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๐Ÿ” adrian kent ๐Ÿ“‚ Physics
Showing 8871 results for "adrian kent" in Physics
Physics Preprint PDF DOI

Applications of 1.4 GHz diagnostics to Type Ia Supernova host galaxies

S. Ramaiya, M. J. Jarvis, M. Vincenzi, M. Sullivan, I. H. Whittam ยท 2026

Type Ia supernova (SN Ia) standardisation parameters exhibit evidence for systematic variation across the host galaxy star-formation rate - stellar mass (SFR$-M_\star$) plane, motivating the incorporaโ€ฆ

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Physics Preprint PDF DOI

Multi-wavelength polarisation imaging with inverse designed metasurfaces

Sarah E. Dean, Neuton Li, Josephine Munro, Benjamin Laudert, Thomas Siefke, Quyet Ngo, Robert Sharp, Dragomir N. Neshev, Falk Eilenberger, Andrey A. Sukhorukov ยท 2026

Multispectral polarisation imaging has a broad range of applications, from biological cell imaging to agricultural remote surveying. For such applications, especially involving lightweight unmanned aeโ€ฆ

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SRGA J115215.0$-$510656: an unusual long-period eclipsing dwarf nova with disc wind signatures

Nikita Rawat, David A. H. Buckley, John R. Thorstensen, Christian Knigge, Yusuke Tampo, Stephen B. Potter, Anupam Bhardwaj, Simone Scaringi, Ilya A. Mereminskiy, Jeewan C. Pandey, Srinivas M Rao, Alexander A. Lutovinov ยท 2026

We present the first detailed optical study of the cataclysmic variable SRGA J115215.0$-$510656, based on new time-resolved photometric and spectroscopic observations complemented by long-baseline Traโ€ฆ

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Rigged Liouville space formulation for quasi-Hermitian Liouville operators

Shousuke Ohmori, Junichi Takahashi ยท 2026

We discuss a super bra-ket formalism for quasi-Hermitian Liouvillian operators within the framework of rigged Hilbert spaces (RHS). An RHS in terms of the Liouville space, referred to as a rigged Liouโ€ฆ

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Structure Prediction and Bonding Analysis of B$_{18}$Ag$_2$ Clusters Featuring Double-Ring Motifs

Peter Ludwig Rodriguez-Kessler ยท 2026

The structural stability, electronic structure, and bonding characteristics of the silver-doped boron cluster B18Ag2 were investigated using density functional theory (DFT) combined with global optimiโ€ฆ

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Asteroseismic analysis of RY Leporis: the post-main sequence HADS in a binary system

Wojciech Niewiadomski, Jadwiga Daszynska-Daszkiewicz, Przemys{l}aw Walczak, Wojciech Szewczuk, Eloy Rodriguez, Piotr Ko{l}aczek-Szymanski, Aliz Derekas ยท 2026

We present a comprehensive study of the pulsating primary component of the long-period binary system RY Lep. The spectral energy distribution and the absence of detectable lines indicate that the compโ€ฆ

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Physics Preprint PDF DOI

Quantum-Accelerated Gowers $U_2$ Norm for Bent Boolean Functions

Rajdeep Dwivedi, C. A Jothishwaran, Sugata Gangopadhyay, Vishvendra Singh Poonia ยท 2026

Bent Boolean functions extremal objects that maximally resist affine approximation are notoriously hard to construct for large numbers of variables. We propose a hybrid quantum-classical genetic aโ€ฆ

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Demonstration of quantum random number generation using nitrogen vacancy centres

Conrad Strydom, Mark Tame ยท 2026

Quantum random number generation (QRNG) relies on the inherent unpredictability of quantum mechanical phenomena to efficiently generate high-quality random numbers that can be used in a wide range of โ€ฆ

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Propagating data-driven galaxy redshift distribution uncertainties in 3$\times$2-pt analyses

Jaime Ruiz-Zapatero, Qianjun Hang, Yun-Hao Zhang, Benjamin Joachimi, Joe Zuntz, Ian Harrison, Carlos Garcia-Garcia, Alex Malz, Benjamin Stolzner, the LSST Dark Energy Science Collaboration ยท 2026

Uncertainties in the radial distribution of galaxies, $\boldsymbol{n}(\boldsymbol{z})$, are one of the major contributions to the error budget of early Stage-IV galaxy survey analyses of weak gravitatโ€ฆ

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Physics Preprint PDF DOI

Can classical theories of gravity produce entanglement?

Anirudh Gundhi, Giorgia Infantino, Angelo Bassi ยท 2026

A recent paper published on Nature [Nature,646,813(2025)] by Aziz and Howl, claims that quantum particles become entangled when they interact gravitationally, even if the gravitational potential is trโ€ฆ

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Localization and Confidence Region Estimation of Short GRBs with the COSI BGO Shield Using a HEALPix-Based Deep Learning Approach

N. Parmiggiani, A. Bulgarelli, G. Panebianco, E. Burns, E. Neights, V. Fioretti, I. Martinez-Castellanos, L. Castaldini, A. Ciabattoni, A. Di Piano, R. Falco, S. Gallego, G. Mustafa, P. Patel, A. Rizzo, E. A. Wulf, D. H. Hartmann, C. A. Kierans, J. A. Tomsick, A. Zoglauer ยท 2026

The Compton Spectrometer and Imager is a NASA satellite mission under development that will survey the entire sky in the 0.2-5 MeV range using a wide-field germanium detector array, surrounded on the โ€ฆ

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A Salpeter-like filament linear density function across nearby molecular clouds

Guo-Yin Zhang, Alexander Men'shchikov, Jin-Zeng Li ยท 2026

Filamentary structures in molecular clouds are thought to play a central role in star formation, yet the statistical distribution of their mass per unit length -- and any connection to the stellar iniโ€ฆ

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Massive star clusters and clumps in the collisional ring galaxy Arp 147

Z. Randriamanakoto, M. Rakototafika, B. Mongwane, P. Vaisanen, M. Rakotomanga ยท 2026

We conduct a photometric study of star clusters (or knots) in the collisional ring galaxy (CRG) Arp 147 to trace the star formation history across its empty ring. Using HST F450W, F606W and F814W imagโ€ฆ

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Metal enrichment in the galaxy group IC 1262

Satish S. Sonkamble, Dharam V. Lal, S. Ilani Loubser, Mahadev B. Pandge ยท 2026

We present a new metal enrichment analysis of a unique galaxy group IC 1262 using archival Chandra and GMRT observations, focusing on metal transport via radio jet, sloshing cold fronts, and shock froโ€ฆ

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M1-92: AGB interruption and isotopic ratio paradox. Chemistry and morpho-kinematics from improved shapemol modelling

E. Masa, J. Alcolea, M. Santander-Garcia, V. Bujarrabal, C. Sanchez Contreras, A. Castro-Carrizo, W. Steffen, N. Koning ยท 2026

The shaping of planetary nebulae on their evolution from asymptotic giant branch circumstellar envelopes to their final, most often axisymmetrical, form is still a process with many unknown details. Tโ€ฆ

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Significantly enhanced detectability of dark photons with a steady-state excited microwave cavity

S. R. He, L. Gao, P. H. Ouyang, H. Zheng, X. N. Feng, L. F. Wei ยท 2026

The resonant cavity system has been widely used to search for the electromagnetic response of dark photons, although its achievable detection sensitivity remains at a relatively low level. In this letโ€ฆ

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Systematic Design of Local Rules for Directing Emergent Structure in Bottom-Up Systems

Andrew Slezak, Varda F. Hagh ยท 2026

Many biological systems collectively construct complex, adaptive, and functional architectures, where function emerges from bottom-up building processes rather than top-down planning or centralized coโ€ฆ

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Critical transverse compressive stresses of straight and bent CORC$^\circledR$ wires with and without impregnation

X. Xu, F. Wan, S. Cohan, V. V. Kashikhin ยท 2026

CORC$^\circledR$ wires are a promising superconductor for accelerator magnet applications. While their excellent uniaxial tensile properties have been well established, potential degradation under traโ€ฆ

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Catapult neutrons from neck snapping in fission

J{o}rgen Randrup, Roberto Capote, Ramona Vogt ยท 2026

Dynamical fission calculations show that the post-scission configurations resemble two collinear pear-shaped fragments whose juxtaposed surface bulges subside relatively quickly, as the fragments acquโ€ฆ

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Ages and masses of asymptotic giant branch stars from the period--luminosity diagram

Iain McDonald ยท 2026

A method of determining ages and masses of asymptotic giant branch (AGB) stars between 0.8 and $\sim$6 M$_\odot$ is demonstrated, based on comparing the star's position in the period--absolute-magnituโ€ฆ

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