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๐Ÿ” program evaluation ๐Ÿ“‚ Physics
Showing 135435 results for "program evaluation" in Physics
Physics Preprint PDF DOI

$3d_{z^2}$ orbital delocalization and magnetic collapse in superconducting (La,Pr)$_3$Ni$_2$O$_{7-\delta}$ films

Xiaoyang Chen, Wenliang Zhang, Fei Peng, Ting Cui, Guangdi Zhou, Zezhong Li, Jaewon Choi, Lizhi Xu, Yiu-Fung Chiu, Stefano Agrestini, Sahil Tippireddy, Haoliang Huang, Heng Wang, Xianfeng Wu, Peng Li, Jin-Feng Jia, Mirian Garcia-Fernandez, Yi Lu, Er-Jia Guo, Qi-Kun Xue, Zhuoyu Chen, Donglai Feng, Ke-Jin Zhou ยท 2026

The recent discovery of Ruddlesden--Popper (RP) nickelate thin-film superconductors has opened a new frontier in unconventional superconductivity. Its realization requires both compressive epitaxial sโ€ฆ

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Ion Channel Dynamics in Temperature-Dependent Weibel Instability Saturation

Vivek Shrivastav, Mani K Chettri, Hemam D. Singh, Britan Singh, Rupak Mukherjee ยท 2026

We present 1X2V continuum Vlasov-Maxwell simulations of interpenetrating plasma beams with mobile ions. While the early-time evolution is similar to the stationary-ion case, the late-time dynamics areโ€ฆ

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High-performance cellular automaton decoders for quantum repetition and toric code

Don Winter, Thiago L. M. Guedes, Markus Muller ยท 2026

Execution of quantum algorithms on large-scale quantum computers will require extremely low logical error rates, which necessitates the development of scalable decoding architectures. Local decoders aโ€ฆ

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Replay-buffer engineering for noise-robust quantum circuit optimization

Akash Kundu, Sebastian Feld ยท 2026

Deep reinforcement learning (RL) for quantum circuit optimization faces three fundamental bottlenecks: replay buffers that ignore the reliability of temporal-difference (TD) targets, curriculum-based โ€ฆ

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Perturbation Dynamics and Structure Formation in Extended Proca-Nuevo Gravity

N. S. Kavya, Avik De, Tee-How Loo ยท 2026

A comprehensive analysis of cosmological perturbations and structure formation is presented for the Extended Proca-Nuevo (EPN) framework, a vector-tensor extension of General Relativity with a massiveโ€ฆ

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Broad-band High-Energy Resolution Hard X-ray Spectroscopy using Transition Edge Sensors at SPring-8

Shinya Yamada, Yuto Ichinohe, Hideyuki Tatsuno, Ryota Hayakawa, Hirotaka Suda, Takaya Ohashi, Yoshitaka Ishisaki, Tomoya Uruga, Oki Sekizawa, Kiyofumi Nitta, Yoshio Takahashi, Takaaki Itai, Hiroki Suga, Makoto Nagasawa, Masato Tanaka, Minako Kurisu, Tadashi Hashimoto, Douglas Bennett, Ed Denison, William (Randy) Doriese, Malcolm Durkin, Joseph Fowler, Galen O'Neil, Kelsey Morgan, Dan Schmidt, Daniel Swetz, Joel Ullom, Leila Vale, Shinji Okada, Takuma Okumura, Toshiyuki Azuma, Toru Tamagawa, Tadaaki Isobe, Satoshi Kohjiro, Hirofumi Noda, Keigo Tanaka, Akimichi Taguchi, Yuki Imai, Kosuke Sato, Tasuku Hayashi, Teruhiko Kashiwabara, Kohei Sakata ยท 2026

We have succeeded in operating a transition-edge sensor (TES) spectrometer and evaluating its performance at the SPring-8 synchrotron X-ray light source. The TES spectrometer consists of a 240 pixel Nโ€ฆ

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Multi-Nucleon Transfer Reactions and the Creation and the Evolution of the Compound Nucleus

Matthew Kafker, Aurel Bulgac ยท 2026

There is no microscopic quantum approach based on the time-dependent Schr\"{o}dinger equation which has yet to describe the formation of a compound nucleus. The most advanced microscopic approach deveโ€ฆ

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Unitary Time Evolution and Vacuum for a Quantum Stable Ghost

Cedric Deffayet, Atabak Fathe Jalali, Aaron Held, Shinji Mukohyama, Alexander Vikman ยท 2026

We quantize a classically stable system of a harmonic oscillator polynomially coupled to a ghost with negative kinetic energy. We prove that due to an integral of motion with a positive discrete spectโ€ฆ

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The clock ambiguity problem: extended or extinguished?

Ovidiu Cristinel Stoica ยท 2026

I show that the clock ambiguity cannot be solved by a purely relational condition like the noninteraction condition, and it is even stronger, extending to evolution laws. The ambiguity is solved by spโ€ฆ

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Ground-state properties of superheavy $Z=122$ isotopes within the deformed relativistic Hartree-Bogoliubov theory in continuum

Jin-Hong Zhuang, Zhen-Hua Zhang, Yuan-Yuan Wang, Cong Pan, Kai-Yuan Zhang, Huan-Yu Zhang, Yu Sun ยท 2026

The ground-state properties of superheavy $Z = 122$ isotopes are investigated using the deformed relativistic Hartree-Bogoliubov theory in continuum (DRHBc). Bulk properties, including binding energieโ€ฆ

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Direct observation of surface bandgap shrinkage and negative electronic compressibility in SrTiO3

Warakorn Jindata, Trung-Phuc Vo, Chutchawan Jaisuk, Sung-Kwan Mo, Thanh-Tien Nguyen, Jan Minar, Worawat Meevasana ยท 2026

In this work, we investigate and compare the electronic structures of SrTiO3 and KTaO3 under ultraviolet (UV) light induced electron doping. Using angle-resolved photoemission spectroscopy (ARPES), thโ€ฆ

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Nearly Complete Charge--Spin Conversion via Strain-Eliminated Fermi Pockets in $d$-Wave Altermagnets

Wancheng Zhang, Zhenhua Zhang, Rui Xiong, Zhihong Lu ยท 2026

$d$-wave altermagnets possess nearly orthogonal flat Fermi surfaces, which in an idealized limit enable complete spin-channel separation and a theoretical charge-to-spin conversion efficiency (CSE) ofโ€ฆ

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Quantum-information diagnostics of cosmological perturbations with nontrivial sound speed in inflation

Shi-Cheng Liu, Lei-Hua Liu, Bichu Li, Hai-Qing Zhang, Peng-Zhang He ยท 2026

In this work, we systematically investigate the quantum-information diagnostics of cosmological perturbations with a nontrivial sound speed, utilizing a normalized open two-mode squeezed-state framewoโ€ฆ

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Neural surrogates for crystal growth dynamics with variable supersaturation: explicit vs. implicit conditioning

Matteo Rigoni, Daniele Lanzoni, Francesco Montalenti, Roberto Bergamaschini ยท 2026

Simulations of crystal growth are performed by using Convolutional Recurrent Neural Network surrogate models, trained on a dataset of time sequences computed by numerical integration of Allen-Cahn dynโ€ฆ

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Delving into the depths of NGC 3783 with XRISM: V. Broad-band modeling of ionized outflows

Keqin Zhao, Jelle S. Kaastra, Liyi Gu, Missagh Mehdipour, Megan E. Eckart, Keigo Fukumura, Matteo Guainazzi, Chen Li, Christos Panagiotou, Matilde Signorini ยท 2026

The Seyfert 1 galaxy NGC 3783 hosts a multiphase warm absorber (WA) that has been extensively studied in the X-ray band. High-resolution spectra from 2000-2001 revealed a complex outflow with multipleโ€ฆ

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Towards hybrid kinetic/drift-kinetic simulations in 6d Vlasov codes

M. Pelkner, K. Hallatschek, M. Raeth ยท 2026

Simulating fully kinetic, two-species plasmas is computationally challenging due to the stiff multiscale dynamics of electrons and ions. While enforcing a quasi-neutral time evolution mitigates this sโ€ฆ

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Self-consistent evaluation of the Berry connection for Wannier functions

Martin Thummler, Alexander Croy, Thomas Lettau, Ulf Peschel, Stefanie Grafe ยท 2026

The Berry connection is a gauge-dependent quantity frequently used to describe the optical response of solids. Its evaluation requires a k-derivative with respect to the cell periodic-part of the Blocโ€ฆ

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Modeling of the magnetic stellar wind braking of the ssrAp 33 Lib (HD137949)

A.G. Nikiforov, V.D. Bychkov, M.V. Barkov ยท 2026

Using the ssrAp star 33 Lib (HD137949) as an example, we show that magnetic braking caused by the interaction of a strong magnetic field with a stellar wind can play a key role in slowing the rotationโ€ฆ

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Two-gap to Single-gap Transition and Two-dome-like Superconductivity in Alkali-Metal Intercalated Bilayer PdTe2

Yu-Lin Han, Shu-Xiang Qiao, Kai-Yue Jiang, Jie Zhang, Bao-Tian Wang, Ping Zhang, C. S. Ting, Hong-Yan Lu ยท 2026

PdTe2 has been synthesized with controllable thickness down to the monolayer limit. Based on first-principles calculations within the fully anisotropic Migdal-Eliashberg framework, this work reveals tโ€ฆ

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Aspects of gravitational clustering and structure formation in the Universe

Swati Gavas ยท 2026

The distribution of galaxies, halo abundance, and peculiar velocities are influenced by non-linear gravitational interactions, making the study of non-linear evolution crucial for accurate cosmologicaโ€ฆ

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