I hereby claim:
- I am jamesamiller on github.
- I am millerja (https://keybase.io/millerja) on keybase.
- I have a public key whose fingerprint is 06B1 8D7A FB64 382E 292B 858D EC72 8F76 E67A 0E67
To claim this, I am signing this object:
I hereby claim:
To claim this, I am signing this object:
\documentclass[crop=true, border=10pt]{standalone} | |
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\begin{comment} | |
:Title: Attack from Andromeda | |
:Author: J A Miller (millerja@uah.edu), 2020/02/04 | |
The Andromeda "paradox". Spacetime diagram for aliens launching an attack on Earth, according to three observers: one on the ground in the same frame as the aliens, and two walking past the first in opposite directions with the same speed. | |
References: |
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\begin{comment} | |
:Title: Area preservation in the Lorentz Transformations | |
:Author: J A Miller, UAH Physics & Astronomy, millerja@uah.edu | |
2020/02/04 | |
Plot to demonstrate how the Lorentz Transformation preserves area. Suppose the primed frame is moving in the $+x$ direction with speed $v$ relative to the unprimed frame. | |
Consider a unit square in the primed frame, with corners at $A^\prime =(x,t) =(0,0)$, $B^\prime =(0,1)$, $C^\prime =(1,1)$, and $D^\prime =(1,0)$. In the unprimed system, these points are transformed into $A = (0,0)$, $B = (\gamma v,\gamma)$, $C = (\gamma (1+v),\gamma (1+v))$, and $D = (\gamma,\gamma v)$, which outlines a parallelogram (in the unprimed coordinate system). |
\documentclass[crop=true, border=10pt]{standalone} | |
\usepackage{comment} | |
\begin{comment} | |
:Title: Spacetime diagrams | |
:Author: J A Miller (millerja@uah.edu), 2020/02/06 | |
Generate spacetime or two-observer diagrams. | |
Parameters can be set by the user. The distance between neighboring grid lines is one. |
\documentclass[crop=true, border=10pt]{standalone} | |
\usepackage{comment} | |
\begin{comment} | |
:Title: Two passing spaceships | |
:Author: J A Miller, UAH Physics & Astronomy, millerja@uah.edu | |
2020/02/14 | |
Two spaceships passing each other | |
The distance between neighboring grid lines is one. |
\documentclass[crop=true, border=10pt]{standalone} | |
\usepackage{comment} | |
\begin{comment} | |
:Title: Tortoise and Hare - Variation 1 | |
:Author: J A Miller (millerja@uah.edu), 2020/03/03 | |
A race between a tortoise and hare. | |
The distance between neighboring grid lines is one. |
\documentclass[crop=true, border=10pt]{standalone} | |
\usepackage{comment} | |
\begin{comment} | |
:Title: Accelerated coordinate system | |
:Slug: Accelerated coordinates | |
:Tags: special relativity | |
:Author: J A Miller, UAH Physics & Astronomy, millerja@uah.edu, 2020/05/12 | |
Plot of accelerated coordinates $\xi$ and $\eta$ on an $x$-$t$ inertial spacetime. |
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\begin{comment} | |
:Title: Motion of stars in the accelerated rocket frame | |
:Slug: Accelerated frame | |
:Tags: special relativity | |
:Author: J A Miller, UAH Physics & Astronomy, millerja@uah.edu, 2020/05/12 | |
Worldlines of stars in the accelerated rocket coordinates $\xi$ and $\eta$. |
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\usepackage{comment} | |
\begin{comment} | |
:Title: Motion of another rocket in an accelerated rocket frame | |
:Slug: Accelerated frame | |
:Tags: special relativity | |
:Author: J A Miller, UAH Physics & Astronomy, millerja@uah.edu, 2020/05/18 | |
Worldlines of a test rocket in the accelerated coordinates $\xi$ and $\eta$ of an observer rocket. This illustrates that a constant proper distance requires different accelerations. |
\documentclass[crop=true, border=10pt]{standalone} | |
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\begin{comment} | |
:Title: Motion of stars in the accelerated rocket frame | |
:Slug: Rocket frame | |
:Tags: special relativity | |
:Author: J A Miller, UAH Physics & Astronomy, millerja@uah.edu, 2020/05/12 | |
Worldlines of stars and a rocket in the inertial $x$-$t$ frame, with light rays from one of | |
the stars to the rocket worldline. |