#--------------------------------
# Overall label for this simulation
#--------------------------------

# Short descriptive name
# NOTE: this name is not necessarily unique! Please use the SXS or PRIVATE
# identifier in alternative-names to unambiguously refer to this simulation.
simulation-name = d52.5_m2.1_m1.4_g2k101_s0_0_0_s0_0_0.0/Lev0

# Other names under which this run has been referenced (e.g. papers)
alternative-names = BHNSq1.5s0, SXS:BHNS:0006

# Keywords to qualitatively identify this simulation
keywords = NonSpinning,Polytrope

#--------------------------------
# Researchers
#--------------------------------

# Point-of-contact for this waveform.  Usually the person having placed the
# waveform into the repository
point-of-contact-email = francois.foucart@unh.edu

# Researchers who contributed to the generation of this waveform.
# (typically this is the list of authors for publications using this
#  waveform).
authors-emails         = Francois Foucart <francois.foucart@unh.edu>, Matthew Duez <m.duez@wsu.edu>, Tanja Hinderer <T.Hinderer@astro.ru.nl>, Andrew Williamson <a.williamson@science.ru.nl>, Michael Boyle <michael.oliver.boyle@gmail.com>, Alessandra Buonanno <alessandra.buonanno@aei.mpg.de>, Roland Haas <rhaas@ncsa.illinois.edu>, Dan Hemberger <daniel.hemberger@gmail.com>, Larry Kidder  <kidder@astro.cornell.edu>, Harald Pfeiffer <harald.pfeiffer@aei.mpg.de>, Mark Scheel <scheel@tapir.caltech.edu>

#--------------------------------
# References
#--------------------------------

# (1) papers describing this particular run (if any)
simulation-bibtex-keys = Hinderer:2016eia,Chakravarti:2018uyi,SXSCatalogWebsite

# (2) papers describing the evolution code
code-bibtex-keys = Foucart:2012vn,Duez:2008rb,SpECwebsite

# (3) papers describing the initial data
initial-data-bibtex-keys = Foucart:2008qt,Lovelace:2008tw,Pfeiffer:2007yz,Caudill:2006hw,Cook:2004kt

# (4) papers describing eccentricity reduction
quasicircular-bibtex-keys = Mroue:2012kv,Buonanno:2010yk,Mroue:2010re,Boyle:2007ft

#--------------------------------
# Input Parameters for Initial Data
#--------------------------------

initial-data-type         = BHNS
initial-separation        = 52.5
initial-orbital-frequency = 0.004524450
initial-adot              = -0.00001206

# Type of compact object (bh or ns)
object1 = bh
object2 = ns
eos     = "polytrope(kappa=101.4496,gamma=2)"

#--------------------------------
# t=0 quantities
#--------------------------------

initial-ADM-energy           =  3.475229291
initial-ADM-linear-momentum  =  -3.4134203732589281e-06  -2.0768413414982537e-06   2.7871896796905579e-09
initial-ADM-angular-momentum = 0 0 1.2993342233650518e+01

# Christodoulou mass at t=0
initial-mass1     =  2.1
# ADM mass of an isolated, non-rotating NS of the same baryon mass as the evolved object
initial-mass2     =  1.4

# dimensionless spins at t=0
initial-dimensionless-spin1 = 1.04907e-12 -1.52309e-12 8.39152e-08
initial-dimensionless-spin2 = 0 0 0 

initial-position1 = 20.992 0.367546 0 
initial-position2 = -31.5 0 0

#--------------------------------
# Quantities at reference time
#--------------------------------

# time at which we deem junk radiation to have sufficiently decayed
relaxation-time = 500

# time at which the reference quantities are measured
reference-time = 500

# Christodoulou mass at reference time
reference-mass1    = 2.10000631184477
reference-mass2    = [unknown]
# dimensionless spins, i.e. \chi_i = S_i / M_i^2, at reference time
reference-dimensionless-spin1 = -4.0524119925502e-09 4.82734757914467e-09 2.61796370681615e-06
reference-dimensionless-spin2 = [unknown]

# black hole and neutron star centers at reference time
reference-position1 = -1.3190184373128345e+01   1.6224653083611660e+01  -1.4802832124883989e-05
reference-position2 = 2.0020131533248218e+01  -2.4148526076861419e+01   0.0000000000000000e+00

# orbital frequency at reference time
reference-orbital-frequency = 0.00460696476484

#--------------------------------
# Info that concerns complete run
#--------------------------------

# orbital eccentricity and mean anomaly estimated at reference time
reference-eccentricity = <2.7e-4
reference-mean-anomaly = 2.4

# merger time [= peak of GW amplitude]
merger-time  = 16076

# number of orbits between t=0 merger time
number-of-orbits  = 16.6

#--------------------------------
# Remnant properties
#--------------------------------
# We do not attempt to reliably evolve remnants in this simulation -> Set all values to unknown
# time at which remnant properties are measured
final-time       = [unknown]

# mass of final BH (remnant)
remnant-mass     = [unknown]

# dimensionless spin of BH remnant
remnant-dimensionless-spin = [unknown]

# coordinate velocity of BH remnant
remnant-velocity = [unknown]

# mass outside black hole
disk-mass = [unknown]

# unbound mass passing through outer boundaries
ejecta-mass = [unknown]

#--------------------------------
# Code information
#--------------------------------

# version of this metadata file
metadata-version = 1

# unique, ordered list of revisions used for the evolution
spec-revisions  = c02c103233e97a037e4900fcc474577a451387ac

# revision used for the initial data creation
spells-revision = f1711ed27b495806b012750cace5ad78f99df063

