The Neutron Time Of Flight (n-TOF) facility is a neutron spectrometer at CERN. It consists of a pulsed source, a flight path of 200 m length, and a detector systems. Neutron energies are deduced from the time of flight between source and detector; hence the name of the facility. The neutrons are produced by neutron spallation; by directing a pulsed beam of protons from the Proton Synchrotron (PS) towards a lead target about 300 neutrons expelled for each impact of a proton. The neutrons are slowed after being emitted, first by the lead target and afterwards by a slab containing water. This results in a wide range of neutron energies since some neutrons will slow down more than others when passing through the targets. Finally, the neutrons are ejected through the 200m long flight path before they arrive at an experimental area. (Wikipedia).
Can You Calculate The TIME OF FLIGHT For This Ball?!? #Mechanical #Engineering #Physics #Projectile #NicholasGKK #Shorts
From playlist Mechanical Engineering
Physics - Relativity: Understanding Space, Time & Relativity (16 of 55) Time to Fly to the Sun
Visit http://ilectureonline.com for more math and science lectures! In this video I will explain how distance and amount of time needed to travel to the Sun change for observer B (on space ship) traveling closer and closer to the speed of light. Next video in this series can be seen at:
From playlist PHYSICS 62.1 UNDERSTANDING RELATIVITY & SPACE
Physics 2.5 - Motion In 1-D - Graphical Solution (2 of 12) Ex.2 Jet on Aircraft
Visit http://ilectureonline.com for more math and science lectures! In this video I will graphically solve the acceleration=? of a jet going from 0-175mph in 2.5 seconds. Next video can be seen at: https://youtu.be/DbbuL0-cQ84
From playlist PHYSICS MECHANICS 1: INTRO, VECTORS, MOTION, PROJECTILE MOTION, NEWTON'S LAWS
Teach Astronomy - Photons and Space Analogy
http://www.teachastronomy.com/ Photons are the fastest thing there is. Light and other forms of electromagnetic communication travel at three hundred thousand kilometers per second, vastly out seeding the capabilities of any type of rocket that we know or can imagine. As an example of th
From playlist 28. Interstellar Travel, SETI, and the Rarity of Life
Earth To Mars In 100 Days? The Power Of Nuclear Rockets
The Solar System is a really big place, and it takes forever to travel from world to world with traditional chemical rockets. But one technique, developed back in the 1960s might provide a way to dramatically shorten our travel times: nuclear rockets. Of course, launching a rocket powered
From playlist Mars
Lec 35: Professor Lewin’s Early days at MIT | 8.01 Classical Mechanics, Fall 1999 (Walter Lewin)
Professor Lewin talks about some of the highlights from his early days at MIT. It began with balloon flights at very high altitude to make observations of the stars in X-rays. This led to discoveries of X-ray flaring events and a periodic X-ray source (GX 1+4). In the seventies and eightie
From playlist 8.01 Physics I: Classical Mechanics, Fall 1999 (Complete Lectures by Walter Lewin)
الميكانيك التقليدي (إم آي تي) 35: وداع خاص، الفيزياء الفلكية عالية الطاقة
MIT المحاضرة الخامسة والثلاثون والأخيرة من مساق "الميكانيك التقليدي" من جامعة "إم آي تي" للبروفيسور والتر لوين وهي عن: وداع خاص، الفيزياء الفلكية عالية الطاقة بالإضافة للفيديو هناك ملفات مرفقة على موقعنا الالكتروني https://shamsunalarabia.net/courses/ﺍﻟﻤﻴﻜﺎﻧﻴﻚ-التقليدي/ رابط المساق https:
From playlist 8.01 Arabic Subtitles
Physics - Relativity: Understanding Space, Time & Relativity (12 of 55) What Happens to Time at v=c?
Visit http://ilectureonline.com for more math and science lectures! In this video I will explain what happens to time when we reach the speed of light. According to Einstein, every observer see light moving at the speed of light regardless of the observer's speed. Next video in this seri
From playlist PHYSICS 62.1 UNDERSTANDING RELATIVITY & SPACE
8.01x - Lect 35 - Farewell Special, My Early Days in Astrophysics, Huge Balloons
My Research during my Early Years at MIT - Balloon Astronomy in Australia - Great Photos - Great Story. Exam (final): http://freepdfhosting.com/739ff9822b.pdf Solutions (final): http://freepdfhosting.com/c5d81e6fb2.pdf
From playlist 8.01x - MIT Physics I: Classical Mechanics
Neutron Stars: Crash Course Astronomy #32
In the aftermath of an 8-20 solar mass star’s demise, we find a weird little object known as a neutron star. Neutron stars are incredibly dense, spin rapidly, and have very strong magnetic fields. Some of them we see as pulsars, flashing in brightness as they spin. Neutron stars with the s
From playlist Astronomy
الاهتزازات والأمواج (جامعة إم آي تي) - المحاضرة 23: الوداع
MIT المحاضرة الثالثة والعشرون من مساق "الاهتزازات والأمواج" من جامعة إم آي تي للبروفيسور والتر لوين وهي مخصصة للوداع بالإضافة للفيديو هناك ملفات مرفقة على موقعنا الالكتروني https://shamsunalarabia.net/courses/الاهتزازات-والأمواج/ رابط المساق https://www.youtube.com/watch?v=FfdJewVimWs&lis
From playlist 8.03 Arabic Subtitles
Astronomy - Ch. 22: Neutron Star (7 of 17) What is the Upper Limit of a Neutron Star?
Visit http://ilectureonline.com for more math and science lectures! To donate: http://www.ilectureonline.com/donate https://www.patreon.com/user?u=3236071 We will learn the upper and lower limit of a neutron star are 1.0-2.5 times the mass of our Sun, and about 12 miles or 20 km in diame
From playlist THE "WHAT IS" PLAYLIST
Lec 36: Farewell Special | 8.02 Electricity and Magnetism, Spring 2002 (Walter Lewin)
Farewell Special. Bring a Friend! This lecture is part of 8.02 Physics II: Electricity and Magnetism, as taught in Spring 2002 by Dr. Walter Lewin at MIT. This video was formerly hosted on the YouTube channel MIT OpenCourseWare. This version was downloaded from the Internet Archive, at h
From playlist MIT: 8.02 Electricity and Magnetism - CosmoLearning.com Phys
Physics - Nuclear Physics (1 of 22) Mass of Proton, Neutron, and Electron
Visit http://ilectureonline.com for more math and science lectures! In this video I will show you how to find the mass of proton, neutron, and electron.
From playlist MOST POPULAR VIDEOS
Lec 23: Farewell Lecture | 8.03 Vibrations and Waves, Fall 2004 (Walter Lewin)
Farewell Special - Bring a Friend! This lecture is part of 8.03 Physics III: Vibrations and Waves, as taught in Fall 2004 by Dr. Walter Lewin at MIT. This video was formerly hosted on the YouTube channel MIT OpenCourseWare. This version was downloaded from the Internet Archive, at https:
From playlist 8.03 Vibrations and Waves - CosmoLearning.com Physics
Teach Astronomy - Properties of Neutron Stars
http://www.teachastronomy.com/ Neutron stars are truly remarkable objects. Think of something with the mass of the Sun, normally one and a half million kilometers across, compressed down to the size of a small asteroid, about twenty kilometers across. Conservation of angular momentum dic
From playlist 16. Stars 3
Flare States of the Crab Nebula
From NASA Astrophysics and the amazings at Goddard Space Flight Center. The famous Crab Nebula supernova remnant has erupted in an enormous flare five times more powerful than any flare previously seen from the object. On April 12, NASA's Fermi Gamma-ray Space Telescope first detected the
From playlist Violent Universe
HOW IT WORKS: Nuclear Propulsion
The theory, design, and operation of a nuclear propulsion engine advantages are explained verses conventional chemical rockets such as the Saturn V.
From playlist HOW IT WORKS