How Do We Derive Hawking’s Most Famous Equation? The Temperature of a Black Hole
Physics Explained
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Physics Explained is a channel that explores advanced topics in physics without skimping on the mathematical detail. There is a growing community of independent learners who are keen to explore modern ideas in physics with the aid of mathematical reasoning. This channel aims to tackle advanced topics head on whilst at the same time providing a historical narrative to help provide context to the ideas. A bit about my educational background: I have a PhD in theoretical physics, specialising in string theory. I now dedicate most of my my time to physics education. You can help support this channel via the Physics Explained Patreon account: https://www.patreon.com/physicsexplained
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Black holes are perhaps the most enigmatic objects in the universe. Popularised in movies and science fiction, they evoke the magic and mystery of our universe and provide inspiration for those looking to make their mark in the world of academic physics. But what exactly is a black hole? And how can we study them? According to Einstein’ theory of general relativity, a black hole is a region of spacetime where gravity is so strong that nothing, not even light can escape. The boundary of this region is known as the event horizon of the black hole, and according to classical relativity, once an object has passed the event horizon, it will never be able to escape the clutches of the black hole. However, when you throw quantum mechanics into the mix, as is often the case, the situation becomes a bit more subtle. In fact, in 1974 Stephen Hawking demonstrated that by combining certain elements of quantum field theory with General relativity, it was possible to show that Black holes do in fact radiate, causing them to slowly evaporate, and eventually disappear. Now I don’t know about you, but when I first read about black holes as a child I was instantly hooked and desperately wanted to find out more. The only problem is that the physics of black holes, and in particular Hawking’s work, is notoriously difficult and requires an advanced knowledge of Einstein’s theory of general relativity as well as quantum field theory. But is it possible to determine the most exciting and mysterious properties of black holes using only advanced high school mathematics? Well, it turns out the answer is yes, and in this short video I would like to show you how. References: Black Holes and Time Warps - Kip Thorne Dimensional Analysis and Black Holes - David Wakeham (https://hapax.github.io/assets/dimensional-analysis.pdf) Some Simple Black Hole Thermodynamics - Michael LoPreso (https://pubs.aip.org/aapt/pte/article-abstract/41/5/299/273943/Some-Simple-Black-Hole-Thermodynamics?redirectedFrom=fulltext) Gravity from the ground up - Shutz Black Hole Math - Nasa Resource (https://www.nasa.gov/sites/default/files/atoms/files/black_hole_math.pdf) Hawking for beginners: A dimensional analysis activity to perform in the classroom - Pinochet (https://iopscience.iop.org/article/10.1088/1361-6552/ab8ccc/pdf) The Holographic principle - Jean-Pierre Luminet (https://arxiv.org/pdf/1602.07258.pdf) You can help support this channel via the Physics Explained Patreon account: https://www.patreon.com/physicsexplained You can follow me on instagram: https://www.instagram.com/physics_explained_ig You can follow me on Twitter: https://twitter.com/PhysicsExplain1 https://iopscience.iop.org/article/10.1088/1361-6552/acdbb0/meta https://iopscience.iop.org/article/10.1088/1361-6552/acfe54
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