Black Holes and Diagrams of Different Coordinate Systems
In General Relativity by Woodhouse there are the three following diagrams in Chapter 9 about Black Holes. Despite a (very brief) description of these diagrams in the book itself, I am struggling to understand what they exactly correspond to? Does anyone have good way of looking at how these diagrams help convey a) the properties of the particular coordinate system and b) a understanding of how black holes work in the particular coordinate system being looked at.
geometry differential-geometry mathematical-physics general-relativity
add a comment |
In General Relativity by Woodhouse there are the three following diagrams in Chapter 9 about Black Holes. Despite a (very brief) description of these diagrams in the book itself, I am struggling to understand what they exactly correspond to? Does anyone have good way of looking at how these diagrams help convey a) the properties of the particular coordinate system and b) a understanding of how black holes work in the particular coordinate system being looked at.
geometry differential-geometry mathematical-physics general-relativity
Crossposted from physics.stackexchange.com/q/450464/2451
– Qmechanic
Dec 26 at 16:39
add a comment |
In General Relativity by Woodhouse there are the three following diagrams in Chapter 9 about Black Holes. Despite a (very brief) description of these diagrams in the book itself, I am struggling to understand what they exactly correspond to? Does anyone have good way of looking at how these diagrams help convey a) the properties of the particular coordinate system and b) a understanding of how black holes work in the particular coordinate system being looked at.
geometry differential-geometry mathematical-physics general-relativity
In General Relativity by Woodhouse there are the three following diagrams in Chapter 9 about Black Holes. Despite a (very brief) description of these diagrams in the book itself, I am struggling to understand what they exactly correspond to? Does anyone have good way of looking at how these diagrams help convey a) the properties of the particular coordinate system and b) a understanding of how black holes work in the particular coordinate system being looked at.
geometry differential-geometry mathematical-physics general-relativity
geometry differential-geometry mathematical-physics general-relativity
asked Dec 26 at 15:13
Permian
2,1801035
2,1801035
Crossposted from physics.stackexchange.com/q/450464/2451
– Qmechanic
Dec 26 at 16:39
add a comment |
Crossposted from physics.stackexchange.com/q/450464/2451
– Qmechanic
Dec 26 at 16:39
Crossposted from physics.stackexchange.com/q/450464/2451
– Qmechanic
Dec 26 at 16:39
Crossposted from physics.stackexchange.com/q/450464/2451
– Qmechanic
Dec 26 at 16:39
add a comment |
1 Answer
1
active
oldest
votes
The radial null geodesics for the Schwarzschild metric have the form
$$
t pm [r + 2 m ln (r - 2m)] = k tag{1}
$$
where $k$ is a constant. This is a plot for different values of $k$
The plots you showed are just an attempt to represent these geodesics in three spatial coordinates. Unfortunately that cannot be done trivially, so instead Woodhouse decided to ignore one of the coordinates and draw Eq. (1) in the other two. You can do that by setting $x = rcosphi$ and $y = r sinphi$ for $0leq phi leq 2pi$. Or equivalently by rotating the curves in the figure above around the $t$ axis. This is an example for $k = 1$
This is just a fancy extension of the first figure above, but it is completely unnecessary, since the problem has spherical symmetry, and adding an extra coordinate just adds to the noise without any benefit.
Hi what software did you use for plotting?
– magma
Dec 27 at 14:03
@magma Good old python
– caverac
Dec 27 at 14:04
add a comment |
Your Answer
StackExchange.ifUsing("editor", function () {
return StackExchange.using("mathjaxEditing", function () {
StackExchange.MarkdownEditor.creationCallbacks.add(function (editor, postfix) {
StackExchange.mathjaxEditing.prepareWmdForMathJax(editor, postfix, [["$", "$"], ["\\(","\\)"]]);
});
});
}, "mathjax-editing");
StackExchange.ready(function() {
var channelOptions = {
tags: "".split(" "),
id: "69"
};
initTagRenderer("".split(" "), "".split(" "), channelOptions);
StackExchange.using("externalEditor", function() {
// Have to fire editor after snippets, if snippets enabled
if (StackExchange.settings.snippets.snippetsEnabled) {
StackExchange.using("snippets", function() {
createEditor();
});
}
else {
createEditor();
}
});
function createEditor() {
StackExchange.prepareEditor({
heartbeatType: 'answer',
autoActivateHeartbeat: false,
convertImagesToLinks: true,
noModals: true,
showLowRepImageUploadWarning: true,
reputationToPostImages: 10,
bindNavPrevention: true,
postfix: "",
imageUploader: {
brandingHtml: "Powered by u003ca class="icon-imgur-white" href="https://imgur.com/"u003eu003c/au003e",
contentPolicyHtml: "User contributions licensed under u003ca href="https://creativecommons.org/licenses/by-sa/3.0/"u003ecc by-sa 3.0 with attribution requiredu003c/au003e u003ca href="https://stackoverflow.com/legal/content-policy"u003e(content policy)u003c/au003e",
allowUrls: true
},
noCode: true, onDemand: true,
discardSelector: ".discard-answer"
,immediatelyShowMarkdownHelp:true
});
}
});
Sign up or log in
StackExchange.ready(function () {
StackExchange.helpers.onClickDraftSave('#login-link');
});
Sign up using Google
Sign up using Facebook
Sign up using Email and Password
Post as a guest
Required, but never shown
StackExchange.ready(
function () {
StackExchange.openid.initPostLogin('.new-post-login', 'https%3a%2f%2fmath.stackexchange.com%2fquestions%2f3053022%2fblack-holes-and-diagrams-of-different-coordinate-systems%23new-answer', 'question_page');
}
);
Post as a guest
Required, but never shown
1 Answer
1
active
oldest
votes
1 Answer
1
active
oldest
votes
active
oldest
votes
active
oldest
votes
The radial null geodesics for the Schwarzschild metric have the form
$$
t pm [r + 2 m ln (r - 2m)] = k tag{1}
$$
where $k$ is a constant. This is a plot for different values of $k$
The plots you showed are just an attempt to represent these geodesics in three spatial coordinates. Unfortunately that cannot be done trivially, so instead Woodhouse decided to ignore one of the coordinates and draw Eq. (1) in the other two. You can do that by setting $x = rcosphi$ and $y = r sinphi$ for $0leq phi leq 2pi$. Or equivalently by rotating the curves in the figure above around the $t$ axis. This is an example for $k = 1$
This is just a fancy extension of the first figure above, but it is completely unnecessary, since the problem has spherical symmetry, and adding an extra coordinate just adds to the noise without any benefit.
Hi what software did you use for plotting?
– magma
Dec 27 at 14:03
@magma Good old python
– caverac
Dec 27 at 14:04
add a comment |
The radial null geodesics for the Schwarzschild metric have the form
$$
t pm [r + 2 m ln (r - 2m)] = k tag{1}
$$
where $k$ is a constant. This is a plot for different values of $k$
The plots you showed are just an attempt to represent these geodesics in three spatial coordinates. Unfortunately that cannot be done trivially, so instead Woodhouse decided to ignore one of the coordinates and draw Eq. (1) in the other two. You can do that by setting $x = rcosphi$ and $y = r sinphi$ for $0leq phi leq 2pi$. Or equivalently by rotating the curves in the figure above around the $t$ axis. This is an example for $k = 1$
This is just a fancy extension of the first figure above, but it is completely unnecessary, since the problem has spherical symmetry, and adding an extra coordinate just adds to the noise without any benefit.
Hi what software did you use for plotting?
– magma
Dec 27 at 14:03
@magma Good old python
– caverac
Dec 27 at 14:04
add a comment |
The radial null geodesics for the Schwarzschild metric have the form
$$
t pm [r + 2 m ln (r - 2m)] = k tag{1}
$$
where $k$ is a constant. This is a plot for different values of $k$
The plots you showed are just an attempt to represent these geodesics in three spatial coordinates. Unfortunately that cannot be done trivially, so instead Woodhouse decided to ignore one of the coordinates and draw Eq. (1) in the other two. You can do that by setting $x = rcosphi$ and $y = r sinphi$ for $0leq phi leq 2pi$. Or equivalently by rotating the curves in the figure above around the $t$ axis. This is an example for $k = 1$
This is just a fancy extension of the first figure above, but it is completely unnecessary, since the problem has spherical symmetry, and adding an extra coordinate just adds to the noise without any benefit.
The radial null geodesics for the Schwarzschild metric have the form
$$
t pm [r + 2 m ln (r - 2m)] = k tag{1}
$$
where $k$ is a constant. This is a plot for different values of $k$
The plots you showed are just an attempt to represent these geodesics in three spatial coordinates. Unfortunately that cannot be done trivially, so instead Woodhouse decided to ignore one of the coordinates and draw Eq. (1) in the other two. You can do that by setting $x = rcosphi$ and $y = r sinphi$ for $0leq phi leq 2pi$. Or equivalently by rotating the curves in the figure above around the $t$ axis. This is an example for $k = 1$
This is just a fancy extension of the first figure above, but it is completely unnecessary, since the problem has spherical symmetry, and adding an extra coordinate just adds to the noise without any benefit.
answered Dec 26 at 19:08
caverac
13.5k21029
13.5k21029
Hi what software did you use for plotting?
– magma
Dec 27 at 14:03
@magma Good old python
– caverac
Dec 27 at 14:04
add a comment |
Hi what software did you use for plotting?
– magma
Dec 27 at 14:03
@magma Good old python
– caverac
Dec 27 at 14:04
Hi what software did you use for plotting?
– magma
Dec 27 at 14:03
Hi what software did you use for plotting?
– magma
Dec 27 at 14:03
@magma Good old python
– caverac
Dec 27 at 14:04
@magma Good old python
– caverac
Dec 27 at 14:04
add a comment |
Thanks for contributing an answer to Mathematics Stack Exchange!
- Please be sure to answer the question. Provide details and share your research!
But avoid …
- Asking for help, clarification, or responding to other answers.
- Making statements based on opinion; back them up with references or personal experience.
Use MathJax to format equations. MathJax reference.
To learn more, see our tips on writing great answers.
Some of your past answers have not been well-received, and you're in danger of being blocked from answering.
Please pay close attention to the following guidance:
- Please be sure to answer the question. Provide details and share your research!
But avoid …
- Asking for help, clarification, or responding to other answers.
- Making statements based on opinion; back them up with references or personal experience.
To learn more, see our tips on writing great answers.
Sign up or log in
StackExchange.ready(function () {
StackExchange.helpers.onClickDraftSave('#login-link');
});
Sign up using Google
Sign up using Facebook
Sign up using Email and Password
Post as a guest
Required, but never shown
StackExchange.ready(
function () {
StackExchange.openid.initPostLogin('.new-post-login', 'https%3a%2f%2fmath.stackexchange.com%2fquestions%2f3053022%2fblack-holes-and-diagrams-of-different-coordinate-systems%23new-answer', 'question_page');
}
);
Post as a guest
Required, but never shown
Sign up or log in
StackExchange.ready(function () {
StackExchange.helpers.onClickDraftSave('#login-link');
});
Sign up using Google
Sign up using Facebook
Sign up using Email and Password
Post as a guest
Required, but never shown
Sign up or log in
StackExchange.ready(function () {
StackExchange.helpers.onClickDraftSave('#login-link');
});
Sign up using Google
Sign up using Facebook
Sign up using Email and Password
Post as a guest
Required, but never shown
Sign up or log in
StackExchange.ready(function () {
StackExchange.helpers.onClickDraftSave('#login-link');
});
Sign up using Google
Sign up using Facebook
Sign up using Email and Password
Sign up using Google
Sign up using Facebook
Sign up using Email and Password
Post as a guest
Required, but never shown
Required, but never shown
Required, but never shown
Required, but never shown
Required, but never shown
Required, but never shown
Required, but never shown
Required, but never shown
Required, but never shown
Crossposted from physics.stackexchange.com/q/450464/2451
– Qmechanic
Dec 26 at 16:39