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๐Ÿ” arnab acharya ๐Ÿ“‚ Physics
Showing 247 results for "arnab acharya" in Physics
Physics Preprint PDF DOI

Transition path sampling in Ising models on heterogeneous graphs

Riccardo Cipolloni, Federico Ricci-Tersenghi, Francesco Zamponi ยท 2026

Activated transitions have rates that are often exponentially small in system size. Extracting the associated activation barriers is challenging in practice, especially in the deeply metastable regimeโ€ฆ

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Physics Preprint PDF DOI

CHARA Interferometry and TESS Asteroseismology of the Core-Helium Burning Red Giant $\kappa$ Cyg

Arnab Chowhan, Timothy R. Bedding, Daniel Huber, J. M. Joel Ong, Lea S. Schimak, Yaguang Li, Courtney L. Crawford, Timothy R. White ยท 2026

We present a detailed study of the secondary red clump star, $\kappa$ Cyg, by combining long-baseline visible interferometry using the PAVO beam combiner at the CHARA Array with high-precision asterosโ€ฆ

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Physics Preprint PDF DOI

Distributed Quantum Property Testing with Communication Constraints

Mina Doosti, Ryan Sweke, Chirag Wadhwa ยท 2026

We introduce a framework for distributed quantum inference under communication constraints. In our model, $m$ distributed nodes each receive one copy of an unknown $d$-dimensional quantum state $\rho$โ€ฆ

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Physics Preprint PDF DOI

Complete synchronization in networks of Sakaguchi-Kuramoto oscillators with bi-harmonic coupling

Subhasish Chowdhury, Sangita Dutta, Pitambar Khanra, Swarup Kumar Laha, Prosenjit Kundu ยท 2026

In heterogeneous networks of coupled oscillators, phase frustration typically prevents the emergence of complete synchronization in the Sakaguchi-Kuramoto (SK) model. In this study, we propose an analโ€ฆ

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Physics Preprint PDF DOI

Detection and Astrometry of the Ba-Bb Subsystem in $\alpha$ Piscium: First Dual-Field Interferometry at the CHARA Array

Narsireddy Anugu, Robert Klement, John D. Monnier, Douglas R. Gies, Gail H. Schaefer, Stefan Kraus, Sebastian Carrazco-Gaxiola, Akshat S. Chaturvedi, Mayra Gutierrez, Becky Flores, Jeremy Jones, Colin Kane, Rainer Kohler, Karolina Kubiak, Olli W. Majoinen, Nicholas J. Scott, Kayvon Sharifi ยท 2026

We present the first on-sky demonstration of dual-field interferometry at the CHARA Array and the first direct resolution of the inner Ba--Bb subsystem in the bright hierarchical triple $\alpha$ Pisciโ€ฆ

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Physics Preprint PDF DOI

CHARA Array Delay Lines: Upgrades, Performance and Future Directions

Narsireddy Anugu, Nils H. Turner, Theo A. ten Brummelaar, Gail H. Schaefer, Philippe Berio, Christopher D. Farrington, Becky Flores, Douglas R. Gies, Stefan Kraus, Edgar R. Ligon III, Olli Majoinen, John D. Monnier, Denis Mourard, Nicholas J. Scott, Norman L. Vargas ยท 2026

Long baseline optical and infrared interferometric arrays achieve high angular resolution and enable detailed astrophysical measurements. Interferometers have enabled observations of stars at various โ€ฆ

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Physics Preprint PDF DOI

Influence of electrical properties on thermal boundary conductance at metal/semiconductor interface

Quentin Pompidou (ITheMM, URCA UFR SEN), Juan Carlos Acosta Abanto (CETHIL), M. Brouillard (IEMN, MICROELEC SI - IEMN), Nicolas Bercu (L2n, LRN), L. Giraudet (L2n, LRN), Rami Sheikh, C. Adessi (ILM, iLM - ENERGIE, iLM - MMCI), S. Merabia (ILM, iLM - ENERGIE, iLM - MMCI), S. Gomes (CETHIL), Pierre-Olivier Chapuis (CETHIL), J.-F. Robillard (MICROELEC SI - IEMN, IEMN), Mihai Chirtoc (ITheMM, URCA UFR SEN), N. Horny (ITheMM, URCA UFR SEN) ยท 2026

Recent experimental investigations have demonstrated that doping a semiconductor is a route to increase the thermal boundary conductance at metal/semiconductor interfaces. In this work, the influence โ€ฆ

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Physics Preprint PDF DOI

Analytic Interferometry of Rotating Stellar Surfaces

Shashank Dholakia, Benjamin J. S. Pope ยท 2025

The surfaces of rotating stars serve as a window into their interiors, magnetic dynamos, and are important in other areas including exoplanet discovery and atmospheric characterization. While indirectโ€ฆ

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Physics Preprint PDF DOI

The CHARA Array Polarization Model and Prospects for Spectropolarimetry

Linling Shuai, John D. Monnier, Benjamin R. Setterholm, Stefan Kraus, Narsireddy Anugu, Tyler Gardner, Jean-Baptiste Le Bouquin, Gail H. Schaefer ยท 2025

Polarimetric data provide key insights into infrared emission mechanisms in the inner disks of YSOs and the details of dust formation around AGB stars. While polarization measurements are well-establiโ€ฆ

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Physics Preprint PDF DOI

The Small Separation A-Star Companion Population: Tentative Signatures of Enhanced Multiplicity with Primary Mass

Matthew De Furio, Tyler Gardner, John D. Monnier, Michael R. Meyer, Kaitlin M. Kratter, Cyprien Lanthermann, Narsireddy Anugu, Stefan Kraus, Benjamin R. Setterholm ยท 2025

We present updated results from our near-infrared long-baseline interferometry (LBI) survey to constrain the multiplicity properties of intermediate-mass A-type stars within 80 pc. Previous adaptive oโ€ฆ

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Physics Preprint PDF DOI

Precise Age For The Binary HD 21278 In The Young Alpha Persei Cluster

Christopher A. Danner, Eric L. Sandquist, Gail H. Schaefer, Luigi R. Bedin, Christopher D. Farrington, Cyprien Lanthermann, Stefan Kraus, Robert Klement, Narsireddy Anugu, John D. Monnier, Jerome A. Orosz, Isabelle Codron, Tyler Gardner, Mayra Gutierrez, Benjamin R. Setterholm, Jeremy Jones, Becky Flores ยท 2025

We present a study of the double-lined spectroscopic binary HD 21278 that contains one of the brightest main sequence stars in the young $\alpha$ Persei open cluster. We analyzed new spectra and reanaโ€ฆ

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Physics Preprint PDF DOI

Constraining the physical structure of the circumstellar environment of V838 Monocerotis remnant

Muhammad Zain Mobeen, Tomasz Kaminski, Stephen Potter ยท 2025

V838 Monocerotis (V838 Mon) erupted in 2002 as a luminous red nova after which it cooled and began to form dust. The remnant is predicted to become a blue straggler. Interferometric observations in thโ€ฆ

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Physics Preprint PDF DOI

The Dynamic Inner Disk of a Planet Forming Star

Benjamin R. Setterholm, John D. Monnier, Fabien Baron, Jaehan Bae, Jacques Kluska, Stefan Kraus, Nuria Calvet, Nour Ibrahim, Evan Rich, Narsireddy Anugu, Claire L. Davies, Jacob Ennis, Tyler Gardner, Aaron Labdon, Cyprien Lanthermann, Gail Schaefer ยท 2025

Planets are a natural byproduct of the stellar formation process, resulting from local aggregations of material within the disks surrounding young stars. Whereas signatures of gas-giant planets at larโ€ฆ

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Physics Preprint PDF DOI

A Spectroscopic and Interferometric Study of W Serpentis Stars. I. Circumbinary Outflow in the Interacting Binary W Serpentis

Katherine Shepard, Douglas R. Gies, Gail H. Schaefer, Narsireddy Anugu, Fabien R. Baron, Cyprien Lanthermann, John D. Monnier, Stefan Kraus, Theo ten Brummelaar ยท 2025

W Serpentis is an eclipsing binary system and the prototype of the Serpentid class of variable stars. These are interacting binaries experiencing intense mass transfer and mass loss. However, the idenโ€ฆ

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Two types of domain walls in $\mathcal{N}=1$ super-QCD: how they are classified and counted

Shi Chen, Evgenii Ievlev, Mikhail Shifman ยท 2024

We study multiplicities and junctions of BPS domain walls interpolating between different chiral vacua in $\mathcal{N}=1$ supersymmetric QCD (SQCD) with the SU$(N)$ gauge group and a varying number ofโ€ฆ

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Multiplicity of Galactic Cepheids from long-baseline interferometry V. High-accuracy orbital parallax and mass of SU Cygni

A. Gallenne, N. R. Evans, P. Kervella, J. D. Monnier, C. R Proffitt, G. H. Schaefer, E. M. Winston, J. Kuraszkiewicz, A. Merand, G. Pietrzynski, W. Gieren, B. Pilecki, S. Kraus, J-B Le Bouquin, N. Anugu, T. ten Brummelaar, S. Chhabra, I. Codron, C. L. Davies, J. Ennis, T. Gardner, M. Gutierrez, N. Ibrahim, C. Lanthermann, D. Mortimer, B. R. Setterholm ยท 2024

Cepheid masses are particularly necessary to help solving the mass discrepancy, while independent distance determinations provide crucial test of the period-luminosity relation and Gaia parallaxes. Weโ€ฆ

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Physics Preprint PDF DOI

Visual Orbits of Wolf-Rayet Stars II: The Orbit of the Nitrogen-Rich WR Binary WR 138 measured with the CHARA Array

Amanda Holdsworth, Noel Richardson, Gail H. Schaefer, Jan J. Eldridge, Grant M. Hill, Becca Spejcher, Jonathan Mackey, Anthony F. J. Moffat, Felipe Navarete, John D. Monnier, Stefan Kraus, Jean-Baptiste Le Bouquin, Narsireddy Anugu, Sorabh Chhabra, Isabelle Codron, Jacob Ennis, Tyler Gardner, Mayra Gutierrez, Noura Ibrahim, Aaron Labdon, Cyprien Lanthermann, Benjamin R. Setterholm ยท 2024

Classical Wolf-Rayet stars are descendants of massive OB-type stars that have lost their hydrogen-rich envelopes, and are in the final stages of stellar evolution, possibly exploding as type Ib/c supeโ€ฆ

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Physics Preprint PDF DOI

Absolute Dimensions of the Interferometric Binary HD 174881: A Test of Stellar Evolution Models for Evolved Stars

Guillermo Torres (CfA), Andrew F. Boden (Caltech), John D. Monnier (U Michigan), Gerard T. van Belle (Lowell Obs.) ยท 2024

We report high-resolution spectroscopic monitoring and long-baseline interferometric observations with the PTI of the 215-day binary system HD 174881 (K1 II-III), composed of two giant stars. The systโ€ฆ

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On estimating the trace of quantum state powers

Yupan Liu, Qisheng Wang ยท 2024

We investigate the computational complexity of estimating the trace of quantum state powers $\text{tr}(\rho^q)$ for an $n$-qubit mixed quantum state $\rho$, given its state-preparation circuit of sizeโ€ฆ

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Physics Preprint PDF DOI

Visual Orbits of Wolf-Rayet Stars I: The Orbit of the dust-producing Wolf-Rayet binary WR\,137 measured with the CHARA Array

Noel D. Richardson, Gail H. Schaefer, Jan J. Eldridge, Rebecca Spejcher, Amanda Holdsworth, Ryan M. Lau, John D. Monnier, Anthony F. J. Moffat, Gerd Weigelt, Peredur M. Williams, Stefan Kraus, Jean-Baptiste Le Bouquin, Narsireddy Anugu, Sorabh Chhabra, Isabelle Codron, Jacob Ennis, Tyler Gardner, Mayra Gutierrez, Noura Ibrahim, Aaron Labdon, Cyprien Lanthermann, Benjamin R. Setterholm ยท 2024

Classical Wolf-Rayet stars are the descendants of massive OB stars that have lost their hydrogen envelopes and are burning helium in their cores prior to exploding as type Ib/c supernovae. The mechaniโ€ฆ

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