ONF-Chihuahua
Universidad Autónoma de Ciudad Juárez IADA T318 Ciudad Juárez, México
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Estimad@s profesore(a)s, hoy hemos enviado los diplomas de su participación como asesores (as) de nuestros participantes. Por favor, revisen los correos que registraron los estudiantes como dato de contacto institucional. En caso de cualquier error u omisión, les pedimos nos lo hagan saber para corregirlo. [email protected]
Felicidades a todos los participantes y nuestro reconocimiento especial a los ganadores de esta XXXI Olimpiada Nacional de Física Etapa Estatal
Cordialmente invitados
Estimados estudiantes, los diplomas de participación de la Olimpiada Estatal fueron enviados vía electrónica a los responsables que registraron en sus instituciones. Cualquier omisión que hayamos tenido, les pedimos nos informen para enviarles los reconocimientos. Todavía faltan de enviar los diplomas de asesores y ganadores.
Estimados alumnos, todos los seleccionados para la segunda etapa, debieron recibir también un segundo correo especificando el SALÓN virtual , en el que presentarán su examen. Revisen por favor su correo.
When a massive star collapses under its own gravity, it forms a black hole that is so heavy that it captures everything that passes its event horizon. Not even ...light can escape. At the event horizon, time replaces space and points only forward. The flow of time carries everything towards a singularity furthest inside the black hole, where density is infinite and time ends (see figure). Roger Penrose awarded the 2020 Nobel Prize in Physics invented ingenious mathematical methods to explore Albert Einstein’s general theory of relativity. He showed that the theory leads to the formation of black holes, those monsters in time and space that capture everything that enters them. Not even Albert Einstein, the father of general relativity, thought that black holes could actually exist. However, ten years after Einstein’s death, the British theorist Roger Penrose demonstrated that black holes can form and described their properties. At their heart, black holes hide a singularity, a boundary at which all the known laws of nature break down. To prove that black hole formation is a stable process, Penrose needed to expand the methods used to study the theory of relativity tackling the theory’s problems with new mathematical concepts. Penrose’s ground-breaking article was published in January 1965 and is still regarded as the most important contribution to the general theory of relativity since Einstein. The 2020 Nobel Prize in Physics has been awarded with one half to Roger Penrose for the discovery that black hole formation is a robust prediction of the general theory of relativity and the other half jointly to Reinhard Genzel and Andrea Ghez for the discovery of a supermassive compact object at the centre of our galaxy. Press release: https://bit.ly/309oZqF Popular information: https://bit.ly/3jjZSJk Advanced information: https://bit.ly/3kEwwFI
Estimados ganadores del Concurso de Talentos en Física, hoy les enviamos el diploma como ganadores del evento. Por favor, les pedimos avisarnos en caso de alguna omisión.
Ya estamos en la sesión de dudas del examen de mañana por TEAMS.
Orgullosos de nuestros ex-olímpicos.
¡Felicidades! XVI Concurso Nacional de Talentos en Física Etapa Estatal Resultados
Hoy iniciamos el programa de entrenamiento a las 5:30 p.m rumbo a la Etapa Nacional. Los detalles fueron enviados a los correos electrónicos de los participantes. ¡No falten!
BREAKING NEWS The Royal Swedish Academy of Sciences has decided to award the 2020 Nobel Prize in Physics with one half to Roger Penrose for the discovery that ...black hole formation is a robust prediction of the general theory of relativity and the other half jointly to Reinhard Genzel and Andrea Ghez for the discovery of a supermassive compact object at the centre of our galaxy. These three laureates share this year’s Nobel Prize in Physics for their discoveries about one of the most exotic phenomena in the universe, the black hole. Roger Penrose showed that the general theory of relativity leads to the formation of black holes. Reinhard Genzel and Andrea Ghez discovered that an invisible and extremely heavy object governs the orbits of stars at the centre of our galaxy. A supermassive black hole is the only currently known explanation. Roger Penrose used ingenious mathematical methods in his proof that black holes are a direct consequence of Albert Einstein’s general theory of relativity. Einstein did not himself believe that black holes really exist, these super-heavyweight monsters that capture everything that enters them. Nothing can escape, not even light. In January 1965, ten years after Einstein’s death, Roger Penrose proved that black holes really can form and described them in detail; at their heart, black holes hide a singularity in which all the known laws of nature cease. His ground-breaking article is still regarded as the most important contribution to the general theory of relativity since Einstein. Reinhard Genzel and Andrea Ghez each lead a group of astronomers that, since the early 1990s, has focused on a region called Sagittarius A* at the centre of our galaxy. The orbits of the brightest stars closest to the middle of the Milky Way have been mapped with increasing precision. The measurements of these two groups agree, with both finding an extremely heavy, invisible object that pulls on the jumble of stars, causing them to rush around at dizzying speeds. Around four million solar masses are packed together in a region no larger than our solar system. Using the world’s largest telescopes, Genzel and Ghez developed methods to see through the huge clouds of inter-stellar gas and dust to the centre of the Milky Way. Stretching the limits of technology, they refined new techniques to compensate for distortions caused by the Earth’s atmosphere, building unique instruments and committing themselves to long-term research. Their pioneering work has given us the most convincing evidence yet of a supermassive black hole at the centre of the Milky Way. The discoveries of this year’s laureates have broken new ground in the study of compact and supermassive objects. But these exotic objects still pose many questions that beg for answers and motivate future research. Not only questions about their inner structure, but also questions about how to test our theory of gravity under the extreme conditions in the immediate vicinity of a black hole, says David Haviland, chair of the Nobel Committee for Physics. Press release: https://bit.ly/309oZqF Popular information: https://bit.ly/3jjZSJk Advanced information: https://bit.ly/3kEwwFI
Les compartimos algunos momentos durante el Examen de Segunda Etapa de la Olimpiada Estatal de Física efectuado hoy sábado 5 de septiembre. Les deseamos el mayor de los éxitos a todos los participantes.
Información
Localidad: Ciudad Juárez
Ubicación: Universidad Autónoma de Ciudad Juárez IADA T318 Ciudad Juárez, México
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