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๐Ÿ” hadi daneshmand ๐Ÿ“‚ Physics
Showing 132 results for "hadi daneshmand" in Physics
Physics Preprint PDF DOI

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

Machine learning for understanding pulsating stars I: the non-linear phenomenon in {\delta} Scuti stars

J.R. Rodon, J. Pascual-Granado, M. Lares-Martiz, M. Rodriguez Sanchez, C. Roche ยท 2026

$\delta$ Scuti stars are pulsating variable stars that exhibit both radial and non-radial pulsations, making them key objects for understanding stellar evolution and internal structures. The current cโ€ฆ

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Physics Preprint PDF DOI

BE Lyncis is not a Black Hole Binary: Lessons From Gaia and Hipparcos Astrometry

Pranav Nagarajan, Kareem El-Badry, Thomas J. Maccarone, Giuliano Iorio, Sara Rastello, Johanna Muller-Horn ยท 2026

BE Lyncis (BE Lyn) is a well-studied high-amplitude $\delta$ Scuti variable star (HADS). Recently, Niu et al. (2026) analyzed a 39-year baseline of times of maximum light of BE Lyn, reporting that it โ€ฆ

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Physics Preprint PDF DOI

Comparison of Static and Evolving Potentials in the Orbital Dynamics of Globular Clusters in the Central Region of the Galaxy

Anisa Bajkova, Anton Smirnov, Vadim Bobylev ยท 2026

A comparative analysis of the dynamics of the orbital motion (regular or chaotic) of 45 globular clusters in the central region of the Galaxy with a radius of 3.5 kpc is carried out. The static and evโ€ฆ

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Physics Preprint PDF DOI

Pulsation Mode Identification and Classification of 46 High-Amplitude $\delta$ Scuti Stars from 50 Candidates with TESS observations

Taozhi Yang, Zhaoyu Zuo ยท 2025

Asteroseismic modelling of high-amplitude $\delta$ Scuti (HADS) variables critically depends on their accurate classification, which provides robust constraints on stellar physical parameters. As a foโ€ฆ

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Physics Preprint PDF DOI

A complex network approach to TESS light curves of $\delta$ Sct stars

E. Ziaali, S. de Franciscis, J. Pascual-Granado, N. Alipour, H. Safari, R. Garrido, J. Rodriguez-Gomez ยท 2025

By using the horizontal visibility algorithm, the TESS light curves of 69 delta Sct stars are mapped to undirected horizontal visibility graphs (HVGs), where the graph nodes represent the light curve โ€ฆ

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Physics Preprint PDF DOI

Bridging doubly heavy tetraquark mass spectrum with heavy baryons utilizing heavy antiquark-diquark symmetry

Liu-Yu Zhang, Tian-Wei Wu, Yong-Liang Ma ยท 2025

Motivated by the observation of the doubly charmed tetraquark $T_{cc}(3875)^+$, we present a systematic study of double heavy tetraquarks ($T_{QQ'\bar{q}\bar{q}'}$) using heavy antiquark-diquark symmeโ€ฆ

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Physics Preprint PDF DOI

Precise Asteroseismology of the High-amplitude Delta Scuti Star EH Librae, an AE UMa Analogue in the Hertzsprung Gap

Xiran Xie, Jianning Fu, Gang Meng, Lester Fox Machado, Raul Michel, Huifang Xue, Nian Liu, Zhongyang Liu, Jie Su, Mingfeng Qin ยท 2025

A subclass of intermediate mass variables Delta Scuti stars, known as High-amplitude Delta Scuti (HADS) stars, exhibits pronounced radial pulsations with high amplitudes. The ground-based and space-baโ€ฆ

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Physics Preprint PDF DOI

An Algorithm for Automated Extraction of Resonance Parameters from the Stabilization Method

Johanna Langner, Anjan Sadhukhan, Jayanta K. Saha, Henryk A. Witek ยท 2025

The application of the stabilization method [A.~U.\ Hazi and H.~S.\ Taylor, Phys.~Rev.~A {\bf 1}, 1109 (1970)]) to extract accurate energy and lifetimes of resonance states is challenging: The processโ€ฆ

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Physics Preprint PDF DOI

Beyond Point Particles -- Extended Structural Dynamics and the H Theorem

Patrick BarAvi ยท 2025

We propose an extended structural dynamics framework that enriches classical mechanics by treating particle orientation and internal structure as fundamental phase-space coordinates. This extension prโ€ฆ

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Physics Preprint PDF DOI

Discovery of resonating integration modes in triple-mode high-amplitude $\delta$ Scuti stars: A new evolutionary phase indicator

Jia-Shu Niu, Hui-Fang Xue ยท 2025

High-amplitude $\delta$ Scuti stars (HADS) that pulsate in their first three radial modes are rare in current samples. Here, we analyse five such triple-mode HADS observed by the Transiting Exoplanet โ€ฆ

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Physics Preprint PDF DOI

Period Variation Rates of Four Radial Single-Mode High-Amplitude Delta Scuti Stars

Tian-Fang Ma, Jia-Shu Niu, Hui-Fang Xue ยท 2025

In this work, we present a study on the long time-scale period variations of four single-mode high-amplitude delta Scuti stars (HADS) via the classical $O-C$ analysis. The target HADS are (i) XX Cygniโ€ฆ

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Physics Preprint PDF DOI

The HADS Star CSS_J102714.3+205943: a Component of a Binary System with an Elliptic Orbit?

Maksym Yu. Pyatnytskyy, Ivan L. Andronov ยท 2025

We analyzed period changes of the high-amplitude Delta Scuti variable star CSS_J102714.3+205943 for about 20 years, utilizing data from the automated sky surveys along with our own observations. With โ€ฆ

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Physics Preprint PDF DOI

New beyond-Voigt line-shape profile recommended for the HITRAN database

P. Wcis{l}o, N. Stolarczyk, M. S{l}owinski, H. Jozwiak, D. Lisak, R. Ciury{l}o, A. Cygan, F. Schreier, C. D. Boone, A. Castrillo, L. Gianfrani, Y. Tan, S-M. Hu, E. Adkins, J. T. Hodges, H. Tran, H. N. Ngo, J.-M. Hartmann, S. Beguier, A. Campargue, R. J. Hargreaves, L. S. Rothman, I. E. Gordon ยท 2025

Parameters associated with the collisional perturbation of spectral lines are essential for modeling the absorption of electromagnetic radiation in gas media. The HITRAN molecular spectroscopic databaโ€ฆ

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Physics Preprint PDF DOI

2024 'Key Reflections' on the 1824 Sadi Carnot's 'Reflexions' and 200 Year Legacy

Milivoje M. Kostic ยท 2025

This author is not a philosopher nor historian of science, but an engineering thermodynamicist. In that regard and in addition to various philosophical "why & how" treatises and existing historical anโ€ฆ

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Search for Higgs boson decays into a pair of pseudoscalar particles in the $\gamma\gamma\tau_{\text{had}}\tau_{\text{had}}$ final state using $pp$ collisions at $\sqrt{s}=13$ TeV with the ATLAS detector

ATLAS Collaboration ยท 2024

A search for exotic decays of the 125 GeV Higgs boson into a pair of new spin-0 particles, $H \to aa$, where one decays into a photon pair and the other into a $\tau$-lepton pair, is presented. Hadronโ€ฆ

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Physics Preprint PDF DOI

Signature of high-amplitude pulsations in seven Delta Sct stars via TESS observations

Fatemeh Vasigh, Elham Ziaali, Hossein Safari ยท 2024

The regular behavior of the pulsations of high-amplitude Delta Sct (HADS) stars gives a greater chance to investigate the interiors of stars. We analyzed seven HADS stars showing peak-to-peak amplitudโ€ฆ

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Physics Preprint PDF DOI

Exploring the unexpected: Disharmonized harmonic pulsation modes in high-amplitude $\delta$ Scuti stars

Hui-Fang Xue, Jia-Shu Niu ยท 2024

Harmonics are a ubiquitous feature across various pulsating stars. They are traditionally viewed as mere replicas of the independent primary pulsation modes and have thus been excluded from asteroseisโ€ฆ

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Physics Preprint PDF DOI

Bayesian Black Hole Photogrammetry

Dominic O. Chang, Michael D. Johnson, Paul Tiede, Daniel C. M. Palumbo ยท 2024

We propose a simple, analytic dual-cone accretion model for horizon scale images of the cores of Low-Luminosity Active Galactic Nuclei (LLAGN), including those observed by the Event Horizon Telescope โ€ฆ

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Physics Preprint PDF DOI

Recurrent Nova V2487 Oph Had Superflares in 1941 and 1942 With Radiant Energies 10$^{42.5\pm1.6}$ Ergs

Bradley E. Schaefer (Louisiana State University) ยท 2024

V2487 Ophiuchi (V2487 Oph) is a recurrent nova with classical nova eruptions in 1900 and 1998, and it is also the most extreme known superflare star. These superflares are roughly-hour-long flares witโ€ฆ

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