DescriereFriedmann universes.svg	English: The age and ultimate fate of the universe can be determined by measuring the Hubble constant today and extrapolating with the observed value of the deceleration parameter, uniquely characterized by values of density parameters (ΩM for matter and ΩΛ for dark energy). A "closed universe" with ΩM > 1 and ΩΛ = 0 comes to an end in a Big Crunch and is considerably younger than its Hubble age. An "open universe" with ΩM ≤ 1 and ΩΛ = 0 expands forever and has an age that is closer to its Hubble age. For the accelerating universe with nonzero ΩΛ that we inhabit, the age of the universe is coincidentally very close to the Hubble age. Intended as a replacement for Universe.svg and Universos.gif.
Dată	23 septembrie 2009
Sursă	Operă proprie
Autor	BenRG
SVG dezvoltare InfoField	Sursa acestui fișier SVG este validă.  Această imagine vectorială a fost creată cu Other tools   This diagram uses embedded text that can be easily translated using a text editor. This diagram supersedes the file Universe.svg. It is recommended to use this file rather than the other one. Deutsch ∙ English ∙ español ∙ فارسی ∙ français ∙ magyar ∙ Bahasa Indonesia ∙ italiano ∙ 日本語 ∙ 한국어 ∙ македонски ∙ മലയാളം ∙ Nederlands ∙ polski ∙ prūsiskan ∙ português do Brasil ∙ русский ∙ slovenščina ∙ svenska ∙ 中文（简体） ∙ 中文（繁體） ∙ +/−

This diagram uses the following exact solutions to the Friedmann equations:

${\displaystyle {\begin{cases}a(t)=H_{0}t&\Omega _{M}=\Omega _{\Lambda }=0\\{\begin{cases}a(q)={\tfrac {\Omega _{M}}{2(1-\Omega _{M})}}(\cosh q-1)\\t(q)={\tfrac {\Omega _{M}}{2H_{0}(1-\Omega _{M})^{3/2}}}(\sinh q-q)\end{cases}}&0<\Omega _{M}<1,\ \Omega _{\Lambda }=0\\a(t)=\left({\tfrac {3}{2}}H_{0}t\right)^{2/3}&\Omega _{M}=1,\ \Omega _{\Lambda }=0\\{\begin{cases}a(q)={\tfrac {\Omega _{M}}{2(\Omega _{M}-1)}}(1-\cos q)\\t(q)={\tfrac {\Omega _{M}}{2H_{0}(\Omega _{M}-1)^{3/2}}}(q-\sin q)\end{cases}}&\Omega _{M}>1,\ \Omega _{\Lambda }=0\\a(t)=\left({\tfrac {\Omega _{M}}{\Omega _{\Lambda }}}\sinh ^{2}\left({\tfrac {3}{2}}{\sqrt {\Omega _{\Lambda }}}H_{0}t\right)\right)^{1/3}&0<\Omega _{M}<1,\ \Omega _{\Lambda }=1-\Omega _{M}\end{cases}}}$

Some of the shown models are implemented as an animation at Cosmos-animation.

use strict;
use Svg;
use Math::Trig qw(sinh cosh acos asinh acosh pi);

sub ScaleFunc {
	my ($H0, $M0, $with_lambda) = @_;
	if ($M0 == 1) {
		my $q0 = 2/(3*$H0);
		return sub { my ($q) = @_; ($q - $q0, (1.5 * $H0 * $q) ** (2/3)) };
	}
	if ($with_lambda) {
		my $L0 = 1 - $M0;
		# assume 0 < $M0 < 1
		my $a = ($M0/$L0) ** (1/3);
		my $b = 1.5 * $H0 * sqrt($L0);
		my $q0 = asinh(sqrt($L0/$M0)) / $b;
		return sub { my ($q) = @_; ($q - $q0, $a * (sinh($b * $q) ** (2/3))) }
	} else {
		# \Omega_{\Lambda_0} = 0
		my $k0 = 1 - $M0;
		if ($M0 == 0) {
			return sub { my ($q) = @_; ($q - 1/$H0, $q * $H0) }
		} else {
			my $a = $M0 / (2 * abs($k0));
			my $b = 1 / ($H0 * sqrt(abs($k0)));
			my $c = $a * $b;
			if ($M0 > 1) {
				my $d = $a * (2 / ($H0 * $M0) - acos(2/$M0 - 1) * $b);
				return sub { my ($q) = @_; ($c * ($q - sin($q)) + $d, $a * (1 - cos($q))) }
			} else {
				# 0 < M < 1
				my $d = $a * (acosh(2/$M0 - 1) * $b - 2 / ($H0 * $M0));
				return sub { my ($q) = @_; ($c * (sinh($q) - $q) + $d, $a * (cosh($q) - 1)) }
			}
		}
	}
}

sub SubscriptedText {
	my $text = shift;
	$text->add(shift);
	my $sub = 0;
	for my $t (@_) {
		$sub = !$sub;
		$text->tspan($sub ? (dy => 4, 'font-size' => 12) : (dy => -4))->add($t);
	}
}

my ($image_width,$image_height) = (620,500);
my ($origin_x, $origin_y) = (30.5,450.5);
my $pad_right = 70;
my ($tlo, $thi, $ahi) = (-15,18,2.5);

my $svg = new Svg(width => $image_width, height => $image_height);
#	$svg->rect(width => $image_width, height => $image_height, fill => 'gray');
$svg->defs()->marker(id => 'arrowhead', refX => 0, refY => 3, markerWidth => 10, markerHeight => 6, markerUnits => 'userSpaceOnUse', orient => 'auto')->path(d => 'M 0,0 L 10,3 L 0,6 z');
my $traces = $svg->group(stroke => 'black', 'stroke-width' => 2, fill => 'none');
my $axes = $svg->group(stroke => 'black', 'stroke-width' => 1, fill => 'none');
my $labels = $svg->group('font-family' => 'Nimbus Roman No9 L, Times, serif', 'font-size' => 20, 'text-anchor' => 'middle', stroke => 'none', fill => 'black');
my $H0 = 1 / 13.95;
my $M0 = 0.279;
my ($graphscalex,$graphscaley) = (($image_width-$origin_x-$pad_right)/($thi-$tlo), -$origin_y/$ahi);
my ($graphofsx,$graphofsy) = ($origin_x - $tlo * $graphscalex, $origin_y);
for my $z ([0,0,30,'none'],[$M0,0,3.17,'1,4'],[1,0,26,'2,2'],[6,0,2*pi,'1,3,4,3'],[$M0,1,27,'5,3']) {
	my ($m0,$with_lambda,$max_q,$dashes) = @$z;
	my $f = ScaleFunc($H0,$m0,$with_lambda);
	my (@x,@y);
	for my $i (0..200) {
		($x[$i],$y[$i]) = &$f($i / 200 * $max_q);
	}
	$traces->path('stroke-dasharray' => $dashes, ($m0 == 6 ? () : ('marker-end' => 'url(#arrowhead)')), d => MakePath(\@x, \@y, $graphscalex, $graphscaley, $graphofsx, $graphofsy, 1));
}
$axes->line(x1 => $origin_x, y1 => $image_height-20, x2 => $origin_x, y2 => 20, 'marker-end' => 'url(#arrowhead)');
$axes->line(x1 => 10, y1 => $origin_y, x2 => $image_width - $pad_right + 10, y2 => $origin_y, 'marker-end' => 'url(#arrowhead)');
$labels->text(x => ($origin_x + $image_width) / 2, y => $image_height-10)->add('Billions of years from now');
my $path = '';
for my $gyr (-13.7, -10, -5, 0, 5, 10, 15) {
	my $x = int($gyr * $graphscalex + $graphofsx);
	my $y = $origin_y-5;
	$path .= "M$x.5,${y}l0,10";
	$labels->text(x => $x, y => $origin_y + 20)->add($gyr);
}
$axes->path(d => $path);
$labels->circle(cx => $graphofsx, cy => $graphscaley + $graphofsy, r => 4);
$labels->text(x => $graphofsx-5, y => $graphscaley + $graphofsy, 'text-anchor' => 'end')->add('Now');
$labels->text()->rotate(-90)->translate($origin_x - 8, $origin_y / 2)->add("Average distance between galaxies");
my $trace_labels = $labels->group('font-family' => 'DejaVu Serif, serif', 'font-size' => 16);
SubscriptedText($trace_labels->text(x => 465, y => 30, 'text-anchor' => 'end'), "\x{3A9}", 'M', " = 0.3, \x{3A9}", "\x{39B}", " = 0.7");
SubscriptedText($trace_labels->text(x => 520, y => 50, 'text-anchor' => 'start'), "\x{3A9}", 'M', ' = 0');
SubscriptedText($trace_labels->text(x => 535, y => 70, 'text-anchor' => 'start'), "\x{3A9}", 'M', ' = 0.3');
SubscriptedText($trace_labels->text(x => 540, y => 95, 'text-anchor' => 'start'), "\x{3A9}", 'M', ' = 1');
SubscriptedText($trace_labels->text(x => 540, y => 400, 'text-anchor' => 'start'), "\x{3A9}", 'M', ' = 6');

$svg->write('Friedmann universes.svg');

Eu, deținătorul drepturilor de autor ale acestei opere, o eliberez domeniului public. Aceasta se aplică în întreaga lume. În anumite țări există posibilitatea ca acest lucru să nu fie legal posibil; în acest caz: permit oricui să utilizeze această operă în orice scop, fără nicio condiție, atâta timp cât asemenea condiții nu sunt cerute de lege.