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๐Ÿ” niraj dayama ๐Ÿ“‚ Physics
Showing 522 results for "niraj dayama" in Physics
Physics Preprint PDF DOI

A note on complete gauge-fixing and the constraint algebra

Ganga Singh Manchanda ยท 2026

The admissibility of a gauge-fixing is governed by the invertibility of $\Delta=\{\sigma^a,\gamma_b\}$ where $\sigma^a$ are gauge-fixing conditions and $\gamma_b$ are independent first-class constrainโ€ฆ

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Distribution function-based modelling of discrete kinematic datasets, in application to the Milky Way nuclear star cluster

Eugene Vasiliev, Anja Feldmeier-Krause, Mattia C. Sormani ยท 2026

We present a method for constructing dynamical models of stellar systems described by distribution functions and constrained by discrete-kinematic data. We implement various improvements compared to eโ€ฆ

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Constraining the Galactic bar and spiral pattern speeds with the Hyades tidal stream

Zi-yi Zhou, Long Wang, Tereza Jerabkova, Zhenghao He ยท 2026

We present a suite of direct $N$-body simulations of the Hyades open cluster and its tidal stream in a Milky Way potential that includes a rotating bar and spiral arms. Using the high-resolution code โ€ฆ

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A Dayem Loop Qubit Based on Interfering Superconducting Nanowires

Cliff Sun, Alexey Bezryadin ยท 2026

We propose a qubit design based on two parallel superconducting nanowires (i.e., a "Dayem loop qubit"). The inclusion of two nanowires instead of one leads to the Little-Parks effect, which provides aโ€ฆ

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Quantum and Classical mechanics vs QFT

G.E. Volovik ยท 2026

15 years ago Dmitry Diakonov wrote the paper "Towards lattice-regularized Quantum Gravity", arXiv:1109.0091. In his approach, gravity with metric and tetrads arise from pre-geometric quantum fields leโ€ฆ

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Dynamical Formation of Self-Similar Wormholes

Yasutaka Koga, Ryota Maeda, Daiki Saito, Daisuke Yoshida ยท 2026

We study spherically symmetric, self-similar wormhole solutions supported by colliding streams of negative-energy null dust, and their dynamical formation. Under the assumption of self-similarity, theโ€ฆ

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Optical Thermodynamics Beyond the Weak Nonlinearity Limit

Emily Kabat, Shrohan Mohapatra, P.G. Kevrekidis, Tsampikos Kottos ยท 2026

Optical thermodynamics has recently emerged as a theoretical framework describing a Rayleigh-Jeans (RJ) modal power distribution of multimoded nonlinear photonic circuits. However, its applicability iโ€ฆ

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A New Torus Generator for AGAMA

James Binney, Thomas J Wright, Eugene Vasiliev ยท 2025

Code is presented that computes and exploits orbital tori for any axisymmetric gravitational potential. The code is a development of the AGAMA software package for action-based galaxy modelling and caโ€ฆ

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A New Definition of Horndeski Theory and the Possibility of Multiple Scalar Field Extensions

Tomoki Katayama ยท 2025

In the single-field case, Horndeski provides the most general scalar-tensor theory with second-order field equations. By contrast, systematic multi-field extensions remain incomplete: while the generaโ€ฆ

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Effects of crystal field and momentum-based frustrated exchange interactions on multiorbital square skyrmion lattice

Yan S. Zha, Satoru Hayami ยท 2025

Motivated by recent theoretical predictions of a square-shaped skyrmion lattice (S-SkL) in centrosymmetric tetragonal Ce-based magnets [Yan Zha and Satoru Hayami, \href{https://journals.aps.org/prb/abโ€ฆ

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Keck Observatory as an HWO Testbed: validating wavefront sensing and control schemes on a large segmented aperture in parallel with high-contrast science

Maissa Salama, Rebecca Jensen-Clem, Mahawa Cisse, J. Kent Wallace, Mitchell Troy, Laurent Pueyo, Charlotte Guthery, Antonin Bouchez, Vincent Chambouleyron ยท 2025

Exoplanet direct imaging allows us to directly probe and characterize an exoplanet's atmosphere, searching for signs of life in its atmospheric signatures. Directly imaging an Earth-like planet aroundโ€ฆ

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DAMA/LIBRA and dark matter: decisive tension or contrived cancellation

Giorgio Busoni, Jonathan M. Cornell, Will Handley, Felix Kahlhoefer, Anders Kvellestad, Masen Pitts, Lauren Street, Aaron C. Vincent, Martin White ยท 2025

We assess the tension between DAMA/LIBRA and the latest dark matter annual modulation results from the ANAIS-112 and COSINE-100 NaI experiments, under a range of hypotheses ranging from physical to geโ€ฆ

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Additional Evidence for the Existence of a Primordial Disk System

Shuai Xu, Haibo Yuan, Bowen Huang, Timothy C. Beers, Yang Huang, Maosheng Xiang, Kai Xiao, Jihye Hong, Young Sun Lee, Wuming Yang ยท 2025

The origin of very metal-poor (VMP; [Fe/H] $\leq -2.0$) stars on planar orbits has been the subject of great attention since their first discovery. However, prior to the release of the Gaia BP/RP (XP)โ€ฆ

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COSINUS -- a model-independent challenge of the DAMA/LIBRA dark matter claim with cryogenic NaI detectors operated in a new low-background facility

G. Angloher, M. R. Bharadwaj, A. Bohmer, M. Cababie, I. Colantoni, I. Dafinei, N. Di Marco, C. Dittmar, L. Einfalt, F. Ferella, F. Ferroni, S. Fichtinger, A. Filipponi, M. Friedl, L. Gai, M. Gapp, M. Heikinheimo, K. Heim, M. N. Hughes, K. Huitu, M. Kellermann, R. Maji, M. Mancuso, L. Pagnanini, F. Petricca, S. Pirro, F. Probst, G. Profeta, A. Puiu, F. Reindl, K. Schaffner, J. Schieck, P. Schreiner, C. Schwertner, K. Shera, M. Stahlberg, A. Stendahl, M. Stukel, C. Tresca, S. Yue, V. Zema, Y. Zhu, N. Zimmermann (The COSINUS Collaboration) ยท 2025

Low-temperature detectors are a powerful technology for dark matter search, offering excellent energy resolution and low energy thresholds. COSINUS is the only experiment that combines scintillating sโ€ฆ

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Calibrating the photometric performance of a high-time-resolution photon-counting imager for optical astronomy

Mana Hasebe, Takeshi Nakamori, Kazuaki Hashiyama, Anju Sato, Miu Maeshiro, Rin Sato, Masayoshi Shoji, Masaru Kino, Dai Takei, Tomohiro Sato, Kazuki Ueno ยท 2025

Optical observations with high time resolution are essential for understanding the origin of sub-millisecond timescale astronomical phenomena, including giant radio pulses from the Crab Pulsar. We havโ€ฆ

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Search for Magnetic Monopoles with the Complete ANTARES Dataset

A. Albert, S. Alves, M. Andre, M. Ardid, S. Ardid, J.-J. Aubert, J. Aublin, B. Baret, S. Basa, Y. Becherini, B. Belhorma, F. Benfenati, V. Bertin, S. Biagi, J. Boumaaza, M. Bouta, M.C. Bouwhuis, H. Branzas, R. Bruijn, J. Brunner, J. Busto, B. Caiffi, D. Calvo, S. Campion, A. Capone, F. Carenini, J. Carr, V. Carretero, T. Cartraud, S. Celli, L. Cerisy, M. Chabab, R. Cherkaoui El Moursli, T. Chiarusi, M. Circella, J.A.B. Coelho, A. Coleiro, R. Coniglione, P. Coyle, A. Creusot, A. F. Diaz, B. De Martino, C. Distefano, I. Di Palma, C. Donzaud, D. Dornic, D. Drouhin, T. Eberl, A. Eddymaoui, T. van Eeden, D. van Eijk, S. El Hedri, N. El Khayati, A. Enzenhofer, P. Fermani, G. Ferrara, F. Filippini, L. Fusco, S. Gagliardini, J. Garcia-Mendez, C. Gatius Oliver, P. Gay, N. Geisselbrecht, H. Glotin, R. Gozzini, R. Gracia Ruiz, K. Graf, C. Guidi, L. Haegel, H. van Haren, A.J. Heijboer, Y. Hello, L. Hennig, J.J. Hernandez-Rey, J. Hossl, F. Huang, G. Illuminati, B. Jisse-Jung, M. de Jong, P. de Jong, M. Kadler, O. Kalekin, U. Katz, A. Kouchner, I. Kreykenbohm, V. Kulikovskiy, R. Lahmann, M. Lamoureux, A. Lazo, D. Lefevre, E. Leonora, G. Levi, S. Le Stum, S. Loucatos, J. Manczak, M. Marcelin, A. Margiotta, A. Marinelli, J.A. Martinez-Mora, P. Migliozzi, A. Moussa, R. Muller, S. Navas, E. Nezri, B. 'O Fearraigh, E. Oukacha, A.M. Paun, G.E. Pavalas, S. Pena-Martinez, M. Perrin-Terrin, P. Piattelli, C. Poire, V. Popa, T. Pradier, N. Randazzo, D. Real, G. Riccobene, A. Romanov, A. Sanchez Losa, A. Saina, F. Salesa Greus, D. F. E. Samtleben, M. Sanguineti, P. Sapienza, F. Schussler, J. Seneca, M. Spurio, Th. Stolarczyk, M. Taiuti, Y. Tayalati, B. Vallage, G. Vannoye, V. Van Elewyck, S. Viola, D. Vivolo, J. Wilms, S. Zavatarelli, A. Zegarelli, J.D. Zornoza, J. Zuniga ยท 2025

This study presents a novel search for magnetic monopoles using data collected over a 14 year period (2008-2022) by the ANTARES neutrino telescope. The interaction of magnetic monopoles with matter waโ€ฆ

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commensurability: a Python package for classifying astronomical orbits based on their toroid volume

Subhadeep Sarkar, Michael S. Petersen ยท 2025

As a star orbits the center of its host galaxy, the trajectory is encompassed within a 3D toroid. The orbit probes all points in this toroid, unless its orbital frequencies exhibit integer ratios (comโ€ฆ

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Physics Preprint PDF DOI

COSINUS model-independent sensitivity to the DAMA/LIBRA dark matter signal

G. Angloher, M. R. Bharadwaj, A. Bohmer, M. Cababie, I. Colantoni, I. Dafinei, N. Di Marco, C. Dittmar, L. Einfalt, F. Ferella, F. Ferroni, S. Fichtinger, A. Filipponi, T. Frank, M. Friedl, Z. Ge, M. Heikinheimo, M. N. Hughes, K. Huitu, M. Kellermann, R. Maji, M. Mancuso, L. Pagnanini, F. Petricca, S. Pirro, F. Probst, G. Profeta, A. Puiu, F. Reindl, K. Schaffner, J. Schieck, P. Schreiner, C. Schwertner, K. Shera, M. Stahlberg, A. Stendahl, M. Stukel, C. Tresca, F. Wagner, S. Yue, V. Zema, Y. Zhu, The COSINUS Collaboration ยท 2025

COSINUS is a dark matter direct detection experiment using NaI crystals as cryogenic scintillating calorimeters. If no signal is observed, this will constrain the dark matter scattering rate in sodiumโ€ฆ

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AGN outflows and their properties in Mrk 766 as revealed by KOOLS-IFU on the Seimei Telescope

Kyuseok Oh, Yoshihiro Ueda, Satoshi Yamada, Yoshiki Toba, Keisuke Isogai, Atsushi Tanimoto, Shoji Ogawa, Ryosuke Uematsu, Yuya Nakatani, Kanta Fujiwara, Yuta Okada, Kazuya Matsubayashi, Kenta Setoguchi ยท 2025

We present the emission-line flux distributions and their ratios, as well as the gas outflow features, of the innermost 2 kpc region of the type 1 Seyfert galaxy Mrk 766, using the Kyoto Okayama Opticโ€ฆ

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Prompt and Conventional High-Energy Muon Spectra from a full Monte Carlo Simulation via $\texttt{CORSIKA7}$

Ludwig Neste, Pascal Gutjahr, Mirco Hunnefeld, Jean-Marco Alameddine, Wolfgang Rhode, Julia Becker Tjus, Felix Riehn, Kevin Kroninger, Johannes Albrecht ยท 2025

Extensive air showers produce high-energy muons that can be utilized to probe hadronic interaction models in cosmic ray interactions. Most muons originate from pion and kaon decays, called $\textit{coโ€ฆ

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