fixed reference errors
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@ -34,7 +34,7 @@ The *mesocnt* angle style uses the potential
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where :math:`\Delta \theta = \theta - \pi` is the bending angle of the nanotube, :math:`K_\text{H}` and :math:`K_\text{B}` are prefactors for the harmonic and linear regime respectively and :math:`\theta_\text{B}` is the buckling angle. Note that the usual 1/2 factor for the harmonic potential is included in :math:`K_\text{H}`.
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The style implements parametrisation presets of :math:`K_\text{H}`, :math:`K_\text{B}` and :math:`\theta_\text{B}` for mesoscopic simulations of
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carbon nanotubes based on the atomistic simulations of :ref:`(Zhigilei) <Zhigilei>` and buckling considerations of :ref:`(Volkov) <Volkov>`.
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carbon nanotubes based on the atomistic simulations of :ref:`(Srivastava) <Srivastava_2>` and buckling considerations of :ref:`(Zhigilei) <Zhigilei1_1>`.
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The following coefficients must be defined for each angle type via the
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:doc:`angle_coeff <angle_coeff>` command as in the examples above, or in
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@ -94,10 +94,10 @@ none
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----------
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.. _Zhigilei:
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.. _Srivastava_2:
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**(Zhigilei)** Zhigilei, Wei and Srivastava, Phys. Rev. B 71, 165417 (2005).
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**(Srivastava)** Zhigilei, Wei, Srivastava, Phys. Rev. B 71, 165417 (2005).
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.. _Volkov:
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.. _Zhigilei1_1:
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**(Volkov)** Volkov and Zhigilei, ACS Nano 4, 10, 6187–6195 (2010).
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**(Zhigilei)** Volkov and Zhigilei, ACS Nano 4, 6187 (2010).
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@ -31,7 +31,7 @@ The *mesocnt* bond style is a wrapper for the :doc:`harmonic <bond_harmonic>` st
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where :math:`r_0` is the equilibrium bond distance. Note that the usual 1/2
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factor is included in :math:`K`.
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The style implements parametrisation presets of :math:`K` for mesoscopic simulations of
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carbon nanotubes based on the atomistic simulations of :ref:`(Zhigilei) <Zhigilei>`.
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carbon nanotubes based on the atomistic simulations of :ref:`(Srivastava) <Srivastava_1>`.
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Other presets can be readily implemented in the future.
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@ -73,6 +73,6 @@ none
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----------
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.. _Zhigilei:
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.. _Srivastava_1:
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**(Zhigilei)** Zhigilei, Wei and Srivastava, Phys. Rev. B 71, 165417 (2005).
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**(Srivastava)** Zhigilei, Wei and Srivastava, Phys. Rev. B 71, 165417 (2005).
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