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The combinatorial model includes a detailed microscopic calculation of the intrinsic state density and of the rotational enhancement factor, but a phenomenological treatment of the vibrational effect.
Proton neutron quasi-particle random phase approximation (pn-QRPA) theory has recently being used for a microscopic calculation of stellar weak interaction rates of iron isotopes with success.
Recently the microscopic calculation of weak interaction mediated rates on key isotopes of iron was introduced using the proton neutron quasiparticle random phase approximation (pn-QRPA) theory with improved model parameters.
Excited state Gamow Teller distributions are much different from ground state and a microscopic calculation of decay rates from these excited states greatly increases the reliability of the total decay rate calculation specially during the late stages of stellar evolution.
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A general strategy for applying the method to specific systems is outlined, which includes microscopic model formulation, calculation of zero-temperature phase diagrams, numerical calculation of thermodynamic and structural quantities at non-zero temperatures, and estimation of effective, lateral interaction energies that cannot be obtained by first-principles methods.
The pn-QRPA theory allows a microscopic "state-by-state" calculation of stellar rates as explained later in text.
However, as discussed in Ref. [2] the microscopic interpretation and theoretical calculation of the surface optical response from first principles is still a challenging task.
While determining the macroscopic residual stress, M-RS, by diffraction methods is well known, the calculation of the microscopic residual stress, m-RS, which varies from grain to grain in single-phase alloys is still a pending task.
Collectively, all of these parameters allow the calculation of the microscopic protonation and deprotonation rate constants necessary for constructing the kinetic master equation (see section S.8 of the Supporting Information for details).
This is the first calculation of a microscopic ATPase coupling efficiency for nucleosome repositioning and also further supports our conclusion that a second bound ISWI does not contribute to the repositioning reaction.
Existence of an excess positive charge near the dot boundary has been directly confirmed by the microscopic first-principles calculations of Delerue et al. [16] and Trani et al. [18].
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