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๐Ÿ” arindam mitra ๐Ÿ“‚ Physics
Showing 825 results for "arindam mitra" in Physics
Physics Preprint PDF DOI

Holographic realization of higher-spin Carrollian free fields

Ethan D'Arcy, Arnaud Delfante, Stefan Fredenhagen ยท 2026

We provide a holographic bulk realization of Carrollian free-field structures arising in three-dimensional asymptotically flat (higher-spin) gravity. We construct a class of boundary conditions that gโ€ฆ

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Physics Preprint PDF DOI

On matrix Lax representations for (1+1)-dimensional evolutionary differential-difference equations

Sergei Igonin ยท 2026

Differential-difference matrix Lax representations (Lax pairs), gauge transformations, and discrete Miura-type transformations (MTs) belong to the main tools in the theory of (nonlinear) integrable diโ€ฆ

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Physics Preprint PDF DOI

VLTI-GRAVITY measurements of cool evolved stars: II. Pulsation properties and mass-loss process of the Mira star R Car and the red supergiant VX Sgr

D. Jadlovsky, M. Wittkowski, A. Chiavassa, K. Kravchenko, B. Freytag, S. Hofner, J. Krticka, C. Paladini, G. Rau, M. Broz, T. Granzer, M. Weber ยท 2026

The mass-loss process of red supergiant (RSG) and asymptotic giant branch (AGB) stars and its relation to variability is poorly constrained. We study two evolved stars, the Mira-type AGB star R Car anโ€ฆ

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Physics Preprint PDF DOI

Mid-infrared JWST spectra of carbon stars in the Large Magellanic Cloud

G. C. Sloan, B. Aringer, Kathleen E. Kraemer, J. Cami, K. Eriksson, S. Hoefner, K. Justtanont, E. Lagadec, Paola Marigo, M. Matsuura, I. McDonald, E. J. Montiel, R. Sahai, A. A. Zijlstra ยท 2026

Mid-infrared spectra from the Medium Resolution Spectrometer on the James Webb Space Telescope have revealed the molecular chemistry of carbon stars in the Large Magellanic Cloud with better resolutioโ€ฆ

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Physics Preprint PDF DOI

Revisiting the Milky Way stellar long bar and the 3 kpc arm

M. Lopez-Corredoira, W. Wu, H.-F. Wang, F. Garzon ยท 2026

CONTEXT. One of the most difficult and unexplored regions of the Milky Way is the highly extincted in-plane central region within the Galactic coordinates $10^\circ \lesssim |\ell |\lesssim 30^\circ $โ€ฆ

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Effect of machine arithmetic errors for multi-turn invariant curve destruction

David Nikitin, Nataliya Stankevich ยท 2026

Using the example of three-dimensional Mira map, it is shown that the destruction of a multi-turn invariant curve can occur through the appearance of local multiple bends. It was found that, dependingโ€ฆ

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Physics Preprint PDF DOI

Photometric and Spectral Evolution of the Symbiotic Nova HM Sagittae since 2003

N.P. Ikonnikova, V.I. Shenavrin, G.V. Komissarova, M.A. Burlak, A.V. Dodin ยท 2026

We present photometric and spectral monitoring of the symbiotic system HM Sge, which consists of a Mira variable with a dust shell and a hot white dwarf ionizing the surrounding gaseous nebula. The syโ€ฆ

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Spectroscopic study of five Mira stars

David Boyd ยท 2026

Mira stars are popular with amateur astronomers because they are generally bright and their pulsations produce large changes in brightness. This also means they are eminently suitable to study using sโ€ฆ

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Is Mira B a low mass white dwarf?

R. K. Zamanov, V. Irincheva, B. Spassov, A. Kurtenkov, D. Marchev, M. Minev, M. F. Bode, L. Dankova, B. Borisov, M. Dechev, G. Yordanova ยท 2026

We report photometric observations in Johnson B and V bands of the short term variability (flickering) of Mira (omicron Ceti). The observations were performed during 7 nights in the period August - Ocโ€ฆ

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Size-Dependent Properties of Miura-ori Tessellations

Chaewon Baek, Tomohiro Tachi, Jinkyu Yang, Hiromi Yasuda ยท 2026

We investigate the size-dependent behavior of Miura-ori-based origami tessellations by changing the number of origami unit cells. For large tessellations, the Miura-ori sheet generally exhibits a negaโ€ฆ

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Variable Red Giants Exploration with MASTER Robotic Net: Main Algorithms and Study of Three Mira-type Targets

Alexander N. Tarasenkov, Vladimir M. Lipunov, Artem S. Kuznetsov, Gleb A. Antipov, Pavel V. Balanutsa, Nataly V. Tyurina, Yakov Yu. Kechin ยท 2026

We are discussing the capabilities of MASTER network of robotic telescopes to study variable red giant stars. We report the discovery and present archival light curves for three optical transients, coโ€ฆ

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A homogeneous view of asymptotic giant branch carbon stars as seen by Gaia

Alessio Liberatori, Despina Hatzidimitriou, Konstantinos Antoniadis, Giada Pastorelli, Michele Trabucchi, M.A.T. Groenewegen, Diego Bossini, Leo Girardi, Paola Marigo, Alessandro Bressan, Ioannis N. Kallimanis, Guglielmo Costa, Vasileios Katsis, Georgios Vasilopoulos, Stamatis Chatzipetros ยท 2026

Carbon stars on the asymptotic giant branch are major contributors to galactic dust enrichment, with gas mass-loss rates up to 1e-4 Msun/yr. We present a homogeneous spectral energy distribution analyโ€ฆ

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A surprisingly large asymmetric ejection from Mira A

T. Khouri, W. H. T. Vlemmings, D. A. Raudales Oseguera, D. Tafoya, H. Olofsson, C. Paladini M. Maercker, M. Saberi, P. Gorai, T. Danilovich ยท 2026

Stars with masses between roughly 1 and 8~$M_\odot$ end their lives on the asymptotic giant branch (AGB), when intense mass loss takes place. The outflows are generally accepted to be driven by radiatโ€ฆ

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The Role of Long Period Variable Stars in Observational Astrophysics

Dorota M. Skowron, Igor Soszynski ยท 2026

Long-period variables (LPVs) are evolved red giant and supergiant stars whose pulsations provide unique insights into late stages of stellar evolution and serve as essential tools in modern astrophysiโ€ฆ

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Bihamiltonian tests for integrable systems associated to rank-$1$ F-CohFTs

Alexandr Buryak, Jianghao Xu, Di Yang ยท 2026

Double ramification (DR) hierarchies associated to rank-$1$ F-CohFTs are important integrable perturbations of the Riemann--Hopf hierarchy. In this paper, we perform bihamiltonian tests for these DR hโ€ฆ

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Discretization of the Mikhailov model

Song-lin Zhao, Xiao-gang Mu, Da-jun Zhang ยท 2026

In this paper the Mikhailov model is discretized by means of the Cauchy matrix approach. A pair of discrete Miura transformations are constructed. The discrete Mikhailov model is a coupled system, in โ€ฆ

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Magnetically Induced Transparency-Absorption and Normal-Anomalous Dispersion Characteristics of ${}^{87}\text{Rb}$ Medium or Any J-Type Configuration Atomic Vapors Subject to a Vector Magnetic Field and a Weak Resonant Pump

Hayk L. Gevorgyan ยท 2026

We have developed an analytical framework for magnetically induced transparency-absorption (MITA) and normal-anomalous dispersion (MINAD) in a weakly driven ${}^{87}\text{Rb}$ vapor, or any J-type thrโ€ฆ

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A phoenix rises from the ashes: WOH G64 is still a red supergiant, for now

Jacco Th. van Loon (Keele University, UK), Keiichi Ohnaka (Universidad Andres Bello, Chile) ยท 2026

For a long time, WOH G64 was known as the most extreme red supergiant outside our Galaxy. However, in a matter of years it has faded, its pulsations have become suppressed and the spectrum has become โ€ฆ

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Changes in R Leonis over Two Centuries: Period evolution and dust shell development

Mike Goldsmith ยท 2025

The AAVSO-based historical light curve of the oxygen-rich Mira variable R Leonis is used to determine and analyse the properties of the star's maxima and minima. The pulsation period is found to have โ€ฆ

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An integrable hierarchy associated with loop extension of $\mathbb{Z}_2^2$-graded $\mathfrak{osp}(1|2)$

N. Aizawa, I. Fujii, R. Ito ยท 2025

A hierarchy of $\mathbb{Z}_2^2$-graded integrable equations is constructed using the loop extension of the $\mathbb{Z}_2^2$-graded Lie superalgebra $\mathfrak{osp}(1|2)$. This hierarchy includes $\matโ€ฆ

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