OpenMD 3.2
Molecular Dynamics in the Open
Loading...
Searching...
No Matches
VelocityField.hpp
Go to the documentation of this file.
1/*
2 * Copyright (c) 2004-present, The University of Notre Dame. All rights
3 * reserved.
4 *
5 * Redistribution and use in source and binary forms, with or without
6 * modification, are permitted provided that the following conditions are met:
7 *
8 * 1. Redistributions of source code must retain the above copyright notice,
9 * this list of conditions and the following disclaimer.
10 *
11 * 2. Redistributions in binary form must reproduce the above copyright notice,
12 * this list of conditions and the following disclaimer in the documentation
13 * and/or other materials provided with the distribution.
14 *
15 * 3. Neither the name of the copyright holder nor the names of its
16 * contributors may be used to endorse or promote products derived from
17 * this software without specific prior written permission.
18 *
19 * THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS "AS IS"
20 * AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE
21 * IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE
22 * ARE DISCLAIMED. IN NO EVENT SHALL THE COPYRIGHT HOLDER OR CONTRIBUTORS BE
23 * LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR
24 * CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF
25 * SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS
26 * INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN
27 * CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE)
28 * ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
29 * POSSIBILITY OF SUCH DAMAGE.
30 *
31 * SUPPORT OPEN SCIENCE! If you use OpenMD or its source code in your
32 * research, please cite the following paper when you publish your work:
33 *
34 * [1] Drisko et al., J. Open Source Softw. 9, 7004 (2024).
35 *
36 * Good starting points for code and simulation methodology are:
37 *
38 * [2] Meineke, et al., J. Comp. Chem. 26, 252-271 (2005).
39 * [3] Fennell & Gezelter, J. Chem. Phys. 124, 234104 (2006).
40 * [4] Sun, Lin & Gezelter, J. Chem. Phys. 128, 234107 (2008).
41 * [5] Vardeman, Stocker & Gezelter, J. Chem. Theory Comput. 7, 834 (2011).
42 * [6] Kuang & Gezelter, Mol. Phys., 110, 691-701 (2012).
43 * [7] Lamichhane, Gezelter & Newman, J. Chem. Phys. 141, 134109 (2014).
44 * [8] Bhattarai, Newman & Gezelter, Phys. Rev. B 99, 094106 (2019).
45 * [9] Drisko & Gezelter, J. Chem. Theory Comput. 20, 4986-4997 (2024).
46 */
47
48/*! \file perturbations/VelocityField.hpp
49 \brief Linear (homogeneous) ambient velocity field, queried at a location
50*/
51
52#ifndef PERTURBATIONS_VELOCITYFIELD_HPP
53#define PERTURBATIONS_VELOCITYFIELD_HPP
54
55#include "brains/SimInfo.hpp"
57#include "math/Vector3.hpp"
58#include "perturbations/VelocityFieldParameters.hpp"
59
60namespace OpenMD {
61
62 //! A linear (homogeneous) ambient velocity field, v(r) = v0 + K . r
63 /*! Built from a velocityField{ ... } block. The velocity gradient
64 \f$ K_{ij} = \partial v_i / \partial r_j \f$ is assembled from an
65 optional constant-stress (rate-of-strain) part and an optional
66 constant-vorticity part:
67
68 \f$ \mathsf{K} = \mathsf{E} + \mathsf{W}, \qquad
69 \mathsf{E} = \mathrm{sym}(\mathsf{K}), \quad
70 \mathsf{W} = \mathrm{antisym}(\mathsf{K}). \f$
71
72 Unlike the electric-field gradient in UniformGradient (which Laplace's
73 equation forces to be symmetric and traceless), K carries an
74 independent antisymmetric part. Because E is built traceless and W is
75 antisymmetric, this decomposed field is divergence-free by
76 construction (incompressible, \f$\nabla\cdot\mathbf{v}=0\f$).
77
78 This is a passive object: it is queried by the (Langevin /
79 hydrodynamic) integrator rather than registered as a ForceModifier.
80 Accessors expose the quantities the mobility coupling consumes: the
81 ambient velocity (leading drag), the rate of strain (stresslet), and
82 the vorticity / co-rotation rate (rotational coupling). Since the
83 flow is linear, \f$\nabla^2\mathbf{v}=0\f$ and the a^2/6 Faxen term
84 vanishes identically.
85
86 The velocity field can be applied by specifying one of these blocks in the
87 omd file:
88
89 \code{.unparsed}
90
91 // pure planar/uniaxial extension along x
92 velocityField {
93 useVelocityField = true;
94 strainRate = 1.0e-3; // fs^-1
95 strainDirection1 = (1, 0, 0);
96 strainDirection2 = (1, 0, 0);
97 }
98
99 // rigid rotation about z (vorticity only)
100 velocityField {
101 useVelocityField = true;
102 vorticity = (0, 0, 2.0e-3); // fs^-1
103 }
104
105 // background velocity field
106 velocityField {
107 useVelocityField = true;
108 backgroundVelocity = (0, 0, 1.0e-4); // Angstrom fs^-1
109 }
110
111 // simple shear v_x = gammaDot * y (equal strain + vorticity)
112 velocityField {
113 useVelocityField = true;
114 strainRate = 1.0e-3;
115 strainDirection1 = (1, 0, 0);
116 strainDirection2 = (0, 1, 0);
117 vorticity = (0, 0, -1.0e-3);
118 }
119 \endcode
120
121 This last block is important: simple shear is not a pure strain
122 or pure vorticity state — it's \f$ K_{xy} = \f$ split as \f$
123 E_{xy} = \dot{\gamma} / 2 \f$ plus \f$ \omega = -\dot{\gamma}
124 \f$, which is why both strain and vorticity appear.
125 */
126 class VelocityField {
127 public:
128 explicit VelocityField(SimInfo* info);
129
130 //! true when a valid velocityField{} block was supplied
131 bool isActive() const { return doVelocityField_; }
132
133 //! ambient velocity at position r: v0 + K . r
134 Vector3d getVelocity(const Vector3d& r) const { return v0_ + K_ * r; }
135
136 //! constant velocity gradient, K_ij = d v_i / d r_j
137 const Mat3x3d& getVelocityGradient() const { return K_; }
138
139 //! rate-of-strain tensor E = sym(K) (the constant-stress part)
140 const Mat3x3d& getRateOfStrain() const { return E_; }
141
142 //! spin tensor W = antisym(K)
143 const Mat3x3d& getSpin() const { return W_; }
144
145 //! vorticity vector, omega = curl v (the constant-vorticity part)
146 const Vector3d& getVorticity() const { return omega_; }
147
148 //! angular velocity an immersed sphere co-rotates with, omega / 2
149 Vector3d getAngularVelocity() const { return 0.5 * omega_; }
150
151 //! uniform background velocity v0
152 const Vector3d& getBackgroundVelocity() const { return v0_; }
153
154 private:
155 void initialize();
156
157 SimInfo* info_;
159
160 bool initialized_ {false};
161 bool doVelocityField_ {false};
162
163 Vector3d v0_ {V3Zero}; // uniform background velocity
164 Mat3x3d K_ {}; // velocity gradient
165 Mat3x3d E_ {}; // sym(K), rate of strain
166 Mat3x3d W_ {}; // antisym(K), spin
167 Vector3d omega_ {V3Zero}; // vorticity = curl v
168 };
169} // namespace OpenMD
170
171#endif // PERTURBATIONS_VELOCITYFIELD_HPP
Parsed contents of the velocityField{ ... } block.
One of the heavy-weight classes of OpenMD, SimInfo maintains objects and variables relating to the cu...
Definition SimInfo.hpp:96
const Mat3x3d & getSpin() const
spin tensor W = antisym(K)
const Mat3x3d & getVelocityGradient() const
constant velocity gradient, K_ij = d v_i / d r_j
Vector3d getAngularVelocity() const
angular velocity an immersed sphere co-rotates with, omega / 2
bool isActive() const
true when a valid velocityField{} block was supplied
const Mat3x3d & getRateOfStrain() const
rate-of-strain tensor E = sym(K) (the constant-stress part)
const Vector3d & getBackgroundVelocity() const
uniform background velocity v0
Vector3d getVelocity(const Vector3d &r) const
ambient velocity at position r: v0 + K . r
const Vector3d & getVorticity() const
vorticity vector, omega = curl v (the constant-vorticity part)
This basic Periodic Table class was originally taken from the data.cpp file in OpenBabel.