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305 pages, Kindle Edition
First published September 15, 2022
The Biggest Ideas in the Universe is dedicated to the idea that it is possible to learn about modern physics for real, equations and all, even if you are more amateur than professional and have every intention of staying that way. It is meant for people who have no more mathematical experience than high school algebra, but are willing to look at an equation and think about what it means. If you’re willing to do that bit of thinking, a new world opens up.
Most popular books assume that you don’t want to make the effort to follow the equations. Textbooks, on the other hand, assume that you don’t want to just understand the equations, you want to solve them. And solving these equations, it turns out, is enormously more work and requires enormously more practice and learning than “merely” understanding them does.
The Biggest Ideas in the Universe is dedicated to the idea that it is possible to learn about modern physics for real, equations and all, even if you are more amateur than professional and have every intention of staying that way. It is meant for people who have no more mathematical experience than high school algebra, but are willing to look at an equation and think about what it means.
If we draw a sphere centered on the sun, the lines of force all pass through that sphere. If we draw another sphere with a bigger radius, the same lines will pass through it, but they will be more spread out—fewer lines will pass through any fixed area of the sphere.
Now there are two distinct notions of what is meant by "time." One notion of time is as a coordinate on spacetime. Spacetime is a four-dimensional continuum, and if we want to specify locations within it, it's convenient to attach a nunmber called "the time" to every point within it. That's generally what we have in mind when we think of "6 p.m." and "7 p.m." Those refer to values of a coordinate on spacetime, labels that help us locate events. Everyone is supposed to understand what we mean when we say "meet at the restaurant at 7 p.m."
But, says relativity, just as the distance as the crow flies is generally different from the distance you actually travel between two points in space, the duration of time that you experience along your world line generally won't be the same as the universal coordinate time. You experience an amount of time that could be measured by a clock that you carry with you on the journey. This is the proper time along the path. And the duration measured by a clock, just like the distance traveled as measured by the odometer on your car, will depend on the path you take.
In space, a straight line describes the shortest distance between two points. In spacetime, by contrast, a straight path yields the longest elapsed time between two events.
[Imported automatically from my blog. Some formatting there may not have translated here.]
I've read a couple of Sean Carroll's pop-science books (The Big Picture and Something Deeply Hidden) over the past few years, so when this new one became available at Portsmouth Public Library, I grabbed it.
Now, science books aimed at the masses will often shy away from math. Sometimes their authors will acknowledge and excuse this by pointing out the relevant market forces: their publishers' research shows that each equation in a book will decrease sales by X percent, or something. But (I assume) Carroll successfully persuaded his publisher to let him math it up in this book, so good for him. This book is volume one of a projected trilogy; the next one will be subtitled Quanta and Fields, and the last Complexity and Emergence. I'm on board.
But this book concentrates on "classical" physics. He starts off slow, describing Newtonian mechanics, conservation laws, aided by basic calculus. Moving on to Lagrangian mechanics and the principle of least action. And then Hamiltonian mechanics. All do an approximately fine job of describing non-relativistic motion of macroscopic bodies.
But then we edge into Einsteinian insights, the interplay between space, time, mass, and energy. And then (watch out!) the notion of curved spacetime, which quickly invokes (eek!) tensor notation, the better to introduce General Relativity. And before you know it, we're hip deep in Riemann and Ricci and all that stuff. To a point where (if you've been following along, nodding your head) you can appreciate beauty of the Einstein equation (I'm not sure how this will appear on Goodreads):
Rμν - ½Rgμν = 8πGTμν
And we wind up with a good (but quick) discussion of black holes (they're hairless!), event horizons, naked singularities, accretion disks, gravitational waves and the like.
I must confess that, even though I was a physics major decades ago, I got lost at a certain point. I think to actually know this material, you have to take courses from smarter people, doing problem sets along the way. There's no shiny magic path to understanding. But (on the other hand) I learned a good deal at the fuzzy territory between "yeah, this is simple, I get this" and "whoa, what's going on here?"