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D1-Talks 2
Date:
27 Mar 11:00 - 12:45
Conveners
Cosmic Rays/Galactic/Extragalactic
Dr. Alvarez, Cesar (Universidad Autonoma de Chiapas)
Los Halos de TeV son regiones de emisión extendida alrededor de un pulsar central. Los Halos se producen por dispersión de Compton inversa de partículas cargadas aceleradas en la nebulosa de viento de pulsar y que viajan difusivamente fuera de la nebulosa. En este trabajo se presenta un modelo analítico que depende sólo de las características de los pulsares para estimar el flujo en rayos ga
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Presented by Mrs. Maria Fernanda CARREON GONZALEZ
on
27/3/2023
at
17:30
La conexión entre los destellos de rayos gamma cortos (sGRBs) y las ondas gravitacionales (GWs) han sido objeto de estudio y motivación para la búsqueda de contrapartes por instrumentos de rayos gamma. Sin embargo, solo un evento hasta la fecha ha sido identificado como una ocurrencia simultánea de ambos, GRB 170817A y GW170817. GRB 170817A fue clasificado como un destello de corta duración
... More
Presented by Mr. Jorge MONTES MIRELES
on
27/3/2023
at
18:15
HAWC es un observatorio terrestre con 300 detectores Cherenkov en agua distribuidos en un área de 22,000 m$^2$, detecta de forma indirecta rayos gamma y rayos cósmicos con energías superiores a los 300 GeV. Una de las tareas críticas es la reconstrucción de energía de los rayos gamma y rayos cósmicos. Actualmente, se cuenta con dos estimadores de energía dedicados a rayos gamma, mientras q
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Presented by Alexander ALVARADO
on
27/3/2023
at
17:15
En 2017 el observatorio HAWC descubrió un nuevo tipo de fuente de altas energías, los halos de TeV. Son regiones extensas alrededor de algunos pulsares de edad media. Su emisión de fotones es a energías de decenas de TeV y se produce por interacciones de Compton inverso de electrones y positrones acelerados por el pulsar. En este trabajo se propone utilizar el software EDGE y un modelo analít
... More
Presented by Mr. Erick Alejandro RANGEL
on
27/3/2023
at
17:45
The energy spectrum of cosmic rays contains crucial information about the propagation and acceleration mechanisms of these particles, on their astrophysical sources and about the presence of possible nearby cosmic-ray accelerators. The energy region between 10 TeV and 1 PeV in the spectrum has received recent interest since new observations have revealed a break in this energy regime and bec
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Presented by Mr. Jorge Antonio MORALES SOTO
on
27/3/2023
at
17:00
Los destellos de rayos gamma (GRB) son de los fenómenos mas energéticos del universo. Se caracterizan por su emisión inmediata en rayos X-duros y por su emisión tardía a lo largo del espectro electromagnético. El GRB 221009A ha sido uno de los destellos más luminosos detectados hasta la fecha. Durante los primeros 2000 segundos de su emisión se detectaron fotones de rayos gamma con energí
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Presented by Ms. Sara FRAIJA CASTELLANOS
on
27/3/2023
at
18:30
Los halos de tera-electronvolt (TeV halos) son una nueva subclase de fuentes de rayos-$\gamma$ recientemente detectados alrededor de algunos pulsares de edad media. Se trata de regiones de emisión extendidas a energías de TeV con tamaños de $\sim 10 \mathrm{~pc}$ alrededor del pulsar central. Recientemente, se han propuesto modelos para cuantificar la población de TeV halos en la Vía Láctea
... More
Presented by Mr. Alexis ANDRÉS
on
27/3/2023
at
18:00
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