder, D. Keane, A. Kechechyan, M. Kesler, A. Khanal, A. Khanal, J. Kim, A. Kiselev, A. G. Knospe, L. Kochenda, Y. Kong, A. A. Korobitsin, B. Korodi, A. Yu. Kraeva, P. Kravtsov, L. Kumar, M. C. Labonte, R. Lacey, J. M. Landgraf, C. Larson, A. Lebedev, R. Lednicky, J. H. Lee, Y. H. Leung, C. Li, D. Li, H-S. Li, H. Li, H. Li, H. Li, W. Li, X. Li, X. Li, Y. Li, Z. Li, Z. Li, X. Liang, T. Lin, Y. Lin, C. Liu, G. Liu, H. Liu, L. Liu, L. Liu, Z. Liu, Z. Liu, T. Ljubicic, O. Lomicky, E. M. Loyd, T. Lu, J. Luo, X. F. Luo, V. B. Luong, L. Ma, R. Ma, Y. G. Ma, N. Magdy, R. Manikandhan, O. Matonoha, K. Menduli, K. Mi, N. G. Minaev, B. Mohanty, B. Mondal, M. M. Mondal, I. Mooney, D. A. Morozov, M. I. Nagy, C. J. Naim, A. S. Nain, J. D. Nam, M. Nasim, H. Nasrulloh, E. Nedorezov, J. M. Nelson, M. Nie, G. Nigmatkulov, T. Niida, L. V. Nogach, T. Nonaka, G. Odyniec, A. Ogawa, S. Oh, V. A. Okorokov, K. Okubo, B. S. Page, M. Pal, S. Pal, A. Pandav, A. Panday, A. K. Pandey, Y. Panebratsev, T. Pani, P. Parfenov, A. Paul, S. Paul, C. Perkins, S. Ping, I. D. Ponce Pinto, M. Posik, E. Pottebaum, A. Povarov, S. Prodhan, T. L. Protzman, N. K. Pruthi, J. Putschke, Y. Qi, Z. Qin, H. Qiu, C. Racz, S. K. Radhakrishnan, A. Rana, R. L. Ray, C. W. Robertson, O. V. Rogachevsky, M. A. Rosales Aguilar, D. Roy, L. Ruan, A. K. Sahoo, N. R. Sahoo, H. Sako, S. Salur, S. S. Sambyal, E. Samigullin, D. T. Samuel, J. K. Sandhu, S. Sato, B. C. Schaefer, N. Schmitz, J. Seger, R. Seto, P. Seyboth, N. Shah, E. Shahaliev, P. V. Shanmuganathan, T. Shao, M. Sharma, N. Sharma, R. Sharma, S. R. Sharma, A. I. Sheikh, D. Shen, D. Y. Shen, K. Shen, S. Shi, Y. Shi, Shilpa, E. Shulga, F. Si, J. Singh, S. Singha, P. Sinha, M. J. Skoby, Y. Söhngen, Y. Song, T. D. S. Stanislaus, M. Strikhanov, Y. Su, X. Sun, Y. Sun, B. Surrow, D. N. Svirida, Z. W. Sweger, A. C. Tamis, A. H. Tang, Z. Tang, A. Taranenko, T. Tarnowsky, J. H. Thomas, A. Timofeev, D. Tlusty, M. V. Tokarev, D. Torres-Valladares, S. Trentalange, O. D. Tsai, C. Y. Tsang, Z. Tu, J. E. Tyler, T. Ullrich, D. G. Underwood, G. Van Buren, A. N. Vasiliev, F. Videbæk, S. Vokal, S. A. Voloshin, F. Wang, G. Wang, G. Wang, J. S. Wang, J. Wang, K. Wang, X. Wang, Y. Wang, Y. Wang, Y. Wang, Z. Wang, Z. Wang, Z. Wang, J. C. Webb, P. C. Weidenkaff, G. D. Westfall, H. Wieman, G. Wilks, S. W. Wissink, C. P. Wong, J. Wu, X. Wu, X. Wu, X. Wu, B. Xi, Y. Xiao, Z. G. Xiao, G. Xie, W. Xie, H. Xu, N. Xu, Q. H. Xu, X. Xu, Y. Xu, Y. Xu, Y. Xu, Y. Xu, Z. Xu, Z. Xu, G. Yan, Z. Yan, C. Yang, Q. Yang, S. Yang, Y. Yang, Z. Ye, Z. Ye, L. Yi, Y. Yu, W. Yuan, W. Zha, C. Zhang, D. Zhang, J. Zhang, K. Zhang, L. Zhang, S. Zhang, W. Zhang, X. Zhang, Y. Zhang, Y. Zhang, Y. Zhang, Y. Zhang, Z. Zhang, Z. Zhang, F. Zhao, J. Zhao, S. Zhou, Y. Zhou, C. Zhu, X. Zhu, M. Zurek, M. Zyzak

Probing Late-Stage Hadronic Interactions at High Baryon Density via $K^{*0}$ Production in the RHIC Beam Energy Scan Program

A precision measurement of the $K^{*0}$ meson yield is reported in Au+Au collisions at $\sqrt{s_{NN}} = 7.7,\; 11.5,\; 14.6,\; 19.6,$ and $27~\mathrm{GeV}$ using the high-statistics data sample collected by the STAR experiment during the Beam Energy Scan II (BES-II) program at RHIC. The transeverse momentum ($p_{T}$)-integrated yield...

💬 0 commentsarXiv:2601.14884v2PDF
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Posted in cond-mat.str-el · 2026-01-21 · V. P. Mineev

Altermagnets versus Antiferromagnets

Altermagnets are metals with a momentum-dependent spin splitting of electron bands due to a specific crystal structure that is invariant under time reversal only in combination with rotations and reflections, or lacks time reversal altogether. The developed phenomenological approach allows one to obtain a spectrum of electron bands in...

💬 0 commentsarXiv:2601.14878v3PDF
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Posted in astro-ph.EP · 2026-01-21 · Miguel J. S. Martinho, Hamed Valizadegan, Jon M. Jenkins, Douglas A. Caldwell, Joseph D. Twicken, Ben Tofflemire, Marziye Jafariyazani

ExoMiner++ 2.0: Vetting TESS Full-Frame Image Transit Signals

The Transiting Exoplanet Survey Satellite (TESS) Full-Frame Images (FFIs) provide photometric time series for millions of stars, enabling transit searches beyond the limited set of pre-selected 2-minute targets. However, FFIs present additional challenges for transit identification and vetting. In this work, we apply ExoMiner++ 2.0,...

💬 0 commentsarXiv:2601.14877v2PDF
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Posted in quant-ph · 2026-01-21 · Antonin Grateau, Alexander Boeschoten, Tanguy Favin-Lévêque, Isael Herrera, Nicolas Treps

Multiparameter estimation for the superresolution of two incoherent sources

We experimentally demonstrate the simultaneous estimation of the three parameters characterizing a pair of incoherent optical sources in the sub-Rayleigh regime, enabling super-resolved scene characterization. Using spatial-mode demultiplexing (SPADE) with two demultiplexers--one deliberately shifted--we determine separations well...

💬 0 commentsarXiv:2601.14876v2PDF
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Posted in hep-ph · 2026-01-21 · Piotr Lebiedowicz, Otto Nachtmann, Antoni Szczurek

Central exclusive production of $η$ and $η'$ mesons in diffractive proton-proton collisions at the LHC and the nature of the pomeron

Central exclusive production (CEP) of $η$ and $η'$ mesons in proton-proton collisions at high-energies is discussed. At the LHC the main mechanism for the production of these mesons should be double-pomeron ($\rm I\!P$-$\rm I\!P$) exchange, that is, the fusion reactions ${\rm I\!P I\!P} \to η, η'$. We show that for a scalar pomeron...

💬 0 commentsarXiv:2601.14870v2PDF
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Posted in quant-ph · 2026-01-21 · Qing-Yang Qiu, Wen Huang, Lei Du, Xin-You Lü

Exotic collective behaviors of giant quantum emitters in two-dimensional baths

Nonlocal light-matter interactions with giant atoms in high-dimensional environments are not only fundamentally intriguing for testing quantum electrodynamics beyond the dipole approximation but also crucial for building high-dimensional quantum networks and engineering multipartite entangled states. Given the enigmatic and largely...

💬 0 commentsarXiv:2601.14867v1PDF
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Posted in astro-ph.CO · 2026-01-21 · J. Mena-Fernández, S. Avila, A. Porredon, H. Camacho, J. Muir, E. Sanchez, M. Adamow, K. Bechtol, R. Camilleri, G. Campailla, T. M. Davis, N. Deiosso, C. Doux, A. Drlica-Wagner, A. Ferté, R. A. Gruendl, W. G. Hartley, A. Pieres, M. Raveri, E. S. Rykoff, I. Sevilla-Noarbe, P. Shah, E. Sheldon, M. Vincenzi, B. Yanny, T. M. C. Abbott, M. Aguena, S. Allam, O. Alves, F. Andrade-Oliveira, J. Annis, D. Bacon, J. Blazek, S. Bocquet, D. Brooks, A. Carnero Rosell, J. Carretero, F. J. Castander, R. Cawthon, L. N. da Costa, M. E. da Silva Pereira, J. De Vicente, S. Desai, H. T. Diehl, B. Flaugher, J. Frieman, J. García-Bellido, M. Gatti, D. Gruen, G. Gutierrez, K. Herner, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. Huterer, N. Jeffrey, K. Kuehn, O. Lahav, S. Lee, J. L. Marshall, F. Menanteau, R. Miquel, J. J. Mohr, J. Myles, R. L. C. Ogando, A. Palmese, W. J. Percival, A. A. Plazas Malagón, M. Rodriguez-Monroy, A. Roodman, S. Samuroff, D. Sanchez Cid, B. O. Sánchez, T. Shin, M. Smith, M. Soares-Santos, E. Suchyta, M. E. C. Swanson, D. L. Tucker, V. Vikram, A. R. Walker, N. Weaverdyck, M. Yamamoto

Dark Energy Survey: DESI-Independent Angular BAO Measurement

We present a measurement of the angular baryon acoustic oscillation (BAO) scale from the completed Dark Energy Survey (DES) dataset excluding the area of overlap with the Dark Energy Spectroscopic Instrument (DESI). We follow the same methodology and validation process as in the DES year 6 (Y6) BAO analysis. We interpret the impact of...

💬 0 commentsarXiv:2601.14864v2PDF
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Posted in astro-ph.CO · 2026-01-21 · Mohit Raj Sah, Suvodip Mukherjee

The First Upper Bound on the Nano-Hertz Gravitational Waves and Galaxy Cross-Correlation signal using 15-year NANOGrav Data and DESI Galaxy Survey

The recent detection of a common-spectrum stochastic signal by multiple pulsar timing array (PTA) collaborations has provided tentative evidence for a nanohertz (nHz) stochastic gravitational-wave background (SGWB). This signal can be widely interpreted as originating from a cosmic population of inspiraling supermassive black hole...

💬 0 commentsarXiv:2601.14863v1PDF
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Posted in astro-ph.HE · 2026-01-21 · Kostas Kourmpetis, Shafqat Riaz, Honghui Liu, Temurbek Mirzaev, Cosimo Bambi, Debtroy Das, Jiachen Jiang, Kostas D. Kokkotas, Andrea Santangelo

Modeling X-ray reflection spectra from returning radiation: application to 4U 1630$-$47

Returning radiation is thought to play a key role in disk illumination of black hole X-ray binaries in the high-soft state, yet it has not been fully incorporated into XSPEC reflection models. We present a new table model for reflection spectroscopy that, for the first time, self-consistently accounts for the returning radiation. To...

💬 0 commentsarXiv:2601.14860v1PDF
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Posted in astro-ph.CO · 2026-01-21 · D. Sanchez-Cid, A. Ferté, J. Blazek, S. Samuroff, A. Amon, F. Andrade-Oliveira, J. M. Coloma-Nadal, J. Muir, A. Porredon, J. Prat, N. Weaverdyck, M. Yamamoto, D. Anbajagane, M. R. Becker, P. Carrilho, C. Chang, M. Crocce, G. Giannini, W. d'Assignies, J. DeRose, S. Dodelson, E. Krause, E. Legnani, J. Mena-Fernández, N. MacCrann, A. Pourtsidou, C. Preston, P. Rogozenski, M. Rodriguez-Monroy, R. Rosenfeld, E. Sanchez, I. Sevilla-Noarbe, M. Soares-Santos, C. To, M. A. Troxel, M. Tsedrik, B. Yin, J. Zuntz, T. M. C. Abbott, M. Aguena, S. Allam, O. Alves, S. Avila, D. Bacon, K. Bechtol, E. Bertin, S. Bocquet, D. Brooks, H. Camacho, R. Camilleri, A. Campos, A. Carnero Rosell, J. Carretero, F. J. Castander, R. Cawthon, A. Choi, L. N. da Costa, M. E. da Silva Pereira, T. M. Davis, J. De Vicente, S. Desai, C. Doux, A. Drlica-Wagner, T. Eifler, J. Elvin-Poole, S. Everett, A. E. Evrard, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, M. Gatti, E. Gaztanaga, P. Giles, K. Glazebrook, D. Gruen, G. Gutierrez, I. Harrison, K. Herner, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. Huterer, B. Jain, D. J. James, N. Jeffrey, T. Kacprzak, K. Kuehn, O. Lahav, S. Lee, J. L. Marshall, F. Menanteau, R. Miquel, J. J. Mohr, J. Myles, R. C. Nichol, R. L. C. Ogando, A. Palmese, M. Paterno, W. J. Percival, A. A. Plazas Malagón, M. Raveri, A. Roodman, C. Sánchez, T. Schutt, E. Sheldon, N. Sherman, T. Shin, M. Smith, E. Suchyta, M. E. C. Swanson, M. Tabbutt, G. Tarle, D. Thomas, D. L. Tucker, V. Vikram, A. R. Walker, B. Yanny

Dark Energy Survey Year 6 Results: Weak Lensing and Galaxy Clustering Cosmological Analysis Framework

We present the methodology for the weak lensing and galaxy clustering analyses of the Dark Energy Survey (DES) Year 6 data set. In this work, we design and validate the analysis pipeline for the cosmic shear, galaxy clustering plus galaxy$-$galaxy lensing ($2 \times 2$pt), and the joint analysis in the $3 \times 2$pt. Our framework...

💬 0 commentsarXiv:2601.14859v1PDF
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Posted in physics.optics · 2026-01-21 · Anna Suzuki, Pavel Loiko, Weichao Yao, Parisa Baghery, Martin Hoffmann, Kirill Eremeev, Patrice Camy, Alain Braud, Sergei Tomilov, Yicheng Wang, Clara J. Saraceno

Ho3+-doped CALGO crystals for high-power ultrafast 2.1-μm lasers

Ho3+-doped disordered CaAlGdO4 (CALGO) crystals have recently emerged as a promising gain material platform for next-generation high-power ultrafast 2.1-μm laser systems. This laser gain material offers a unique combination of high-gain, small quantum defect, inhomogeneously broadened spectra, and good thermal conductivity, enabling...

💬 0 commentsarXiv:2601.14854v1PDF
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Posted in hep-ph · 2026-01-21 · João Paulo Pinheiro

Testing the three massive neutrino paradigm: Constraints on Neutrino Properties and Interactions from Recent Experimental Data

Neutrino physics offers unique insights into phenomena beyond the Standard Model (BSM). This thesis presents phenomenological investigations organized around three pillars: consolidation of the three-flavor oscillation paradigm, exploration of new physics viability, and precise determination of solar neutrino fluxes. The theoretical...

💬 0 commentsarXiv:2601.14851v2PDF
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Posted in cond-mat.mtrl-sci · 2026-01-21 · Lingyao Zhang, Musen Li, Nisha Metha, Carla Verdi, Wei Ren, Jeffrey R. Reimers

Significance of the dispersion force for ferroelectric switching in ZnO and related materials

Wurtzite-ZnO is a wide-bandgap polar material with a ferroelectric-switching barrier that is too high to utilize, but the barrier can be reduced and switching observed in substituted materials such as Zn0.5Mg0.5O. Here, we seek to understand atomic-scale features that control concerted polarization switching in these and related...

💬 0 commentsarXiv:2601.14847v1PDF
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Posted in quant-ph · 2026-01-21 · Kenny Campbell, Ahmed Lawey, Mohsen Razavi

Combatting noise in near-term quantum data centres

We analyse the performance of different error handling methods in the quantum data centre paradigm of distributed quantum computing. We compare the impact of quantum error detection, using the three-qubit repetition code and the [[4, 1, 2]] Leung-Nielsen-Chuang-Yamamoto code, on remote gates with that of conventional entanglement...

💬 0 commentsarXiv:2601.14845v1PDF
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Posted in cond-mat.mtrl-sci · 2026-01-21 · Ata Utku Özkan, Talip Serkan Kasırga, Aykut Erbaş

Ionic transport in spontaneously ion-intercalated van der Waals layered structures

Understanding ionic transport under strong confinement is crucial for the design of next-generation energy, catalytic, and information-processing materials; however, repeated field-driven ion motion often degrades conventional solid electrolytes. Van der Waals layered materials offer an alternative by providing structurally resilient...

💬 0 commentsarXiv:2601.14836v1PDF
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Posted in physics.plasm-ph · 2026-01-21 · Shaojie Wang

Electric field induced by radial redistribution of the energetic ion pressure in a fusion plasma

It is found by using the gyrokinetic theory that significant radial electric fields, or zonal flows, can be generated by the radial redistribution of energetic ion pressure in a tokamak fusion device. Trapped energetic ions are more effective to generate the radial electric field than the isotropic energetic ions. This suggests that...

💬 0 commentsarXiv:2601.14834v1PDF
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Posted in astro-ph.CO · 2026-01-21 · E. Legnani, J. Elvin-Poole, D. Anbajagane, D. Sanchez Cid, A. Ferté, N. Weaverdyck, A. Porredon, S. Avila, R. Miquel, J. De Vicente, J. Coloma, S. Samuroff, W. d'Assignies, A. Alarcon, C. Sánchez, J. Muir, J. Prat, N. MacCrann, D. Bacon, M. A. Troxel, C. Chang, M. Crocce, M. R. Becker, J. Blazek, M. Yamamoto, T. Schutt, M. Rodriguez-Monroy, G. Giannini, B. Yin, A. Amon, K. Bechtol, I. Sevilla-Noarbe, T. M. C. Abbott, M. Aguena, S. Allam, O. Alves, F. Andrade-Oliveira, G. M. Bernstein, S. Bocquet, D. Brooks, R. Camilleri, A. Carnero Rosell, J. Carretero, L. N. da Costa, M. E. da Silva Pereira, T. M. Davis, S. Desai, S. Dodelson, P. Doel, C. Doux, J. García-Bellido, D. Gruen, G. Gutierrez, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. Huterer, D. J. James, K. Kuehn, O. Lahav, S. Lee, J. L. Marshall, J. Mena-Fernández, F. Menanteau, J. J. Mohr, J. Myles, R. L. C. Ogando, M. Paterno, A. A. Plazas Malagón, R. Rosenfeld, E. Sanchez, M. Smith, M. Soares-Santos, E. Suchyta, V. Vikram

Dark Energy Survey Year 6 Results: Magnification modeling and its impact on galaxy clustering and galaxy-galaxy lensing cosmology

Gravitational lensing magnification alters the observed spatial distribution of galaxies and must be accounted for to prevent biases in cosmological probes of the large-scale structure. We investigate its effects on the Dark Energy Survey Year 6 galaxy clustering and galaxy-galaxy lensing analyses using the fiducial lens (position...

💬 0 commentsarXiv:2601.14833v1PDF
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Posted in hep-ex · 2026-01-21 · Jake McKean, Laura Munteanu, Seisho Abe

Benchmarking neutrino-nucleus quasielastic scattering model predictions against a missing energy profile obtained using a monoenergetic neutrino beam

We examine three exclusive nuclear ground state shell models implemented in the NEUT neutrino event generator and benchmark them against the recent JSNS$^2$ measurement of missing energy using a monoenergetic neutrino source. The nature of the measurement allows a detailed investigation of nuclear ground-state modeling using a...

💬 0 commentsarXiv:2601.14831v5PDF
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Posted in astro-ph.HE · 2026-01-21 · Monalisa Dubey, Kuntal Misra, Géza Csörnyei, Raya Dastidar, D. Andrew Howell, David J. Sand, Stefano Valenti, WeiKang Zheng, Alexei V. Filippenko, Saurabh Jha, Jesper Sollerman, Peter Brown, Kate D. Alexander, Moira Andrews, Jennifer Andrews, Dre Betz, Emma Born, Kate Bostow, K. Azalee Bostroem, Sea'n J. Brennan, Thomas G. Brink, Collin Christy, Elma Chuang, Yize Dong, Naveen Dukiya, Joseph R. Farah, Noah Franz, Estefania Padilla Gonzalez, Joshua Haislip, Emily Hoang, Griffin Hosseinzadeh, Brian Hsu, Connor Jennings, Vladimir Kouprianov, M. J. Lundquist, Colin Macrie, Curtis McCully, Andrew Mchaty, Darshana Mehta, Katie Mora, Megan Newsome, Jeniveve Pearson, Neil Pichay, Conor Ransome, Aravind P. Ravi, Daniel E. Reichart, Nicolás Meza Retamal, Sophia Risin, Manisha Shrestha, Ajay Kumar Singh, Nathan Smith, Bhagya Subrayan, Giacomo Terreran, William Wu

SN 2023zcu: A Type IIP SN with Early Flash Features

We present a detailed photometric and spectroscopic analysis of the Type IIP supernova SN~2023zcu, which exploded in the galaxy NGC~2139 (redshift $z$ = 0.006). SN~2023zcu exhibits a well-sampled light curve covering the rise, plateau, and nebular phases. It has an optically thick phase of $100.6 \pm 0.6$ d with a magnitude drop of...

💬 0 commentsarXiv:2601.14830v1PDF
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Posted in hep-ph · 2026-01-21 · Héctor Cancio, Pere Masjuan

Phenomenology of a double dilaton soft-wall model: Alpha strong from Ricci flow and pion Form Factors at intermediate-energy region

Through a holographic model of QCD, we present a phenomenological approach to study the running of the strong coupling constant α_s in both non-perturbative and perturbative regimes. The renormalization of the metric tensor, driven by the Ricci Flow, and the breaking of conformal and chiral symmetries -- thanks to introducing a double...

💬 0 commentsarXiv:2601.14829v2PDF
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Posted in quant-ph · 2026-01-21 · Claudia Benedetti, Giovanni Ragazzi, Simone Cavazzoni, Paolo Bordone, Matteo G. A. Paris

Routing Qubits on Noisy Networks

Robust quantum routing is essential for scalable quantum technologies. This paper investigates the resilience of routing protocols in network architectures designed for perfect, high-fidelity transfer of both classical and quantum information under ideal conditions. We encode information in the position of a quantum walker on a graph,...

💬 0 commentsarXiv:2601.14824v1PDF
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Posted in cond-mat.str-el · 2026-01-21 · Gennadiy Ivanovich Mironov

Ionization energy and electron affinity of fullerene C60 in the Hubbard model in the static fluctuation approximation

Within the Hubbard model, the ionization energy and electron affinity of the icosahedral C60 fullerene are calculated in the static fluctuation approximation. A graphical representation of the chemical potential equation is first obtained. The correlation function, which describes the transitions of π-electrons from one fullerene site...

💬 0 commentsarXiv:2601.14817v1PDF