From the 1 of 6 papers with an AI index.
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- Universidade Federal da Integração Latino-AmericanaBR4 papers
- Universidade Federal do Espírito SantoBR4 papers
- Universidade Federal do ParanáBR4 papers
- Universidade Tecnológica Federal do ParanáBR4 papers
- Universidade de São PauloBR3 papers
- Centro Universitário de Rio PretoBR1 paper
- Instituto Nacional de Pesquisas EspaciaisBR1 paper
- Universidade Federal de Campina GrandeBR1 paper
- Universidade Federal do ABCBR1 paper
- University of TorontoCA1 paper
6 papers
Non-thermal emission from the vicinity of the magnetar CXOU J171405.7-381031
Manoel F. Sousa, Rita. C. Anjos
Magnetars are neutron stars with ultra-strong magnetic fields (- G) and are promising candidates for high-energy particle acceleration. We present a multiw…
Multiwavelength study of non-thermal emission in the Swift J1834.9-0846/W41 region
Manoel F. Sousa, Rita C. Dos Anjos, Vitor de Souza
The paper models the broadband non‑thermal emission from the Swift J1834.9‑0846/W41 region, comparing leptonic and lepto‑hadronic scenarios and finding that a lepto‑hadronic model…
Scaling Symmetry in Symplectic Thermodynamics
M. C. Baldiotti, R. Fresneda
This paper investigates scaling symmetry in thermodynamics by unifying constrained Hamiltonian dynamics with symplectic and contact geometries. Through the mathematical processes o…
Canonical quantization for Equilibrium Thermodynamics
Luis F. Santos, Victor Hugo M. Ramos, Danilo Cius +2
We formulate a canonical quantization of Equilibrium Thermodynamics by applying Dirac's theory of constrained systems. Thermodynamic variables are treated as conjugate pairs of coo…
High-Synchrotron-Peaked BL Lacs as Multi-Messenger Sources: Connecting Ultra-High-Energy Cosmic Rays and Neutrinos
Luiz Augusto Stuani Pereira, Rita C. Anjos
High-synchrotron-peaked (HSP) BL Lac objects are extreme particle accelerators whose synchrotron emission peaks at high frequencies, typically in the UV-to-X-ray band ($ν_{\rm pea…
Probing Low-Luminosity Gamma-Ray Emission from SNR G296.5+10.0 and CCO 1E 1207.4-5209 with CTAO
Luana N. Padilha, Rubens Jr. Costa, Rita C. dos Anjos +1
The acceleration mechanisms of cosmic rays (CR) in supernova remnants (SNRs) and their associated compact central objects (CCOs) remain an open question in high-energy astrophysics…