Документ взят из кэша поисковой машины. Адрес оригинального документа : http://hea-www.harvard.edu/~dburke/PDL/README-Astro-Cosmology-0.90 Дата изменения: Sat Aug 4 19:39:55 2001 Дата индексирования: Tue Oct 2 04:28:16 2012 Кодировка: Поисковые слова: п п п п п р п c 1999 s4 linear

Astro::Cosmology
----------------

A set of routines to calculate cosmological measures (ie distance, volume,
and time) for commonly-used cosmological models. The interface is
object-orientated so that you don't have to keep on specifying the parameters
of the model each time you call a routine (an example is included below).

The module also provides a couple of useful constants, however this is only
an interim measure as constants are probably better provided by another
module (for instance see the Astroconst package at
http://clavelina.as.arizona.edu/astroconst/).

Although in the Astro namespace, this module *requires* that PDL is installed
on your system.

History
-------

04 Aug 2001 v0.90 more reorganisation. Hopefully CPAN-friendly now
more tests (thanks Brad)
02 Aug 2001 v0.84 minor reorganisation, no change to code or docs
01 Aug 2001 v0.83 added version method, renamed string to stringify
further documentation improvements
improvements to test suite (thanks Brad)
29 Jul 2001 v0.82 added STERADIAN to constants
improved documentation
28 Jul 2001 v0.81 renamed to Astro::Cosmology
removed need for PDL::Astro::Constants
19 Jul 2001 v0.5 initial "public" release (as PDL::Astro::Cosmology)

Example
-------

use Astro::Cosmology qw( :constants );

my $eds = Astro::Cosmology->new();
my $sn = Astro::Cosmology->new( matter => 0.3, lambda => 0.7,
h0 => 70 );

print "$eds\n$sn\n";
[ Omega_matter = 1 Omega_lambda = 0 H0 = 50 km/s/Mpc ]
[ Omega_matter = 0.3 Omega_lambda = 0.7 H0 = 70 km/s/Mpc ]

my $z = (1 + sequence(10)) / 10;
my $de = 1.0e6 * PARSEC * $eds->lum_dist($z);
my $ds = 1.0e6 * PARSEC * $sn->lum_dist($z);

wcols '%3.1f %9.3e %9.3e', $z, $de, $ds;
0.1 1.894e+25 1.420e+25
0.2 3.869e+25 3.024e+25
0.3 5.914e+25 4.791e+25
0.4 8.022e+25 6.703e+25
0.5 1.019e+26 8.742e+25
0.6 1.240e+26 1.089e+26
0.7 1.466e+26 1.314e+26
0.8 1.696e+26 1.548e+26
0.9 1.930e+26 1.790e+26
1.0 2.168e+26 2.039e+26

Requirements
------------

Requires the PDL distribution, which is available from CPAN or
http://pdl.perl.org/. It should work on most recent (ie v2.1.1 and
later) versions of PDL. It has been developed using v5.6.0 of perl,
but should work with v5.005 .

It has been developed on solaris and linux systems, but it should work
on other "unix-like" systems.

The additional tests, in the cpt/ and hogg/ directories of the distribution
use the PGPLOT interface in PDL to produce graphical output. Therefore
you need to have installed the perl PGPLOT module (available from CPAN) and
the pgplot library ;)

Build/Installation
------------------

The module should build and install using the standard perl approach of:

perl Makefile.PL
make
make test
make install

Note that the module will not build if the PDL module is not installed on
your system. See the ExtUtils::MakeMaker documentation for customisation
hints.

Currently the test script is not very clever. I suggest you also try the
scripts discussed in the next section.

Additional Tests
----------------

The test script mainly checks that the module is consistent - ie that it
works as expected. Although there are some checks of the validity of the
output, it is not guaranteed to catch all problems. I advise you to also
run the additional scripts in the cpt/ and hogg/ directories: these produce
graphical output (using PGPLOT) and should be the same as some of the figures
in:

Carroll, Press & Turner, 1992, ARAA, 30, 499 (directory cpt/)
Hogg, Distance measures in cosmology, astro-ph/9905116 (directory hogg/)

To run the angular diameter test in cpt/ you should be able to do

perl cpt/angular_diameter.pl

after a successful 'make' (you do not need to have done a 'make install' since
the scripts pick up the version in the blib/ directory).

Notes
-----

If you compare the output from 'perl cpt/differential_comoving_volume.pl'
and figure 6 (page 514) of Carroll, Press & Turner, you'll see that my
values are slightly smaller than their values at z ~ 100. I don't know why this
is; I'm hoping that it's just due to numerical differences, but it could be
something wrong with this code. As I don't really work with objects much beyond
z = 1, it's not currently high on my priority list.

To do
-----

.) Add Pen's approximations and more of the functionality from D Hogg's
astro-ph paper.
.) release on CPAN

Acknowledgements
----------------

Thanks to Brad Holden for trying out early versions of this module
and for providing some of the test code.

The cosmology routines make use of code based on routines from

NUMERICAL METHODS: FORTRAN Programs, (c) John H. Mathews 1994
NUMERICAL METHODS for Mathematics, Science and Engineering, 2nd Ed, 1992
Prentice Hall, Englewood Cliffs, New Jersey, 07632, U.S.A.

The "Integration Technique" section of the documentation is based on that
from from the Math::Integral::Romberg module by Eric Boesch (available
on CPAN).

Copyright
---------

Copyright (C) Douglas Burke 1999, 2000, 2001.

All rights reserved. There is no warranty.
This program is free software; you can redistribute it
and/or modify it under the same terms as Perl itself.