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pget_Luminosity
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Created
Sat, Feb 1, 08:39
Size
2 KB
Mime Type
text/x-python
Expires
Mon, Feb 3, 08:39 (2 d)
Engine
blob
Format
Raw Data
Handle
24003682
Attached To
rGTOOLS Gtools
pget_Luminosity
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#!/usr/bin/python
from
optparse
import
OptionParser
import
Ptools
as
pt
from
pNbody
import
*
from
pNbody
import
units
from
pNbody
import
ctes
import
string
from
pNbody
import
units
,
io
,
ctes
from
scipy.optimize
import
bisect
as
bisection
def
parse_options
():
usage
=
"usage: %prog [options] file"
parser
=
OptionParser
(
usage
=
usage
)
parser
.
add_option
(
"--tnow"
,
action
=
"store"
,
dest
=
"tnow"
,
type
=
"float"
,
default
=
None
,
help
=
"desired time"
,
metavar
=
" FLOAT"
)
parse
=
pt
.
add_units_options
(
parser
)
parser
=
pt
.
add_ftype_options
(
parser
)
(
options
,
args
)
=
parser
.
parse_args
()
files
=
args
return
files
,
options
########################################################################
# MAIN
########################################################################
if
__name__
==
'__main__'
:
files
,
opt
=
parse_options
()
if
len
(
files
)
==
0
:
sys
.
exit
()
file
=
files
[
0
]
nb
=
Nbody
(
file
,
ftype
=
opt
.
ftype
)
unit_params
=
pt
.
do_units_options
(
opt
)
HubbleParam
=
unit_params
[
'HubbleParam'
]
nb
.
set_local_system_of_units
(
params
=
unit_params
)
nb
=
nb
.
select
(
1
)
Rmax
=
nb
.
rxyz
()
.
max
()
############################
# find tR using bissectrice
############################
lmax
=
90
nb
.
L
=
nb
.
Luminosity
(
tnow
=
opt
.
tnow
)
Ltot
=
sum
(
nb
.
L
)
rs
=
nb
.
rxyz
()
def
getL
(
r
):
nb_s
=
nb
.
selectc
(
rs
<
r
)
L
=
sum
(
nb_s
.
L
)
return
lmax
-
100
*
L
/
Ltot
Rt
=
bisection
(
getL
,
0.0
,
50
,
args
=
(),
xtol
=
0.1
,
maxiter
=
400
)
nb_s
=
nb
.
selectc
(
rs
<
Rt
)
L
=
sum
(
nb_s
.
L
)
out_units
=
units
.
UnitSystem
(
'local'
,[
units
.
Unit_kpc
,
units
.
Unit_Msol
,
units
.
Unit_s
,
units
.
Unit_K
])
fL
=
nb
.
localsystem_of_units
.
convertionFactorTo
(
out_units
.
UnitLength
)
print
print
"tidal radius : Rt =
%g
[kpc/h]"
%
(
Rt
*
fL
)
print
"tidal radius : Rt =
%g
[kpc]"
%
(
Rt
*
fL
/
HubbleParam
)
print
"Luminosity in tidal radius : L =
%g
[1e6 Lsol]"
%
(
L
/
1e6
)
print
"Total luminosity : Ltot =
%g
[1e6 Lsol]"
%
(
Ltot
/
1e6
)
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