Metric of the de Sitter space–time

Loading...

來自 National Research University Higher School of Economics 的課程

Introduction into General Theory of Relativity

81 個評分

National Research University Higher School of Economics

Introduction into General Theory of Relativity

81 個評分

General Theory of Relativity or the theory of relativistic gravitation is the one which describes black holes, gravitational waves and expanding Universe. The goal of the course is to introduce you into this theory. The introduction is based on the consideration of many practical generic examples in various scopes of the General Relativity. After the completion of the course you will be able to solve basic standard problems of this theory. We assume that you are familiar with the Special Theory of Relativity and Classical Electrodynamics. However, as an aid we have recorded several complementary materials which are supposed to help you understand some of the aspects of the Special Theory of Relativity and Classical Electrodynamics and some of the calculational tools that are used in our course. Also as a complementary material we provide the written form of the lectures at the website: https://math.hse.ru/generalrelativity2015

從本節課中

Cosmological solutions with non-zero cosmological constant

In this module we derive constant curvature de Sitter and anti de Sitter solutions of the Einstein equations with non-zero cosmological constant. We describe the geometric and causal properties of such space-times and provide their Penrose-Carter diagrams. We provide coordinate systems which cover various patches of these space-times.

De Sitter and anti-de Sitter13:00

Geometry of the de Sitter space–time11:33

Metric of the de Sitter space–time9:19

Penrose–Carter diagram for the de Sitter space–time10:15

Poincare' patches for the de Sitter space–time16:50

Geometry of the anti–de Sitter space–time7:20

Metric of the anti–de Sitter space–time9:16

Penrose–Carter diagram of the anti–de Sitter space–time8:25

Poincare' patch of the anti–de Sitter space–time6:08

與講師見面

Emil Akhmedov
Associate Professor
Faculty of Mathematics

[MUSIC]

Okay, we are still considering this hyperboloid X0 squared plus.

x1 squared plus

x d squared equal to h minus second.

And we going to now we discuss

the generic things about the geometry of this space etc.

Now we're going to provide coordinates in the space, or for example.

This hyper void is embedded into the space with signature d x 0 squared minus d

x 1 squared minus d x.

D squared.

So one can solve this equation very easily.

For example, by X zero equal to hyperbolic sign of

HT divided by H.

And XI equal to NI times hyperbole

cosin of HT divided by H where

I is running from one to D.

So, actually I is running all of theese guys and

if ni squared sum over i = 1.

So this defined the units here ni.

We obtained that these things solve this equation.

Now if we flag this into here.

From ni we obtain d- 1 dimensionals sphere.

We'll discuss it in a moment.

So the metric that is induced on this space from this metric

is equal to dt squared- hyperbolic of sine squared of Ht

over h squared d omega D- 1 squared.

So this is a sphere,

D- 1 dimensional unit sphere and it appears exactly from this guy.

Exactly from this guy.

And how to see that?

Let me explain it.

So for example, this equation which is the difference d- 1 dimensional

sphere in d dimensional space can be solved as follows.

We can define n1 which is cosine, cosine of theta 1.

And theta 1 is ranging between- pi over

2 of two P over P then N two equal to sine

tetra one times cosine tetra two and

tetra two is ranging between SP over two

P over 2 and so forth.

Up to md minus 1 which is sine

of theta 1, sine theta 2 dot dot dot,

sine Theta D minus 2 times cos of theta D minus 1 was theta D minus 1.

All these angles ranging in this range and

at the same time, theta D minus 1 is ranging

between Minus pi and pi.

Remember that, well let me finish first and

then I'll explain what what is going on.

ND is equal to sin TAT one sin

TAT to two dot dot dot sin TAT to D minus two sin.

Theta d- 1.

So the situation is very similar with the case of two-dimensional sphere.

Remember that are two angles phi which is ranging exactly in this range.

And theta which is ranging in this range.

This how we cover two-dimensional sphere only once.

And that is exactly the same situation that we encounter here.

So all the angles except this one take this range

and only one angle ranges here.

In case if D = 2,

D = 2 we obtain only that one angle here phi

or theta 1 which is ranging in this range in fact.

So that is a circle.

So we going to draw this in a moment again, but

let me just say the following thing.

The d omega d -1 squared.

If we use this which solves this and

plug it here, we obtain that this guy is just nothing but.

Sum over g from 1 to

d minus 1 and product of

over i from 1 to g minus 1 of sins.

Square of theta i times d theta j squared.

This is a metric on you need d minus 1 dimensional sphere.

Actually by the way, big rotation can be seen already on this metric.

If we change Ht to i

theta D

minus pi over 2, if we do such a change in this metric.

Then we map this metric to 1 over h squared times d omega.

So this metric is map to this, d omega d squared.

So which is exactly the map between de sitter space.

And d dimensional sphere, and

now one can straightforwardly see the meaning of this picture that I drew.

So when we have h zero, which is in fact simply changes

geniously, rising from minus infinity to plus infinity.

This is a x1, x2.

We obtain this hyperboloid every time

slice constant x0 corresponds to constant t.

So, every time slice of this hyperbola, this is just a sphere.

D minus one dimensional sphere.

For this two dimensional case, it's just a circle because in this case,

we have a one dimensional sphere which is a circle and actually using this.

Using this one can see that hyperbolic distance is expressed as false.

It's just a minus hyperbolic sign of Ht1 times

hyperbolic sign of Ht2 +

hyperbolic cosine of Ht1 times hyperbolic cosine

of Ht2 times cosine of omega.

Where cosine of omega is nothing but

n1 scale up of the form where n1 and

n2 are at least vectors defining first and second point.

So, now the geometry of the space becomes apparent and

we're going to consider with the consideration of Penrose diagram

to discuss causal properties of decision space.

We're going to continue the discussion of Penrose diagram for the space.

[MUSIC]

探索我們的目錄

免費加入並獲得個性化推薦、更新和優惠。

Coursera 致力於普及全世界最好的教育，它與全球一流大學和機構合作提供在線課程。

© 2018 Coursera Inc. 保留所有權利。

通過 App Store 下載

通過 Google Play 獲取