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๐Ÿ” gregory weitzner ๐Ÿ“‚ Physics
Showing 646 results for "gregory weitzner" in Physics
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BMS transformed Quantum String Dynamics near a Black Hole

Nihar Ranjan Ghosh, Malay K. Nandy ยท 2026

Asymptotic symmetries are expected to leave subtle but physically meaningful imprints on quantum probes of gravity, yet their manifestation in near-horizon dynamics remains incompletely understood. Weโ€ฆ

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Quadrupolar bremsstrahlung waveform at the third-and-a-half post-Newtonian accuracy

Donato Bini, Thibault Damour, Andrea Geralico ยท 2026

We study the quadrupolar part of the gravitational waveform $h_{ij}$ (encoded in the helicity-($-2)$ radiative quadrupole moment $U_2 = \frac{1}{2!} \bar m^{i} \bar m^{j } U_{i j} \in\frac{R}{4G} \barโ€ฆ

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Asymptotic Symmetries of the Holst Action at Spatial Infinity: Including Supertranslations

Sepideh Bakhoda, Hongguang Liu ยท 2026

We investigate the asymptotic symmetries of General Relativity at spatial infinity within the first-order formalism described by the Holst action. Employing the covariant phase space method, we proposโ€ฆ

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High energy scattering and null strings

Arjun Bagchi, Sachin Grover, Sharang Rajesh Iyer, Amartya Saha ยท 2026

We propose an instrinsic worldsheet description of the ultra-high energy regime of string scattering based on worldsheet symmetries. At very high energies, the fundamental string becomes tensionless aโ€ฆ

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Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge

Aniket Khairnar, Leo C. Stein, Michael Boyle, Nils Deppe, Lawrence E. Kidder, Keefe Mitman, Jordan Moxon, Kyle C. Nelli, William Throwe, Nils L. Vu ยท 2026

The Bondi--van der Burg--Metzner--Sachs (BMS) frame of gravitational waves produced by numerical relativity (NR) simulations is crucial for building accurate waveform models. A proper comparison of NRโ€ฆ

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Isomorphism between the local Poincare generalized translations group and the group of spacetime transformations (x LB1)4

Alcides Garat ยท 2026

We will prove that there is a direct relationship between the Poincare subgroup of translations, and the group of tetrad transformations LB1 introduced in a previous manuscript. LB1 is the group compoโ€ฆ

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Shaving off soft hairs and the black hole image memory effect

Shaoqi Hou, Zong-Hong Zhu ยท 2026

Soft hairs of black holes are the Noether charges associated to the generalized Bondi-Metzner-Sachs symmetries. In this work, the images of soft-haired Kerr black holes were studied. For an eternal blโ€ฆ

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Magnetoacoustic Shocks and Spectropolarimetric Signals in He I 10830 {\AA}

Hirdesh Kumar, Tobias Felipe, Christoph Kuckein, S. J. Gonzalez Manrique, A. Asensio Ramos ยท 2026

Umbral flashes are manifestations of magnetoacoustic shocks in the solar chromosphere. These phenomena are thought to influence the evolution of chromospheric umbral magnetic fields. However, the impaโ€ฆ

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Constraints on BMS Transformations via Energy Conditions and implications on black hole geometry

Nihar Ranjan Ghosh, Malay K. Nandy ยท 2026

We investigate whether the formally infinite-dimensional supertranslation sector of the Bondi-Metzner-Sachs (BMS) group remains fully physically admissible once classical energy conditions are enforceโ€ฆ

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Neural blind deconvolution to reconstruct high-resolution ground-based solar observations

Christoph Schirninger, Robert Jarolim, Astrid M. Veronig, Matthias Rempel, Friedrich Woger ยท 2026

Ground-based solar observations enable unprecedented spatial, spectral, and temporal resolution of the lower solar atmosphere, yet Earths turbulent atmosphere imposes significant limitations, requirinโ€ฆ

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Infrared spectropolarimetry of a C-class solar flare footpoint plasma -- I. Spectral features and forward modelling

Z. Vashalomidze, C. Quintero Noda, T. V. Zaqarashvili, M. Benko, D. Kuridze, P. Gomory, J. Rybak, S. Lomineishvili, M. Collados, C. Denker, M. Verma, C. Kuckein, A. Asensio Ramos ยท 2026

We performed high-spatial resolution spectropolarimetric observations of active region NOAA 13363 during a C-class flare with the Gregor Infrared Spectrograph (GRIS) on 16 July 2023. We examine the coโ€ฆ

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Carrollian Physics and Holography

Romain Ruzziconi ยท 2026

This report reviews key developments in Carrollian physics with an emphasis on their role in the emerging framework of holography in asymptotically flat spacetimes. We begin by introducing the Carrollโ€ฆ

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The gravitational energy-momentum pseudo-tensor in $f(Q)$ non-metric gravity

Salvatore Capozziello, Maurizio Capriolo, Gaetano Lambiase ยท 2026

We derive the affine tensor associated with the energy and momentum densities of both gravitational and matter fields, the complex pseudo-tensor, for $f(Q)$ non-metric gravity, the straightforward extโ€ฆ

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On prethermal time crystals from semi-holography

Toshali Mitra, Sukrut Mondkar, Ayan Mukhopadhyay, Alexander Soloviev ยท 2025

We demonstrate the existence of a pair of almost dissipationless oscillating modes at low temperatures in both the shear and sound channels of a hybrid quantum system, comprised of a weakly self-interโ€ฆ

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Time-domain measurement of Auger electron dynamics in xenon atoms after giant resonant photoionization

Mahmudul Hasan, Jingsong Gao, Hao Liang, Yiming Yuan, Zach Eisenhutt, Ming-Shian Tsai, Ming-Chang Chen, Hans Jakob Worner, Artem Rudenko, Meng Han ยท 2025

Time-resolved measurement of Auger-Meitner (AM) decay [Nature 419, 803 (2002)] marked a milestone in the development of attosecond science. To date, the time constants for the AM decay processes obtaiโ€ฆ

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The Use of Torsion in Supergravity Uplifts and Covariant Fractons

Davide Rovere ยท 2025

The aim of this Thesis is twofold. On the one hand, we find the necessary and sufficient conditions for a maximally supersymmetric supergravity theory in 3D to be a solution of 11D supergravity (but tโ€ฆ

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The calm before the storm: High spatial resolution mosaic of active region NOAA 14274 at the onset of an X1.2 flare

Carsten Denker, Robert Kamlah, Meetu Verma, Alexander G. M. Pietrow ยท 2025

Active region NOAA 14274 produced some of the strongest flares of Solar Cycle 25, including the X1.2 and X5.1 flares on 10 and 11 November 2025, respectively. We present the first large mosaic of specโ€ฆ

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On the center-to-limb variations of the He I 10 830 \AA\ triplet

A.G.M. Pietrow, C. Kuckein, M. Verma, C. Denker, J.C. Trelles Arjona, R. Kamlah, K. Poppenhager ยท 2025

We present high-resolution spectroscopic observations of the quiet-Sun center-to-limb variations (CLV) of the He I triplet at 10 830 {\AA} and the nearby Si I 10 827 {\AA} line, observed with GREGOR Iโ€ฆ

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An Unusual Velocity Field in a Sunspot Penumbra

H. Balthasar, C. Denker, A. Diercke, S. J. Gonzalez Manrique, C. Kuckein, J. Lohner Bottcher, R. E. Louis, M. Sobotka, M. Verma ยท 2025

The photospheric Evershed flow is normally oriented radially outward, yet sometimes opposite velocities are observed not only in the chromosphere but also in the photospheric layers of the penumbra. Wโ€ฆ

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Velocity field of an Active Region filament from GRIS IR He I and IRIS UV observations

M. Murabito, V. Andretta, S. Parenti, C. Kuckein, S. J. Gonzalez Manrique, S. M. Lezzi, S. L. Guglielmino ยท 2025

Plasma flow measurements in solar active region filaments are rare, particularly in the infrared and ultraviolet ranges that probe the chromosphere and transition region. In addition, previous studiesโ€ฆ

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