Warning
This documentation is for an old version of Cantera. You can find docs for newer versions here.
Before we can describe how to define phases, interfaces, and their components (elements, species, and reactions), we need to go over a few points about the mechanics of writing and processing input files.
An input file consists of entries and directives, both of which have a syntax much like functions. An entry defines an object—for example, a reaction, or a species, or a phase. A directive sets options that affect how the entry parameters are interpreted, such as the default unit system, or how certain errors should be handled.
Cantera’s input files follow the syntax rules for Python, so if you’re familiar with Python syntax you already understand many of the details and can probably skip ahead to Dimensional Values.
Entries have fields that can be assigned values. A species entry is shown below that has fields name and atoms (plus several others):
species(name='C60', atoms='C:60')
Most entries have some fields that are required; these must be assigned values, or else processing of the file will abort and an error message will be printed. Other fields may be optional, and take default values if not assigned.
An entry may be either a top-level entry or an embedded entry. Top-level entries specify a phase, an interface, an element, a species, or a reaction, and begin in the first (leftmost) column. Embedded entries specify a model, or a group of parameters for a top-level entry, and are usually embedded in a field of another entry.
The fields of an entry are specified in the form <field_name> = <value>, and may be listed on one line, or extend across several. For example, two entries for graphite are shown below. The first is compact:
stoichiometric_solid(name='graphite', species='C(gr)', elements='C', density=(2.2, 'g/cm3'))
and the second is formatted to be easier to read:
stoichiometric_solid(
name = 'graphite',
elements = 'C',
species = 'C(gr)',
density = (2.2, 'g/cm3')
)
Both are completely equivalent.
The species C(gr) that appears in the definition of the graphite phase is also defined by a top-level entry. If the heat capacity of graphite is approximated as constant, then the following definition could be used:
species(name='C(gr)',
atoms='C:1',
thermo=const_cp(t0=298.15,
h0=0.0,
s0=(5.6, 'J/mol/K'), # NIST
cp0=(8.43, 'J/mol/K'))) # Taylor and Groot (1980)
Note that the thermo field is assigned an embedded entry of type const_cp. Entries are stored as they are encountered when the file is read, and only processed once the end of the file has been reached. Therefore, the order in which they appear is unimportant.
The character # is the comment character. Everything to the right of this character on a line is ignored:
# set the default units
units(length = 'cm', # use centimeters for length
quantity = 'mol') # use moles for quantity
Strings may be enclosed in single quotes or double quotes, but they must match. To create a string containing single quotes, enclose it in double quotes, and vice versa. If you want to create a string to extend over multiple lines, enclose it in triple quotes:
string1 = 'A string.'
string2 = "Also a 'string'"
string3 = """This is
a
string too."""
The multi-line form is useful when specifying a phase containing a large number of species:
species = """ H2 H O O2 OH H2O HO2 H2O2 C CH
CH2 CH2(S) CH3 CH4 CO CO2 HCO CH2O CH2OH CH3O
CH3OH C2H C2H2 C2H3 C2H4 C2H5 C2H6 HCCO CH2CO HCCOH
N NH NH2 NH3 NNH NO NO2 N2O HNO CN
HCN H2CN HCNN HCNO HOCN HNCO NCO N2 AR C3H7
C3H8 CH2CHO CH3CHO """
A sequence of multiple items is specified by separating the items by commas and enclosing them in square brackets or parentheses. The individual items can have any type—strings, integers, floating-point numbers (or even entries or other lists). Square brackets are often preferred, since parentheses are also used for other purposes in the input file, but either can be used:
s0 = (3.5, 'J/mol/K') # these are
s0 = [3.5, 'J/mol/K'] # equivalent
Another way to specify the species C(gr) is shown here:
graphite_thermo = const_cp(t0=298.15,
h0=0.0,
s0=(5.6, 'J/mol/K'), # NIST
cp0=(8.43, 'J/mol/K')) # Taylor and Groot (1980)
species(name='C(gr)', atoms='C:1', thermo=graphite_thermo)
In this form, the const_cp entry is stored in a variable, instead of being directly embedded within the species entry. The thermo field is assigned this variable.
Variables can also be used for any other parameter type. For example, if you are defining several phases in the file, and you want to set them all to the same initial pressure, you could define a pressure variable:
P_initial = (2.0, 'atm')
and then set the pressure field in each embedded state entry to this variable.
Field names may be omitted if the values are entered in the order specified in the entry declaration. (Entry declarations are the text printed on a colored background in the following chapters.) It is also possible to omit only some of the field names, as long as these fields are listed first, in order, before any named fields.
For example, The first four entries below are equivalent, while the last two are incorrect and would generate an error when processed:
element(symbol="Ar", atomic_mass=39.948) # OK
element(atomic_mass=39.948, symbol='Ar') # OK
element('Ar', atomic_mass=39.948) # OK
element("Ar", 39.948) # OK
element(39.948, "Ar") # error
element(symbol="Ar", 39.948) # error
Normally, Cantera will make some checks for errors in the definitions of species and reactions, such as checking for duplicate reactions. To slightly speed up processing (if a mechanism has previously been validated), or in case of spurious validation errors, validation can be disabled using the validate() function. For example, to disable validation of reactions, add the following to the CTI file:
validate(reactions='no')
Many fields have numerical values that represent dimensional quantities—a pressure, or a density, for example. If these are entered without specifying the units, the default units (set by the units directive described in Setting the Default Units) will be used. However, it is also possible to specify the units for each individual dimensional quantity (unless stated otherwise). All that is required is to group the value in parentheses or square brackets with a string specifying the units:
pressure = 1.0e5 # default is Pascals
pressure = (1.0, 'bar') # this is equivalent
density = (4.0, 'g/cm3')
density = 4000.0 # kg/m3
Compound unit strings may be used, as long as a few rules are followed:
Examples of compound units:
A = (1.0e20, 'cm6/mol2/s') # OK
h = (6.626e-34, 'J-s') # OK
density = (3.0, 'g/cm3') # OK
A = (1.0e20, 'cm^6/mol/s') # error (^)
A = (1.0e20, 'cm6/mol2-s') # error ('s' should be in denominator)
density = (3.0, 'g-cm-3') # error (negative exponent)
The default unit system may be set with the units() directive. Note that unit conversions are not done until the entire file has been read. Only one units directive should be present in a file, and the defaults it specifies apply to the entire file. If the file does not contain a units directive, the default units are meters, kilograms, kilomoles, and seconds.
Shown below are two equivalent ways of specifying the site density for an interface. In the first version, the site density is specified without a units string, and so its units are constructed from the default units for quantity and length, which are set with a units directive:
units(length = 'cm', quantity = 'molec')
interface(name = 'Si-100',
site_density = 1.0e15, # molecules/cm2 (default units)
# ...
)
The second version uses a different default unit system, but overrides the default units by specifying an explicit units string for the site density:
units(length = 'cm', quantity = 'mol')
interface(name = 'Si-100',
site_density = (1.0e15, 'molec/cm2') # override default units
# ...
)
The second version is equivalent to the first, but would be very different if the units of the site density were not specified!
The length, quantity and time units are used to construct the units for reaction pre-exponential factors. The energy units are used for molar thermodynamic properties, in combination with the units for quantity.
Since activation energies are often specified in units other than those used for thermodynamic properties, a separate field is devoted to the default units for activation energies:
units(length = 'cm', quantity = 'mol', act_energy = 'kcal/mol')
kf = Arrhenius(A = 1.0e14, b = 0.0, E = 54.0) # E is 54 kcal/mol
See units() for the declaration of the units directive.
Cantera recognizes the following units in various contexts:
field | allowed values |
---|---|
length | 'cm', 'm', 'mm' |
quantity | 'mol', 'kmol', 'molec' |
time | 's', 'min', 'hr', 'ms' |
energy | 'J', 'kJ', 'cal', 'kcal' |
act_energy | 'kJ/mol', 'J/mol', 'J/kmol', 'kcal/mol', 'cal/mol', 'eV', 'K' |
pressure | 'Pa', 'atm', 'bar' |
From the point of view of the user, it appears that a Cantera application that imports a phase definition reads the input file, and uses the information there to construct the object representing the phase or interface in the application. While this is the net effect, it is actually a two-step process. When a function like importPhase is called to import a phase definition from a file, a preprocessor runs automatically to read the input file and create a string that contains the same information but in an XML-based format called CTML. After the preprocessor finishes, Cantera imports the phase definition from this CTML data.
Why two file formats? There are several reasons. XML is a widely-used standard for data files, and it is designed to be relatively easy to parse. This makes it possible for other applications to use Cantera CTML data files, without requiring the substantial chemical knowledge that would be required to use .cti files. For example, “web services” (small applications that run remotely over a network) are often designed to accept XML input data over the network, perform a calculation, and send the output in XML back across the network. Supporting an XML-based data file format facilitates using Cantera in web services or other network computing applications.
The difference between the high-level description in a .cti input file and the lower-level description in the CTML file may be illustrated by how reactions are handled. In the input file, the reaction stoichiometry and its reversibility or irreversibility are determined from the reaction equation. For example:
O + HCCO <=> H + 2 CO
specifies a reversible reaction between an oxygen atom and the ketenyl radical HCCO to produce one hydrogen atom and two carbon monoxide molecules. If <=> were replaced with =>, then it would specify that the reaction should be treated as irreversible.
Of course, this convention is not spelled out in the input file—the parser simply has to know it, and has to also know that a “reactant” appears on the left side of the equation, a “product” on the right, that the optional number in front of a species name is its stoichiometric coefficient (but if missing the value is one), etc. The preprocessor does know all this, but we cannot expect the same level of knowledge of chemical conventions by a generic XML parser.
Therefore, in the CTML file, reactions are explicitly specified to be reversible or irreversible, and the reactants and products are explicitly listed with their stoichiometric coefficients. The XML file is, in a sense, a “dumbed-down” version of the input file, spelling out explicitly things that are only implied in the input file syntax, so that “dumb” (i.e., easy to write) parsers can be used to read the data with minimal risk of misinterpretation.
The reaction definition:
reaction( "O + HCCO <=> H + 2 CO", [1.00000E+14, 0, 0])
in the input file is translated by the preprocessor to the following CTML text:
<reaction id="0028" reversible="yes">
<equation>O + HCCO [=] H + 2 CO</equation>
<rateCoeff>
<Arrhenius>
<A units="cm3/mol/s"> 1.000000E+14</A>
<b>0</b>
<E units="cal/mol">0.000000</E>
</Arrhenius>
</rateCoeff>
<reactants>HCCO:1 O:1</reactants>
<products>H:1 CO:2</products>
</reaction>
The CTML version is much more verbose, and would be much more tedious to write by hand, but is much easier to parse, particularly since it is not necessary to write a custom parser—virtually any standard XML parser, of which there are many, can be used to read the CTML data.
So in general files that are easy for knowledgeable users (you) to write are more difficult for machines to parse, because they make use of high-level application-specific knowledge and conventions to simplify the notation. Conversely, files that are designed to be easily parsed are tedious to write because so much has to be spelled out explicitly. A natural solution is to use two formats, one designed for writing by humans, the other for reading by machines, and provide a preprocessor to convert the human-friendly format to the machine-friendly one.
If you are interested in seeing the internals of how the preprocessing works, take a look at file ctml_writer.py in the Cantera Python package. Or simply start Python, and type:
>>> import cantera.ctml_writer
>>> help(cantera.ctml_writer)
The ctml_writer.py module can also be run as a script to convert input .cti files to CTML. For example, if you have an input file phasedefs.cti, then simply type at the command line:
python -m cantera.ctml_writer phasedefs.cti
to create CTML file phasedefs.xml. On systems which support running Python scripts directly, a script to run ctml_writer directly is also installed. If the Cantera bin directory is on your PATH, you can also do the conversion by running:
ctml_writer phasedefs.cti
This can be used to generate XML input files for use on systems where the Cantera Python package is not installed. Of course, most of the time creation of the CTML file will happen behind the scenes, and you will not need to be concerned with CTML files at all.
During processing of an input file, errors may be encountered. These could be syntax errors, or could be ones that are flagged as errors by Cantera due to some apparent inconsistency in the data—an unphysical value, a species that contains an undeclared element, a reaction that contains an undeclared species, missing species or element definitions, multiple definitions of elements, species, or reactions, and so on.
Syntax errors are caught by the Python preprocessor, not by Cantera, and must be corrected before proceeding further. Python prints a “traceback” that allows you to find the line that contains the error. For example, consider the following input file, which is intended to create a gas with the species and reactions of GRI-Mech 3.0, but has a misspelled the field name reactions:
ideal_gas(name = 'gas',
elements = 'H O',
species = 'gri30: all',
reactionss = 'gri30: all')
When this definition is imported into an application, an error message like the following would be printed to the screen, and execution of the program or script would terminate.
Traceback (most recent call last):
File "<stdin>", line 1, in <module>
File "/some/path/Cantera/importFromFile.py", line 18, in importPhase
return importPhases(file, [name], loglevel, debug)[0]
File "/some/path/Cantera/importFromFile.py", line 25, in importPhases
s.append(solution.Solution(src=file,id=nm,loglevel=loglevel,debug=debug))
File "/some/path/solution.py", line 39, in __init__
preprocess = 1, debug = debug)
File "/some/path/Cantera/XML.py", line 35, in __init__
self._xml_id = _cantera.xml_get_XML_File(src, debug)
cantera.error:
************************************************
Cantera Error!
************************************************
Procedure: ct2ctml
Error: Error converting input file "./gas.cti" to CTML.
Python command was: '/usr/bin/python'
The exit code was: 4
-------------- start of converter log --------------
TypeError on line 4 of './gas.cti':
__init__() got an unexpected keyword argument 'reactionss'
| Line |
| 1 | ideal_gas(name = 'gas',
| 2 | elements = 'H O',
| 3 | species = 'gri30: all',
> 4 > reactionss = 'gri30: all')
| 5 |
--------------- end of converter log ---------------
The top part of the error message shows the chain of functions that were called before the error was encountered. For the most part, these are internal Cantera functions not of direct concern here. The relevant part of this error message is the part starting with the “Cantera Error” heading, and specifically the contents of the converter log section. This message says that that on line 4 of gas.cti, the the keyword argument reactionss was not recognized. Seeing this message, it is clear that the problem is that reactions is misspelled.
Now let’s consider the other class of errors—ones that Cantera, not Python, detects. Continuing the example above, suppose that the misspelling is corrected, and the input file processed again. Again an error message results, but this time it is from Cantera:
cantera.error:
Procedure: installSpecies
Error: species C contains undeclared element C
The problem is that the phase definition specifies that all species are to be imported from dataset gri30, but only the elements H and O are declared. The gri30 datset contains species composed of the elements H, O, C, N, and Ar. If the definition is modified to declare these additional elements:
ideal_gas(name = 'gas',
elements = 'H O C N Ar',
species = 'gri30: all',
reactions = 'gri30: all')
it may be imported successfully.
Errors of this type do not have to be fatal, as long as you tell Cantera how you want to handle them. You can, for example, instruct Cantera to quietly skip importing any species that contain undeclared elements, instead of flagging them as errors. You can also specify that reactions containing undeclared species (also usually an error) should be skipped. This allows you to very easily extract a portion of a large reaction mechanism, as described in Special Processing Options.
Many existing reaction mechanism files are in “CK format,” by which we mean the input file format developed for use with the Chemkin-II software package as specified in the report describing the Chemkin software [SAND89].
Cantera comes with a converter utility program ck2cti (or ck2cti.py) that converts CK format into Cantera format. This program should be run from the command line first to convert any CK files you plan to use into Cantera format (CTI format).
Usage:
ck2cti [--input=<filename>]
[--thermo=<filename>]
[--transport=<filename>]
[--id=<phase-id>]
[--output=<filename>]
[--permissive]
[-d | --debug]
Each of the terms in square brackets is an option that can be passed on the command line to ck2cti. --input is the chemistry input file, containing a list of all the element names that are used, a list of all the species names, and a list of all the reactions to be considered between the species. This file can also optionally contain thermodynamic information for the species. If the --input file does not contain the thermodynamic data, a separate file containing this information must be specified to the --thermo` option. Finally, the --input file can also optionally contain transport information for the species. If it does not, and the user wishes to use a part of Cantera that relies on some transport properties, the --transport option must be used to specify the file containing all the transport data for the species.
Example:
ck2cti --input=chem.inp --thermo=therm.dat --transport=tran.dat
If the output file name is not given, an output file with the same name as the input file, with the extension changed to ‘.cti’.
An input file containing only species definitions (which can be referenced from phase definitions in other input files) can be created by specifying only a thermo file.
Many existing CK format files cause errors in ck2cti when they are processed. Some of these errors may be avoided by specifying the --permissive option. This option allows certain recoverable parsing errors (e.g. duplicate transport or thermodynamic data) to be ignored. Other errors may be caused by incorrect formatting of lines in one or more of the input files.
When ck2cti encounters an error, it attempts to print the surrounding information to help you to locate the error. Many of the most common errors are due to an inconsistency of the input files from their standard, as defined in the report for Chemkin referenced above. These errors include:
Each section of the input files must be started with a keyword representing that section and ending with the keyword END. Keywords that may begin a section include:
- ELEMENTS or ELEM
- SPECIES or SPEC
- THERMO or THERMO ALL
- REACTIONS or REAC
- TRANSPORT
The thermodynamic data is read in a fixed format. This means that each column of the input has a particular meaning. Many common errors are generated because information is missing or in the wrong column. Check thoroughly for extraneous or missing spaces. The format for each thermodynamic entry should be as follows:
N2 N 2 G200.000 6000.000 1000.00 1 2.95258000E+00 1.39690000E-03-4.92632000E-07 7.86010000E-11-4.60755000E-15 2 -9.23949000E+02 5.87189000E+00 3.53101000E+00-1.23661000E-04-5.02999000E-07 3 2.43531000E-09-1.40881000E-12-1.04698000E+03 2.96747000E+00 4The following table is adapted from the Chemkin manual [SAND89] to describe the column positioning of each required part of the entry. Empty columns should be filled with spaces.
Line No. Contents Column 1 Species Name 1–18 1 Date (Optional) 19–24 1 Atomic Symbols and formula 25–44 1 Phase of species (S, L, G) 45 1 Low temperature 46–55 1 High temperature 56–65 1 Common temperature 66–73 1 Additional Atomic Symbols 74–78 1 The integer 1 80 2 Coefficients \(a_1\) to \(a_5\) for the upper temperature interval 1–75 2 The integer 2 80 3 Coefficients \(a_6,\ a_7\) for the upper temperature interval, and \(a_1,\ a_2,\ a_3\) for the lower temperature interval 1–75 3 The integer 3 80 4 Coefficients \(a_4\) through \(a_7\) for the lower temperature interval 1–60 4 The integer 4 80 The first 18 columns are reserved for the species name. The name assigned to the species in the thermodynamic data must be the same as the species name defined in the SPECIES section. If the species name is shorter than 18 characters, the rest of the characters should be filled by spaces. The next six columns (columns 19–24) are typically used to write a date; they are not used further. The next 20 columns (25–44) are used to specify the elemental composition of the species. In column 45, the phase of the species (S, L, or G for solid, liquid, or gas respectively) should be specified. The next 28 columns are reserved for the temperatures that delimit the ranges of the polynomials specified on the next several lines. The first two temperatures have a width of 10 columns each (46–55 and 56–65), and represent the lowest temperature and highest temperature for which the polynomials are valid. The last temperature has a width of 8 columns (66–73) and is the “common” temperature, where the switch from low to high occurs. The next 5 columns (74–78) are reserved for atomic symbols and are usually left blank for the default behavior. Column 79 is blank and finally, the row is ended in column 80 with the integer 1.
The next three lines of the thermodynamic entry have a similar format. They contain the coefficients of the polynomial described in Thermodynamic Property Models for the NASA 7-coefficient polynomial formulation. The second row of the thermo entry (the first after the information row) contains the first five coefficients that apply the the temperature range between the midpoint and the upper limit. 15 columns are alloted for each coefficient (for a total of 75 columns), with no spaces between them. Although the entry above shows spaces between positive coefficients, it is to be noted that this is done only for formatting consistency with other lines that contain negative numbers. After the coefficients, four spaces in columns 76–79 are followed by the integer 2 in column 80. On the next line, the last two coefficients for the upper temperature range and the first three coefficients for the lower temperature range are specified. Once again, this takes up the first 75 columns, columns 76–79 are blank, and the integer 3 is in column 80. Finally, on the last line of a particular entry, the last four coefficients of the lower temperature range are specified in columns 1–60, 19 blank spaces are present, and the integer 4 is in column 80. The 19 blank spaces in the last line are part of the standard. However, since the original Chemkin interpreter ignored those spaces, researchers began using that space to store additional information that was not necessary for the input file. Although these numbers create an error in ck2cti if present, they are harmless and can be ignored by using the --permissive option.
It may be the case that scientific formatted numbers are missing the E. In this case, numbers often show up as 1.1+01, when they should be 1.1E+01. You can fix this with a simple Regular Expression find and replace:
Find: (\d+\.\d+)([+-]\d+) Replace: \1E\2The transport data file also has a specified format, as described in [SAND98], although the format is not as strict as for the thermodynamic entries. In particular, the first 15 columns of a line are reserved for the species name. One common source of errors is a species that is present in the transport data file, but not in the thermodynamic data or in the species list; or a species that is present in the species list but not the transport data file. The rest of the columns on a given line have no particular format, but must be present in the following order:
Parameter Number Parameter Name 1 An integer with value 0, 1, or 2 indicating monatomic, linear, or non-linear molecular geometry. 2 The Lennerd-Jones potential well depth \(\varepsilon/k_B\) in Kelvin 3 The Lennerd-Jones collision diameter \(\sigma\) in Angstrom 4 The dipole moment \(\mu\) in Debye 5 The polarizability \(\alpha\) in Angstrom 6 The rotational relaxation collision number \(Z_{rot}\) at 298 K Another common error is if all 6 of these numbers are not present for every species.
[SAND89] | (1, 2) See R. J. Kee, F. M. Rupley, and J. A. Miller, Sandia National Laboratories Report SAND89-8009 (1989). http://www.osti.gov/scitech/biblio/5681118 |
[SAND98] | See R. J. Kee, G. Dixon-Lewis, J. Warnatz, M. E. Coltrin, J. A. Miller, H. K. Moffat, Sandia National Laboratories Report SAND86-8246B (1998). |