Vectors and Scalars 

This was written a while ago so sorry for any errors.

If a particle is moving in a straight line, it can only go in two ways. One way to look at its action is as good, and the other way as negative. However, a plus or minus sign is no longer enough to show the direction of a particle moving in three dimensions. We need to use a vector instead. This chapter talks about the (vector) rules of combination that work for vectors, which have both direction and size. A vector variable is any number that can be shown as a vector because it has both a size and a direction. These are some examples of vector numbers in the real world: acceleration, motion, and displacement. It will help you a lot in later parts to understand how vector combinations work, because you will be seeing a lot more of them. Not every real amount has a direction that goes with it. As an example, the ideas of time, energy, mass, temperature, and pressure do not “point” in the usual sense. We use normal algebraic rules to deal with these numbers, which are called scalars. Scalars are made up of a single number and a sign, like 40°F. Moving from one place to another is the most basic type of vector number. If a vector shows a displacement, it makes sense to call it a displacement vector. (Acceleration and motion vectors work the same way.) Something goes from A to B and is said to have undergone a transfer from A to B. An arrow from A to B shows this change in position. The line shows what the vector looks like. There are three lines that go from A to B. They are all the same size and point in the same direction. In this way, they show the same change in where the particles are and describe the same vectors of movement. You can move the vector without changing its value as long as its length and direction don’t change. What the shift vector doesn’t tell us is anything about the particle’s real path. Displacement vectors don’t really show motion; they just show how the motion affects everything.

arXiv

If you’re interested in physics or math (or a few other subjects) and want to read the actual papers then you can easily do so.  In my field (cosmology) there is no need to subscribe to expensive journals to read papers.  We just go to the eprint (electronically printed) server arxiv.org where you can look up any paper you want without paying.  It is free and legal.  arXiv is run by Cornell University and has papers from the past 20 years on there.  

Continue reading “arXiv”

(Initial) Review of Dark Energy: Theory and Observations


I want to talk about the first (and as of this post only) textbook on Dark Energy I have used.  As of this post I have not gone through the book but I have read enough to get an idea of how it is.  There is another Dark Energy book I recently discovered that I want to check out, but that will need to wait for another day.  I am not getting paid to write this review, these are my own thoughts.

Dark Energy: Theory and Observations was published in 2010, and was written by Luca Amendola and Shinji Tsujikawa.  A lot has happened in the realm of Dark Energy research since then, but the basics have stayed the same.  This means that much of the book is still useful and you will learn some good tips and tricks throughout, even if some of the theories have been disproved (plus it is always fun and useful to play around with what ifs). Continue reading “(Initial) Review of Dark Energy: Theory and Observations”