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* [1] Meineke, et al., J. Comp. Chem. 26, 252-271 (2005). |
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* [2] Fennell & Gezelter, J. Chem. Phys. 124, 234104 (2006). |
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* [3] Sun, Lin & Gezelter, J. Chem. Phys. 128, 24107 (2008). |
39 |
< |
* [4] Vardeman & Gezelter, in progress (2009). |
39 |
> |
* [4] Kuang & Gezelter, J. Chem. Phys. 133, 164101 (2010). |
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> |
* [5] Vardeman, Stocker & Gezelter, J. Chem. Theory Comput. 7, 834 (2011). |
41 |
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*/ |
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|
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#ifndef UTILS_PHYSICALCONSTANTS_HPP |
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#define UTILS_PHYSICALCONSTANTS_HPP |
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+ |
#include "config.h" |
46 |
+ |
#include <cmath> |
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|
|
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namespace OpenMD { |
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|
|
81 |
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* kcal mol^-1 Angstrom^-1 fs^-1 Kelvin^-1 |
82 |
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*/ |
83 |
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const RealType thermalConductivityConvert = 1.439326479e-5; |
84 |
+ |
|
85 |
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/* Atomic Units are used in the Slater overlap code, and we need |
86 |
+ |
* to get distances back and forth to angstroms and energies back |
87 |
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* and forth to kcal / mol |
88 |
+ |
*/ |
89 |
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const RealType angstromToBohr = 1.88972612; |
90 |
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const RealType bohrToAngstrom = 0.52917721092; |
91 |
+ |
const RealType hartreeToKcal = 627.509469; |
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} |
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} |
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#endif |