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๐Ÿ” sam devlin ๐Ÿ“‚ Physics
Showing 11644 results for "sam devlin" in Physics
Physics Preprint PDF DOI

Bridging Metal Additive Manufacturing and RF Accelerator Design: Development of a 704.4 MHz Crossbar H-Mode Linac for Efficient Beam Acceleration

Chuan Zhang, Eduard Boos, Roland Boehm, Ramy Cherif, Alexander Japs, Stefan Wunderlich ยท 2026

The development of Ultra-High Frequency (UHF) linear accelerators via Metal Additive Manufacturing (MAM) is a strategic research focus of the RACERS team at GSI. The 704.4 MHz Crossbar H-mode (CH) cavโ€ฆ

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Physics Preprint PDF DOI

The Recurrent Nova Population in M31

Allen W. Shafter, Kamil Hornoch ยท 2026

The positions of more than 1300 nova eruptions in M31 catalogued through the end of calendar year 2025 have been compared in order to identify recurrent nova candidates. The work extends the study of โ€ฆ

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Physics Preprint PDF DOI

Parameter Estimation of the Gravitational-Wave Angular Power Spectrum in the Dirty-Map Space

Erik Floden, Alex Granados, Vuk Mandic ยท 2026

We consider a search for the anisotropic stochastic gravitational-wave background (SGWB) that decomposes the sky map into its spherical harmonics components in order to obtain estimators of the angulaโ€ฆ

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Physics Preprint PDF DOI

A search for the first galaxies across $>0.6$ deg$^2$ of JWST imaging: new evidence for a rapid decline in star-formation activity at $z>12$

D. J. McLeod, J. S. Dunlop, R. J. McLure, C. T. Donnan, R. Begley, S. Antonogiannaki, D. Magee, G. D. Illingworth, P. Arrabal Haro, C. Bondestam, A. C. Carnall, F. Cullen, M. Dickinson, R. S. Ellis, B. L. Frye, H. Golawska, N. A. Grogin, I. J. B. Holst, P. S. Kamieneski, H. -H. Leung, F. -Y. Liu, T. M. Stanton, E. R. Tittley ยท 2026

We present a new determination of the evolving galaxy UV luminosity function (LF) over the extreme redshift range $12.5<z<18.5$, based on a wide-area search of $>$0.6 deg$^2$ of JWST NIRCam imaging coโ€ฆ

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Physics Preprint PDF DOI

Early onset of secondary shear instability in Kelvin-Helmholtz braids at high Reynolds number

Emma R. Bouckley, Sam F. Lewin, Adrien Lefauve ยท 2026

We study the onset of two-dimensional secondary shear instability (SSI) in the braid regions connecting primary Kelvin-Helmholtz billows in stratified shear flows. While strain induced by the billows โ€ฆ

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Comment on "Angular momentum dynamics of vortex particles in accelerators''

S.S. Baturin ยท 2026

We comment on Ref.[D. Karlovets, D. Grosman, and I. Pavlov, Phys. Rev. Lett. 136, 085002 (2026)], which proposes a BMT-like equation for the mean kinetic orbital angular momentum (OAM) of vortex partiโ€ฆ

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Sky background accounting in spectral infrared observations of extended objects at the Caucasus Mountain Observatory of the SAI MSU

A.S. Gusev, A.M. Tatarnikov, S.G. Zheltoukhov, M.S. Kirsanova ยท 2026

The Caucasus Mountain Observatory of the Sternberg Astronomical Institute of Moscow State University is the only one in Russia and one of the few in the world where is possible to obtain spectral dataโ€ฆ

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Multi-modes Bessel-Gaussian-Orbital Angular Momentum Beams Quantum Holography

Jinjin Li, Chaoying Zhao ยท 2026

We propose an orbital angular momentum (OAM) quantum holography scheme based on multi-mode Bessel-Gaussian (MBG) beams. Entangled photon pairs are generated through spontaneous parametric down-conversโ€ฆ

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Correlation invariance unlocks robust calibration-free orbital-angular-momentum multiplexing transmission under dynamic scattering scenarios

Haoran Li, Zhiyuan Wang, Zhipeng Yu, Xingpeng Du, Tianting Zhong, Jixiong Pu, Ziyang Chen, Vinu R V, Xiangping Li, Puxiang Lai ยท 2026

Orbital angular momentum (OAM) multiplexing offers a promising approach to high-capacity optical communication by harnessing the orthogonality of vortex beams. However, its practical deployment is sevโ€ฆ

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Hanbury Brown-Twiss effect and classical entanglement with OAM-carrying light

Jyrki Laatikainen, Sushil Pokharel, Olga Korotkova ยท 2026

We establish a decomposition of the intensity-intensity correlation of a scalar optical beam carrying orbital angular momentum (OAM) across multiple modes into intermodal contributions, thereby linkinโ€ฆ

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Beyond the Dilute Instanton Gas: Resurgence with Exact Saddles in the Double Well

Aurelien Dersy, Matthew D. Schwartz ยท 2026

The path-integral approach to the double well has long been limited by the dilute instanton gas approximation. We show that if the finite Euclidean-time structure is taken seriously by using exact sadโ€ฆ

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Single Plane Spatial Mode Sorter

Khen Cohen, Yoav Yosif-Or, Yaron Oz, Ady Arie ยท 2026

A mode sorter separates a set of M orthogonal spatial modes in a shared input channel into M different output channels. Here we present an analytic derivation and experimental validation of a single pโ€ฆ

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Radial Distribution of Star Formation and Gas-phase Metallicity in Spiral-Elliptical Galaxy Pairs

Cailu Shi, Shuai Feng, Shiyin Shen, Linlin Li, Wenyuan Cui, Guozhen Hu ยท 2026

Using integral field spectroscopy from SDSS-IV MaNGA, we investigate the radial distributions of star formation rate (SFR) and gas-phase metallicity in spiral galaxies that reside in spiral-ellipticalโ€ฆ

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JOYS$+$: A JWST/MIRI survey of the evolution of H$_2$ winds and jets from low-mass protostars

L. Francis, {L}. Tychoniec, E. F. van Dishoeck, A. D. Sellek, A.Caratti o Garatti, V. J. M. Le Gouellec, C. Gieser, H. Beuther, J. M. Vorster, M. E. Ressler, P. Nazari, B. Tabone, K. Assani, R. Devaraj, J. J. Tobin, Maria Gabriela Navarro, P. C. Cortes, J. M. Girart, M. Gudel, Th. Henning, G. Ostlin, G. Wright, T. Ray ยท 2026

Protostellar outflows display wide-angle winds and collimated jets, the magnetocentrifugal launching of which enables accretion onto the protostar. The majority of the outflow mass is likely ejected oโ€ฆ

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Manipulation of Superposed Vortex States of $\gamma$ Photon via Nonlinear Compton Scattering

Jun-Lin Zhou, Mamutjan Ababekri, Yong-Zheng Ren, Yu Wang, Ren-Tong Guo, Zhao-Hui Chen, Yu-Han Kou, Zhong-Peng Li, Jian-Xing Li ยท 2026

Vortex $\gamma$ photons in superposition states have important applications in photonuclear, high-energy, and strong-field physics. However, their controlled generation in the $\gamma$-ray regime remaโ€ฆ

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Quantum chaos in many-body systems of indistinguishable particles

Juan-Diego Urbina, Klaus Richter ยท 2026

In quantum systems with a classical limit, advanced semiclassical methods provide the crucial link between phase-space structures, reflecting the distinction between chaotic, mixed or integrable classโ€ฆ

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Kelvin waves over a differentially rotating spherical shell

T. Boismard, M. Rieutord ยท 2026

Context. Be stars are presently viewed as B-type stars surrounded by a disc fueled by the star itself during episodicexcretion events. The origin of these events are poorly understood.Aims. This articโ€ฆ

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The parity operator for parafermions and parabosons

N.I. Stoilova, J. Van der Jeugt ยท 2026

In this paper we reexamine the definition of parafermions and parabosons by means of Green's triple relations, and extend these relations by including a parity operator $P$ which is also determined byโ€ฆ

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Spatially Resolved Kinematics of SLACS Lens Galaxies. II: Breaking Degeneracies with Lensing and Dynamical Models

Shawn Knabel, Tommaso Treu, Michele Cappellari, Simon Birrer, Xiang-Yu Huang, Anowar J. Shajib, William Sheu ยท 2026

We model the dynamical mass density profiles of 14 strong gravitational lens galaxies from the Sloan Lens ACS (SLACS) sample using spatially resolved kinematics obtained from Keck KCWI integral-field โ€ฆ

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JOYS: Launching and destruction of dust in protostellar jets. The case of BHR71-IRS1 with JWST/MIRI

{L}ukasz Tychoniec, Logan Francis, Maria Gabriela Navarro, Jakobus M. Vorster, Ewine F. van Dishoeck, Alessio Caratti o Garatti, Korash Assani, Valentin J. M. Le Gouellec, Benoit Tabone, Pamela Klaassen, Adriaan G. M. Janssen, Kay Justtanont, Daniel Harsono, Pooneh Nazari, Simon Reyes, Katerina Slavicinska, Caroline Gieser, Tyler Bourke, Yao-Lun Yang, Brunella Nisini, Teresa Giannini, Henrik Beuther, R. Devaraj, Thomas P. Ray, Nashanty G. C. Brunken, Yuan Chen, Martijn L. van Gelder ยท 2026

Protostellar winds can theoretically lift solids from the planet-forming disks, but direct evidence for launched dust has been scarce so far. Numerous atomic lines that are unique to mid-infrared (IR)โ€ฆ

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