Skip to content

Releases: AMReX-Astro/Microphysics

Release 20.08

01 Aug 13:15
Compare
Choose a tag to compare
  • Several of the unit tests had separate C++ and Fortran
    implementions. These have been unified (#343, #344, #345)

  • The VBDF integrator was removed (#348)

  • VODE can now reject an internal timestep that has any abundance
    change by more than a factor of 2, or an abundance < 0 or > 1,
    as well as timesteps where the temperature ends up negative. (#350)

Microphysics 20.07

01 Jul 12:53
Compare
Choose a tag to compare

20.07

  • The "master" branch has been renamed "main" (#333)

  • NETWORK_PROPERTIES now includes the number of Aux quantities (#330)

Microphysics 20.06

01 Jun 12:24
Compare
Choose a tag to compare

20.06

  • For integration with simplified SDC, we now interpret atol_spec
    as an absolute tolerance on X alone instead of (rho X) (#311)

  • burn_cell can now use the C++ burner if compiled with
    USE_CXX_REACTIONS=TRUE and run with do_cxx = 1. (#313)

  • The original burn_cell (which used the F90 BoxLib build system)
    is removed and replaced with burn_cell_C (which uses the newer
    build system). (#316)

  • The analytic Jacobian with simplified SDC now is written in terms
    of the conserved fluid state and works for a wide range of
    problems (#228)

Microphysics 20.05

01 May 12:59
Compare
Choose a tag to compare

20.05

  • We now have an option for using sparse storage for aprox13 in C++
    (#307)

  • iso7 and aprox13 are now available as a C++ network (#303, 305)

  • species names are available as an enum in network_properties.H (#304)

  • The screening on O16+O16 in iso7 was fixed (#302)

  • The VODE integrator is now available in C++ (#299)

Microphysics 20.04.1

06 Jun 03:48
Compare
Choose a tag to compare
Microphysics 20.04.1

Microphysics 20.04

01 Apr 13:13
Compare
Choose a tag to compare

20.04

  • The wion network property was removed (#294)

  • There are new unit tests for the screening and aprox rates
    modules (both C++ and Fortran interfaces).

  • The screening routines were ported to C++ (#290) and the screenz
    routine was removed in favor of screen5 (#293)

  • a new method, is_input_valid, was added to all EOSes (both C++
    and Fortran interfaces) that can be used to query whether an EOS
    supports a particular input mode (e.g. eos_input_rp). (#291)

  • The aprox rates used with iso7, aprox13, aprox19, and aprox21
    have been converted to C++ (#288)

  • We've rewritten the VODE integrator to remove all "go to"
    statements (#275, 276, 278, 280, 281, 282, 283, 284, 285, 286,
    287)

  • We removed the ability to have nspec_evolve < nspec. This
    feature was not widely used and greatly complicated the code
    paths.(#279)

Microphysics 20.03

01 Mar 19:18
Compare
Choose a tag to compare

20.03

  • The nuclei information for both Fortran and C++ is now
    automatically generated from a network inputs file at compile
    time. As part of this change, 1/A is precomputed and stored as a
    constant (#253, 258).

  • The license for StarKiller Microphyscs was made explicit and
    a license.txt file was added (#267)

  • A framework for pure C++ EOSes has been created and a pure C++
    unit test, test_eos_C, is available to test these. (#246) The
    following EOSes have been ported to C++: ztwd (#268), multigamma
    (#265), polytrope (#264), gamma_law (#263), helmholtz (#262),
    gamma_law_general (#246), rad_power_law (#269), breakout (#270)

  • The GPackage.mak files that were a remnant of the old
    BoxLib F90 build system have been removed. They were
    not maintained. (#212).

  • All of the interface files have been collected together
    in the interfaces/ dir. (#240)

  • The network C++ headers have been renamed network_properties.H
    and the nuclei information (aion and zion) have been
    added. (#244)

Microphysics 20.02

01 Feb 19:28
Compare
Choose a tag to compare

20.02

  • Added a C++ header file, actual_network.H, that defines the
    network size. This is the start of making making the
    microphysics routines available in C++.

  • regenerated the pynucastro networks with the latest weak rate
    formulations from pynucastro.

Microphysics 20.01

01 Jan 18:47
Compare
Choose a tag to compare

20.01

  • The burn_t type no longer includes ydot or jac -- this allows
    us to optimize the memory access on GPUs (#220)

  • The original VODE integrator was removed and the Fortran 90
    version VODE90 was renamed to VODE. (#221)

  • The test_react unit tests no longer require a composition inputs
    file (xin*). They now create the composition profile at runtime.
    (#211)

Microphysics 19.12

02 Dec 14:28
Compare
Choose a tag to compare
  • Simplified SDC integration now uses the same retry strategy
    as the default (non-SDC) integration. (#215)

  • VODE90 can now participate in the retry strategy that was
    previously available to the VODE integrator, where it can
    switch to the BS integrator if loosening the tolerances
    does not allow the burn to complete. (#201)

  • The parameter ode_max_steps was made consistent in VODE and
    VODE90; in some places it was being ignored. (#214)

  • The helmholtz EOS was restructured, splitting the different
    components into different functions and optimizing the memory
    accesses. (#200)

  • The derivatives with respect to mass fraction (dpdX, dedX, dhdX)
    were removed from eos_t and are now available through a new type,
    eos_xderivs_t and the composition_derivatives() routine. (#207)

  • A bug in the screening of the C12+C12 and O16+O16 rates in iso7
    was fixed.

  • The test_eos unit test now outputs all of the variables in the
    eos_t type.