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- Universidad Nacional Autónoma de MéxicoMX2 papers
- Benemérita Universidad Autónoma de PueblaMX1 paper
- Brookhaven National LaboratoryUS1 paper
- Central Bank of VenezuelaVE1 paper
- Central University of VenezuelaVE1 paper
- Centre National de la Recherche ScientifiqueFR1 paper
- Computing CenterRU1 paper
- Consejo Nacional de Investigaciones Científicas y TécnicasAR1 paper
- European Organization for Nuclear ResearchCH1 paper
- Exact Sciences (United States)US1 paper
- Federico Santa María Technical UniversityCL1 paper
- Fundação de Apoio à Universidade Federal de São PauloBR1 paper
7 papers
Comparison of spin-qubit architectures for quantum error-correcting codes
Mauricio Gutiérrez, Juan S. Rojas-Arias, David Obando +1
We investigate the performance of two quantum error-correcting codes, the surface code and the Bacon-Shor code, for implementation with spin qubits in silicon. In each case, we con…
Non-Equilibrium Thermodynamics of Black-Hole Coronae: QPOs, Turbulence, and Jets
Vanessa López-Barquero, Alejandro Jenkins, Christopher S. Reynolds +1
The variability of X-rays observed from accreting black hole systems, including quasi-periodic oscillations (QPOs), suggests a complex nonlinear dynamics in the corona. Here, we pr…
On the origin of the rotation of massive stars
André Oliva, Facundo D. Moyano, Luca Sciarini +3
We explore the origin of the rotation rates of massive stars. Contrary to their low-mass siblings, most massive stars do not have detectable magnetic fields, so that star-disk inte…
Randomly Initialized Networks Can Learn from Peer-to-Peer Consensus
Esteban RodrÃguez-Betancourt, Edgar Casasola-Murillo
In self-supervised learning, self-distilled methods have shown impressive performance, learning representations useful for downstream tasks and even displaying emergent properties.…
GeV emission in the region of Vela: a new view of the supernova remnant
Miguel Araya, Santiago RamÃrez, Diego Bueso +1
The Vela supernova remnant (SNR), G263.9-3.3, and its pulsar wind nebula (PWN), Vela X, is one of the closest such systems, and it has been studied using observations across the el…
Search for TeV emission from spider millisecond pulsars with HAWC
R. Alfaro, E. Anita-Rangel, M. Araya +90
Millisecond pulsars (MSPs) are observed to emit multi-wavelength radiation, from radio to GeV. Spider MSPs, which interact with their low-mass companion in close orbit (orbital per…