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๐Ÿ” michael albert ๐Ÿ“‚ Physics
Showing 4937 results for "michael albert" in Physics
Physics Preprint PDF DOI

Second harmonic generation and third harmonic generation in topological insulator-based van der Waals metamaterials

Alessandra Di Gaspare, Sara Ghayeb, Craig Knox, Edmund H. Linfield, Joshua Freeman, Miriam S. Vitiello ยท 2026

High-order harmonic generation (HHG) in solids - the frequency up-conversion of an optical signal - is governed by symmetries. At terahertz (THz) frequencies, HHG is a key technology to access high frโ€ฆ

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Physics Preprint PDF DOI

Beyond Cloud-9: The case for discovering more HI-rich failed halos

Jorge Moreno, Coral Wheeler, Francisco J. Mercado, M. Katy Rodriguez Wimberly, Pratik J. Gandhi, Jenna Samuel, Robert Feldmann, James S. Bullock, Andrew Wetzel, Michael Boylan-Kolchin ยท 2026

HI-rich starless halos, should they exist, hold great promise for elucidating properties of dark matter halos. This Letter examines the properties of HI-rich failed halos at redshift zero across stateโ€ฆ

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Physics Preprint PDF DOI

Status of the KM3NeT real-time analysis framework

Martina Marconi (on behalf of the KM3NeT Collaboration) ยท 2026

Multi-messenger astronomy requires real-time systems capable of rapidly responding to external alerts and sharing significant detections with partner observatories. KM3NeT, a deep-sea Cherenkov neutriโ€ฆ

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Physics Preprint PDF DOI

Enabling real-time multi-messenger follow-up of transient events with Astro-COLIBRI

Bernardo Cornejo Avila, Sofia Bisero, Mickael Costa, Antoine Ciric, Ilja Jaroschewski, Weizmann Kiendrebeogo, Fabian Schussler ยท 2026

Time-domain astrophysics is a rapidly growing field focused on the study of transient phenomena such as Gamma-Ray Bursts (GRBs), Fast Radio Bursts (FRBs), supernovae, novae, and AGN flares. Their charโ€ฆ

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Physics Preprint PDF DOI

Gauge Theoretic Signal Processing II: Zero-Latency Whitening for Early Warning Pipelines

James Kennington, Joshua Black, Zach Yarbrough, Yun-Jing Huang, Chad Hanna, Leo Tsukada, Amanda Baylor, Olivia Godwin, Prathamesh Joshi, Cody Messick, Surabhi Sachdev, Ron Tapia ยท 2026

Low-latency gravitational-wave search pipelines provide early-warning alerts for multimessenger astrophysical transients. Current pipelines whiten the data stream using acausal, linear-phase filters, โ€ฆ

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Physics Preprint PDF DOI

SVOM/C-GFT: Instrumentation and Performances on the SVOM Alerts

Chao Wu, Zhe Kang, Xiao-Meng Lu, Xu-Hui Han, Li-Ping Xin, Pin-Pin Zhang, You Lv, Cheng-Wei Zhu, Ruo-Son Zhang, Jin-Song Deng, Yu-Lei Qiu, Mao-Hai Huang, Hong-Bo Cai, Hai-Bo Hu, Lei Huang, Lei Jia, Yu Luo, Jing Wang, Mo Zhang, Si-Cheng Zou, Zhen-Wei Li, Cheng-Zhi Liu, Jian-Yan Wei ยท 2026

The Chinese Ground Follow-up Telescope (C-GFT) is an optical facility upgraded to support the Space Variable Objects Monitor mission (\textit{SVOM}). Located at the Jilin Observation Station, it is caโ€ฆ

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Physics Preprint PDF DOI

Alert Chain and Observation Planning for Ground Wide Angle Camera Network

Xu-hui Han, Pin-pin Zhang, Yu-jie Xiao, Li-ping Xin, Ruo-song Zhang, Lei Huang, Xiao-meng Lu, Hong-bo Cai, Yang Xu, Wen-long Dong, Hua-li Li, Ya-tong Zheng, Jian-yan Wei ยท 2026

The Ground Wide Angle Camera Network (GWAC-N) is a robotic telescope network. It consists of ten wide-field core telescopes (GWAC-A) and two 60cm narrow-field rapid follow-up telescopes (GWAC-F60A/B).โ€ฆ

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Physics Preprint PDF DOI

The VHF alert network of the SVOM mission

B. Cordier, L. Jeannin, Ph. Lafabrie, G. Chavanas, S. Crepaldi, N. Dagoneau, A. Formica, V. Garcia, L. Jolivet, S. Lacour, H. Louvin, E. Sabatier ยท 2026

The scientific success of the SVOM mission will rely on the rapid transmission of alert messages from the satellite to the scientific community, and in particular to the ground-based instruments suppoโ€ฆ

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Physics Preprint PDF DOI

COLIBRI (SVOM/FM-GFT): Instrumentation and Performances on the SVOM Alerts

S. Basa, W. H. Lee, A. M. Watson, F. Dolon, J. Floriot, J.-L. Atteia, D. Dornic, E. E. Lugo-Ibarra, L. Figueroa, R. Langarica, H. Valentin, M. Ageron, F. Agneray, L. C. Alvarez Nunez, C. Angulo-Valdez, S. Antier, T. Auphan, M. Baumann, L. Bautista, R.L. Becerra, S. Benahmed, H. Benamar, C. Blanpain, O. Boulade, Y. Bounab, J. Boy, N.R. Butler, E. O. Cadena Zepeda, S. Cuevas, A. de Ugarte Postigo, C. Delisle, M. Devigny, J.G. Ducoin, F. Fortin, J. Fuentes-Fernandez, C. Gaiti, L. Garcia-Garcia, P. Gallais, R. Gill, N. Globus, G. Guisa, E. Kajfasz, D. Lafforgue, A. Langlois, M. Larrieu, J. Landa, J. Lecubin, D. Lopez-Camara, E. Lopez Angeles, S. Lombardo, F. Magnani, N. Mandarakas, A. Malgoyre, R. Mathon, E. Moreno Mendez, C. Moreau, A. Nouvel de la Fleche, J. L. Ochoa, L. Ortiz, M. H. Pedrayes-Lopez, M. Pereyra, L. Provost, P. Ramon, N.A. Rakotondrainibe, S. Ronayette, J. Ruiz Diaz-Soto, F. Sanchez Alvarez, B. Schneider, A. Secroun, N. Striebieg, S. Tinoco, M. Tourner-Sylvain, F. Valenzuela, D. Vincent ยท 2026

COLIBRI, the French Mexican Ground Followup Telescope (FM GFT) for SVOM, is a 1.3 meter rapid response optical facility specifically developed for prompt, multiband observations of GRB afterglows and โ€ฆ

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Physics Preprint PDF DOI

Overview of the ECLAIRs Trigger for SVOM gamma-ray burst detection

S. Schanne, F. Chateau, N. Dagoneau, F. Daly, H. Le Provost, P. Kestener ยท 2026

The French-Chinese SVOM satellite mission (Space-based multi-band astronomical Variable Objects Monitor) was launched in mid-2024, with science objectives focused on the detection and study of astrophโ€ฆ

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Physics Preprint PDF DOI

The SVOM French Science Center Infrastructure

H. Louvin, D. Corre, A. Formica, L. Jouvin, K. Tazhenova, T. Sadibekova, J. Palmerio, N. Dagoneau, A. Sauvageon, A. Claret, F. Agneray, C. Moreau, T. Fenouillet, Y. Roehlly, J-C. Thome, L. Michel, P. Maggi, L. Kleiver, P. Maeght, U. Jacob, F. Piron, P. Bacon, N. Bellemont, C. Cavet, F. Daigne, F. Lacreu, G. Tcherniatinsky, J. Wang, Y. Canton, I. Jegouzo, N. Leroy, S. Du, S. Lion, R. Le Montagner, C. Van Hove, J. Alaux, M. Boiziot, T. Auphan ยท 2026

At the heart of the SVOM French ground segment, the French Science Center is a cloud-based platform which provides services and tools for the management, storage, scientific processing and visualizatiโ€ฆ

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Physics Preprint PDF DOI

KilonovaSCORER: Prior-Predictive Scoring of Kilonovae for Real-Time Multimessenger Follow-Up

P. Darc, C. D. Kilpatrick ยท 2026

Real-time ranking of optical transient candidates during gravitational-wave (GW) and multimessenger follow-up is challenging when only sparse early-time, multi-band photometry is available.We present โ€ฆ

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Physics Preprint PDF DOI

Electromagnetic Precursors to Binary Neutron Star Mergers: Kinetic Simulations of Magnetospheric Flaring

Jasmine Parsons, Anatoly Spitkovsky, Alexander Philippov, Hayk Hakobyan ยท 2026

We present the first 3D global kinetic simulations of the interacting magnetospheres of pre-merger binary neutron stars. The stars, whose magnetic moments are anti-aligned, twist the field lines conneโ€ฆ

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Physics Preprint PDF DOI

Stochastic Krylov Dynamics: Revisiting Operator Growth in Open Quantum Systems

Arpan Bhattacharyya, S. Shajidul Haque, Jeff Murugan, Mpho Tladi, Hendrik J.R. Van Zyl ยท 2026

In closed quantum systems, Krylov complexity admits a geometric description; operator growth is equivalent to Hamiltonian flow in an emergent phase space whose structure is fixed by the Lanczos coeffiโ€ฆ

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Physics Preprint PDF DOI

Tensor network surrogate models for variational quantum computation

Ryo Watanabe, Dries Sels, Joseph Tindall ยท 2026

We adopt a two-dimensional tensor-network (TN) ansatz to simulate variational quantum algorithms on two-dimensional qubit architectures, demonstrating its capability to accurately simulate deep circuiโ€ฆ

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Physics Preprint PDF DOI

Study on the detector energy response of SVOM/GRM

Xiao-Yun Zhao, Jiang He, Shi-Jie Zheng, Ping Wang, Shao-Lin Xiong, Yue Huang, Dong-Ya Guo, Juan Zhang, Rui Qiao, Hao-Li Shi, Lu Li, Li Zhang, Jin Wang, Meng Bai, Yong-Wei Dong, Min Gao, Louvin Henri, Ulysse Jacob, Yong-Ye Li, Jiang-Tao Liu, Xin Liu, Qing-Yun Mao, Frederic Piron, Li-Ming Song, Rui-Feng Su, Jian-Chao Sun, Wen-Jun Tan, You-Li Tuo, Chen-Wei Wang, Jin-Zhou Wang, Rui-Jie Wang, Bo-Bing Wu, Wen-Hui Yu, Shuang-Nan Zhang, Shu-Min Zhao ยท 2026

The SVOM mission is specifically designed to for the detection and localization of Gamma-Ray Bursts (GRBs) and subsequent follow-up observations. Among the four telescopes installed on the SVOM satellโ€ฆ

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Physics Preprint PDF DOI

A universal relationship between the variability timescale and black hole mass in black hole jetted and non-jetted accreting systems

Yongyun Chen, Qiusheng Gu, Junhui Fan, Dingrong Xiong, Xiaoling Yu, Xiaogu Zhong, Xiaotong Guo ยท 2026

A long-term variability study spanning a range of black hole mass systems, from microquasars hosting stellar-mass black holes to active galactic nuclei (AGNs) harboring supermassive black holes, proviโ€ฆ

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Physics Preprint PDF DOI

SymTFT in Superspace

Federico Ambrosino, Alessandro Duci, Pietro Antonio Grassi, Silvia Penati ยท 2026

We propose a manifestly supersymmetric formulation of the Symmetry Topological Field Theory (SuSymTFT) for theories with supersymmetry. The SymTFT is a framework that helps organizing symmetries and aโ€ฆ

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Physics Preprint PDF DOI

Las Cumbres Observatory Gravitational-Wave Follow-up in O3 and O4: Strengths and Weaknesses of a Rapid Response Galaxy Targeted Strategy

Ido Keinan, Iair Arcavi, D. Andrew Howell, Curtis McCully, Craig Pellegrino, Ayelet Hasson, Moira Andrews, Jamison Burke, Daichi Hiramatsu, Jennifer Barnes, Sukanya Chakrabarti, Joseph R. Farah, Paul J. Groot, Na'ama Hallakoun, Daniel Holz, Saurabh W. Jha, Daniel Kasen, Chris Lidman, Michael J. Lundquist, Dan Maoz, Brian D. Metzger, Ehud Nakar, Megan Newsome, Yuan Qi Ni, Alexander H. Nitz, Estefania Padilla Gonzalez, Tsvi Piran, Dovi Poznanski, Ryan Ridden-Harper, David J. Sand, Brian P. Schmidt, Giacomo Terreran, Brad E. Tucker, Stefano Valenti, J. Craig Wheeler, Samuel Wyatt, Kathryn Wynn ยท 2026

We present a summary of gravitational-wave (GW) follow-up using the Las Cumbres Observatory global network of telescopes during the third (O3) and fourth (O4) observing runs of the GW detectors. As inโ€ฆ

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Physics Preprint PDF DOI

NOMAI : A real-time photometric classifier for superluminous supernovae identification. A science module for the Fink broker

E. Russeil, R. Lunnan, J. Peloton, S. Schulze, P. J. Pessi, D. Perley, J. Sollerman, A. Gkini, Y. Hu, T.-W. Chen, E. C. Bellm, T. X. Chen, B. Rusholme ยท 2026

Superluminous supernovae (SLSNe) are one of the most luminous stellar explosions known, yet they remain poorly understood. Because they are intrinsically rare, efficiently identifying them in the largโ€ฆ

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