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๐Ÿ” vikram voleti ๐Ÿ“‚ Physics
Showing 2823 results for "vikram voleti" in Physics
Physics Preprint PDF DOI

A New Perspective on Galactic Evolution: Studying the Outskirts of the Abell S1063 Galaxy Cluster

L. Pecoraro, A. Mercurio, M.Annunziatella, M. D'Addona, R. Ragusa, G. Angora, M. Girardi, G. Granata, C. Grillo, L. Limatola, P. Rosati, P. Bergamini, G. Caminha, F. Getman, A. Grado, M. Meneghetti, E. Vanzella ยท 2026

Galaxy physical properties are influenced by their environments, but the processes responsible for mass and environmental quenching and structural transformations remain debated. Galaxy clusters are iโ€ฆ

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The SOXS Spectrograph Instrument Control Software

Davide Ricci, Bernardo Salasnich, Andrea Baruffolo, Jani Achren, Matteo Aliverti, Jose A. Araiza-Duran, Iair Arcavi, Laura Asquini, Federico Battaini, Sagi Ben-Ami, Alex Bichkovsky, Anna Brucalassi, Rachel Bruch, Lorenzo Cabona, Sergio Campana, Giulio Capasso, Enrico Cappellaro, Riccardo Claudi, Mirko Colapietro, Rosario Cosentino, Francesco D'Alessio, Paolo D'Avanzo, Sergio D'Orsi, Massimo Della Valle, Rosario Di Benedetto, Simone Di Filippo, Avishay Gal-Yam, Matteo Genoni, Marcos Hernandez Diaz, Ofir Hershko, Jari Kotilainen, Hanindyo Kuncarayakti, Marco Landoni, Gianluca Li Causi, Laurent Marty, Seppo Mattila, Matteo Munari, Luca Oggioni, Hector Perez Ventura, Giorgio Pariani, Giuliano Pignata, Kalyan Kumar Radhakrishnan Santhakumari, Stephen Smartt, Michael Rappaport, Marco Riva, Adam Rubin, Salvatore Savarese, Pietro Schipani, Salvatore Scuderi, Maximilian Stritzinger, Fabrizio Vitali, David Young, Ricardo Zanmar Sanchez, Gerard Zins ยท 2026

SOXS (Son Of X-Shooter) is a new spectrograph for the European Southern Observatory (ESO), recently installed at the New Technology Telescope (NTT) at the La Silla Observatory, Chile. The main instrumโ€ฆ

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Physics Preprint PDF DOI

The KMS and GNS Spectral Gap of Quantum Markov Semigroups

Melchior Wirth ยท 2026

We establish a relation between the exponential decay rates of quantum Markov semigroups with respect to different inner products. More precisely, it was conjectured by Fagnola, Poletti, Sasso and Umaโ€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

VLTI-GRAVITY observations of blazars

Talvikki Hovatta, Elina Lindfors, Heidi Korhonen, Preeti Kharb, Markus Wittkowski, Aaron Labdon, Tapio Pursimo, Kaj Wiik ยท 2026

Parsec-scale jets of blazars have so far been spatially resolved only in millimeter and submillimeter wavelengths, where very long baseline interferometry can be used to obtain milliarcsecond-scale imโ€ฆ

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NOEMA3D: Resolving radial gas flows in disk galaxies at z~1.1-1.6 with high-resolution CO observations

Jean-Baptiste Jolly, Linda J. Tacconi, Reinhard Genzel, Roberto Neri, Karl Schuster, Jianhang Chen, Natascha M. Forster Schreiber, Stavros Pastras, Letizia Scaloni, Giulia Tozzi, Capucine Barfety, Alberto Bolatto, Andreas Burker, Francoise Combes, Pierre Cox, Ric Davies, Frank Eisenhauer, Juan Manuel Espejo Salcedo, Rodrigo Herrera-Camu, Santi Garcia-Burillo, Tadayuki Kodama, Lilian Lee, Minju M. Lee, Daizhong Liu, Dieter Lutz, Giovanni Mazzolari, Thorsten Naab, Amit Nestor Shachar, Claudia Pulsoni, Alvio Renzini, Monica Rubio, Taro T. Shimizu, Amiel Sternberg, Eckhard Sturm, Hannah Ubler, Antonio Usero, Stijn Wuyts ยท 2026

We present NOEMA3D, a unique high-resolution study of purely molecular gas kinematics at $z \sim 1.1$ to 1.6, providing a dedicated view of cold gas dynamics at the late stages of the peak epoch of coโ€ฆ

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Physics Preprint PDF DOI

Molecular Clouds at the Edge of the Galaxy II. Physical properties and scaling relations

C. S. Luo, X. D. Tang, C. Henkel, Y. Sun, Y. Gong, X. W. Zheng, T. Liu, X. Lu, Y. P. Ao, X. P. Chen, D. L. Li, Y. X. He, K. Wang, J. W. Wu, J. Esimbek, J. J. Zhou, G. Wu, Y. X. Ma, W. A. Baan, J. J. Qiu, X. Zhao, J. S. Li, Q. Zhao, L. D. Liu, C. Y. Wang ยท 2026

The outer Galaxy presents an optimal setting for investigating molecular clouds and star formation in environments with low metallicity. A total of 72 Galactic edge clouds were surveyed using the CO\,โ€ฆ

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Fluctuations in Aharonov-Bohm Electrodynamics

F. Minotti, G. Modanese ยท 2026

We consider the application of the Fluctuation Dissipation Theorem (FDT) to the electrodynamics of Aharonov-Bohm (ABE), which differs from Maxwell's in that it allows for local non-conservation of chaโ€ฆ

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Physics Preprint PDF DOI

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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Wavelength-dependent photo-creep in halide perovskite single crystals

Ruitian Chen, Jincong Pang, Lizhong Lang, Jiaze Wu, Mingyu Xie, Shuo Yang, Kaiqi Qiu, Tobin Filleter, Kai Huang, Guangda Niu, Jiang Tang, Yu Zou ยท 2026

Halide perovskites are promising optoelectronic materials, but their time-dependent permanent deformation under illumination (i.e., photo-creep) is poorly understood, limiting their mechanical stabiliโ€ฆ

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Physics Preprint PDF DOI

Evidence of Enhanced Ionization in Protostellar Envelopes

Kamber R. Schwarz, S. Maret, M. R. A. Wells, C. Gieser, A. Belloche, P. Andre, C. Codella ยท 2026

Ionization is a major driver of both physical and chemical evolution in protostellar systems. Recent observations reveal substantial chemical processing in protoplanetary disks by the time the surrounโ€ฆ

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Variational Iterative Rotation Algorithm: Combinatorial Optimization with Classical Kicked Tops

Flaviano Morone, Andrew D. Kent, Dries Sels ยท 2026

We investigate a classical formulation of the Quantum Approximate Optimization Algorithm (QAOA), realized as a Hamiltonian dynamical system of classical kicked tops, which we call the Variational Iterโ€ฆ

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Confinement in Holographic Theories at Finite Theta

Rashmish K. Mishra ยท 2026

A strongly coupled confining gauge theory with a non-zero vacuum angle undergoing a deconfinement to confinement phase transition is studied in the holographic gravitational description. A simplified โ€ฆ

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Magnetic-monopole resummation justifies perturbatively calculated collider production cross sections

Jean Alexandre, Nick E. Mavromatos, Vasiliki A. Mitsou, Emanuela Musumeci ยท 2026

A one-loop resummation scheme, inspired by Dyson-Schwinger (DS) formalism of strongly coupled quantum field theories, is applied to spin-1/2 magnetic monopoles (MMs), in the context of an effective fiโ€ฆ

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Ultraviolet variability in Radio-Loud Active Galactic Nuclei observed by UVIT onboard AstroSat

M. Reshma, C. S. Stalin, Amit Kumar Mandal, S. B. Gudennavar, Senorita Benedict, Prajwel Joseph ยท 2026

Radio-loud active galactic nuclei (AGN) are among the most luminous objects in the Universe, emitting radiation from low-energy radio waves to high energy $\gamma$-rays. They are well known to exhibitโ€ฆ

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Physics Preprint PDF DOI

SIMTERFERE: An optical interferometry simulator for quantifying the coherent flux stability of VLTI/GRAVITY+. Reaching per mill stability: Application to exoplanet spectroscopy

J. R. Sauter, A. von Stauffenberg, G. Bourdarot, W. Brandner, F. Eisenhauer, L. Kreidberg, L. Labadie, S. Scheithauer, D. Trevascus, R. van Boekel ยท 2026

The implementation of the GRAVITY+ Adaptive Optics (GPAO) system at VLTI enables unprecedented sensitivity and stability in optical interferometry. This allows high-precision characterization of direcโ€ฆ

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IRAM 04191+1522: a compact proto-brown dwarf binary candidate

N. Huelamo, I. de Gregorio-Monsalvo, Aina Palau, C. Carrasco-Gonzalez, A. Ribas, H. Bouy, R. Pandey, D. Barrado, N. Otten, V.D. Ivanov, M.F. Sterzik, M. Dunham, L. A. Zapata, E. Pantin, E. Macias ยท 2026

Very low-luminosity objects in nearby star-forming regions have been identified as promising proto-brown dwarf candidates. The study of their multiplicity can shed light on the dominant formation mechโ€ฆ

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Nonequilibrium assembly of Lennard-Jones particles on a sphere

Ivan Yu. Golushko, Olga V. Konevtsova, Daria S. Roshal, Sergei B. Rochal ยท 2026

Studying physical mechanisms and common geometric principles underlying known spherical packings is crucial for rational design of synthetic nanocontainers. Here we model the growth of small sphericalโ€ฆ

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AstroSat-UVIT observations of a possibly interacting pair of galaxies in HCG 77

Anshul Srivastava, Harvinder K. Jassal, Mamta Gulati, Kulinder P. Singh ยท 2026

We aim to study star-forming regions and the spectral energy distribution of two possibly interacting galaxies, PGC 56121 and PGC 56125, in the Hickson Compact Group 77. We utilized the far-ultravioleโ€ฆ

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Effects of Rim Fluctuations in Classical Nucleation Theory of Virus Capsids

Alexander Bryan Clark, Paul van der Schoot, Henri Orland, Roya Zandi ยท 2026

Most spherical viruses exhibit icosahedral symmetry, yet the growth of viral shells remains poorly understood due to the short lifetimes and broad size distribution of assembly intermediates. Classicaโ€ฆ

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