<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">NS</journal-id><journal-title-group><journal-title>Natural Science</journal-title></journal-title-group><issn pub-type="epub">2150-4091</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ns.2015.713061</article-id><article-id pub-id-type="publisher-id">NS-62402</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Biomedical&amp;Life Sciences</subject><subject> Chemistry&amp;Materials Science</subject><subject> Earth&amp;Environmental Sciences</subject><subject> Medicine&amp;Healthcare</subject><subject> Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Group-Invariant Solutions for the Generalised Fisher Type Equation
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>irsten</surname><given-names>Louw</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Raseelo</surname><given-names>J. Moitsheki</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>School of Computer Science and Applied Mathematics, University of the Witwatersrand, Johannesburg, 
South Africa</addr-line></aff><pub-date pub-type="epub"><day>10</day><month>12</month><year>2015</year></pub-date><volume>07</volume><issue>13</issue><fpage>613</fpage><lpage>624</lpage><history><date date-type="received"><day>30</day>	<month>October</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>27</month>	<year>December</year>	</date><date date-type="accepted"><day>30</day>	<month>December</month>	<year>2015</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  In this paper, we construct the group-invariant (exact) solutions for the generalised Fisher type equation using both classical Lie point and the nonclassical symmetry techniques. The generalised Fisher type equation arises in theory of population dynamics. The diffusion term and coefficient of the source term are given as the power law functions of the spatial variable. We introduce the modified Hopf-Cole transformation to simplify a nonlinear second Order Ordinary Equation (ODE) into a solvable linear third order ODE.
 
</p></abstract><kwd-group><kwd>Symmetry Methods</kwd><kwd> Modified Hopf-Cole Transformation</kwd><kwd> Fisher Type Equation</kwd><kwd> Exact Solutions</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>In this paper, the focus is on the generalised Fisher type equation arising in population dynamics. The analysis of the generalised Fisher equation has been carried out using Lie point symmetries (see e.g. [<xref ref-type="bibr" rid="scirp.62402-ref1">1</xref>] ) and construction of conservation laws see e.g. [<xref ref-type="bibr" rid="scirp.62402-ref2">2</xref>] ). These types of equations have appeared in many fields of study, for example, the reaction-diffusion equations arise in heat transfer problems [<xref ref-type="bibr" rid="scirp.62402-ref3">3</xref>] , biology [<xref ref-type="bibr" rid="scirp.62402-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.62402-ref5">5</xref>] , and transmission of nerve signals [<xref ref-type="bibr" rid="scirp.62402-ref6">6</xref>] . The reaction-diffusion equations such as the generalized Fisher equation describe how the concentra- tion of a substance is distributed in space changes, whereby the diffusion term causes the spread over the surface. Fisher [<xref ref-type="bibr" rid="scirp.62402-ref4">4</xref>] had used a nonlinear reaction-diffusion equation to model the population growth of mutant genes over a period of time. One can take Fisher’s equation [<xref ref-type="bibr" rid="scirp.62402-ref4">4</xref>] and with simple modifications, and can derive the Fitzhugh- Nagumo equation [<xref ref-type="bibr" rid="scirp.62402-ref7">7</xref>] . Moreover, one can make a modification to the Fitzhugh-Nagumo equation in order to obtain Huxley’s equation [<xref ref-type="bibr" rid="scirp.62402-ref4">4</xref>] .</p><p>A significant amount of work has been done in the process of studying the reaction-diffusion equations. In particular, from the classical Lie symmetry analysis point of view (see e.g. [<xref ref-type="bibr" rid="scirp.62402-ref8">8</xref>] ), and nonclassical symmetry techniques [<xref ref-type="bibr" rid="scirp.62402-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.62402-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.62402-ref10">10</xref>] . It turns out that reaction diffusion equations such as the generalised Fisher equation admit the genuine nonclassical symmetries if the source term is given by a cubic (see e.g. [<xref ref-type="bibr" rid="scirp.62402-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.62402-ref10">10</xref>] ). In a recent work [<xref ref-type="bibr" rid="scirp.62402-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.62402-ref11">11</xref>] , the authors assume a diffusivity which depends on space variable. In this case, the diffusivity may be given as a power law function of space variable for the given reaction-diffusion equation to admit non- classical symmetries.</p><p>This paper is arranged as follows. In Section 2, we provide the mathematical models for problems arising in population dynamics. In Section 3, we provide a brief account of the symmetry methods. In Sections 4 and 5, we provide the nonclassical and classical Lie point symmetry reductions, respectively. In Section 6, we briefly provide remarks on the conservation laws of the equation in question. The discussions and concluding remarks are given in Section 7.</p></sec><sec id="s2"><title>2. Mathematical Description</title><p>For a diploid population having two available alleles at the locus in question (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x6.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x7.png" xlink:type="simple"/></inline-formula>), there are three possible genotypes;<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x8.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x9.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x10.png" xlink:type="simple"/></inline-formula>, where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x11.png" xlink:type="simple"/></inline-formula> is the allele is under observation. Then, the following three equation describe the change in the genotype frequencies<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x12.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x13.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x14.png" xlink:type="simple"/></inline-formula>,</p><disp-formula id="scirp.62402-formula1481"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x15.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x16.png" xlink:type="simple"/></inline-formula> are the reproductive success rate of genotype <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x17.png" xlink:type="simple"/></inline-formula> <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x18.png" xlink:type="simple"/></inline-formula> is the common death rate, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x19.png" xlink:type="simple"/></inline-formula>is the total population density, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x20.png" xlink:type="simple"/></inline-formula>, and u is the frequency of allele<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x21.png" xlink:type="simple"/></inline-formula>. The frequency of allele <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x22.png" xlink:type="simple"/></inline-formula> is given by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x22.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x23.png" xlink:type="simple"/></inline-formula>. Note that u depends on t and x. The frequency of allele <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x22.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x24.png" xlink:type="simple"/></inline-formula> is</p><disp-formula id="scirp.62402-formula1482"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x25.png"  xlink:type="simple"/></disp-formula><p>Differentiating Equation (2) with respect to t, then the three genotype equations (1) collapse into a single equation that describes the change in frequency of the new mutant gene</p><disp-formula id="scirp.62402-formula1483"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x26.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x27.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x28.png" xlink:type="simple"/></inline-formula>. Equation (3) is a reaction-diffusion-convection equation with cubic nonlinearities referred to here as a generalised Fisher equation. If<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x29.png" xlink:type="simple"/></inline-formula>, the total population density is</p><p>constant in space, Equation (3) reduces to the Fitzhugh-Nagumo equation. When deriving the models with the continuous method, there is an extra convective term due to the assumption that total population density is not uniform spatially.</p><p>If one is to consider the conditions that Fisher had examined, so that the allele in question is completely recessive. This implies that the genotypes <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x30.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x31.png" xlink:type="simple"/></inline-formula> have the same phenotype, therefore they have the same reproductive success rate. Let the alleles represented by A and a be set as the alleles <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x32.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x32.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x33.png" xlink:type="simple"/></inline-formula> respectively. Hence, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x32.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x33.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x34.png" xlink:type="simple"/></inline-formula>is the allele under consideration. If <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x32.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x33.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x34.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x35.png" xlink:type="simple"/></inline-formula> the one obtains</p><disp-formula id="scirp.62402-formula1484"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x36.png"  xlink:type="simple"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x37.png" xlink:type="simple"/></inline-formula>. One can see that Equation (4) is also a reaction-diffusion-convection equation. If<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x38.png" xlink:type="simple"/></inline-formula>, then Equation (4) reduces to a generalized Fisher type equation,</p><disp-formula id="scirp.62402-formula1485"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x39.png"  xlink:type="simple"/></disp-formula><p>which models the propagation of impulses along nerve axons. In this paper we focus on the reaction diffusion equation of the form</p><disp-formula id="scirp.62402-formula1486"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x40.png"  xlink:type="simple"/></disp-formula><p>We refer to Equation (6) as the governing equation. The variable u may be viewed as representing population. The diffusivity <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x41.png" xlink:type="simple"/></inline-formula> may be given by quadratic in x for equations such as Equation (6) to admit genuine nonclassical symmetries (see e.g. [<xref ref-type="bibr" rid="scirp.62402-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.62402-ref11">11</xref>] ). In this paper the coefficient of the cubic source term <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x42.png" xlink:type="simple"/></inline-formula> is given by the power law <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x43.png" xlink:type="simple"/></inline-formula> where n is a real constant.</p></sec><sec id="s3"><title>3. Symmetry Methods for Differential Equations</title><p>In this section, we restrict discussions to symmetry analysis of second order differential equations. Given for example, a second order differential equation of the form</p><disp-formula id="scirp.62402-formula1487"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x44.png"  xlink:type="simple"/></disp-formula><p>where the subscripts denote all possible first and second derivatives of u with respect to t and x. Finding classical Lie point symmetries of Equation (7) implies seeking infinitesimal transformations of the form</p><disp-formula id="scirp.62402-formula1488"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x45.png"  xlink:type="simple"/></disp-formula><p>generated by the vector field</p><disp-formula id="scirp.62402-formula1489"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x46.png"  xlink:type="simple"/></disp-formula><p>Note that the transformations in (8) are equivalent to the one-parameter Lie group of transformations that leaves the Equation (7) unchanged or invariant. The action of X is extended to all derivatives appearing in the equation in question through the appropriate prolongation. The infinitesimal criterion for invariance of the given equation is given by</p><disp-formula id="scirp.62402-formula1490"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x47.png"  xlink:type="simple"/></disp-formula><p>Equation (10) yields an overdetermined system of linear homogeneous equation which can be solved algorithmically. Note that the solution of Equation (10) yield the classical Lie point symmetries admitted by Equation (7). Full theory of determination of Lie point symmetries may be obtain in among other texts [<xref ref-type="bibr" rid="scirp.62402-ref12">12</xref>] - [<xref ref-type="bibr" rid="scirp.62402-ref14">14</xref>] . If the invariance is sought subject to a further constraint</p><disp-formula id="scirp.62402-formula1491"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x48.png"  xlink:type="simple"/></disp-formula><p>known as the invariant surface condition (ISC), that is given</p><disp-formula id="scirp.62402-formula1492"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x49.png"  xlink:type="simple"/></disp-formula><p>then one obtain a system of nonlinear determining equations which may yield the nonclassical symmetry generators [<xref ref-type="bibr" rid="scirp.62402-ref15">15</xref>] .</p></sec><sec id="s4"><title>4. Nonclassical Symmetry Reductions</title><p>In this section, we consider nonclassical symmetry reductions of the generalised Fisher type equation given in Equation (6). Here, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x50.png" xlink:type="simple"/></inline-formula>is given as a cubic function of u (see e.g. [<xref ref-type="bibr" rid="scirp.62402-ref7">7</xref>] ) and both the diffusivity and the coefficient of the source term are given by power law functions of the space variable.</p><sec id="s4_1"><title>4.1. Nonclassical Symmetry Reduction Given n = 1</title><p>In this subsection, we consider Equation (6) with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x51.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x52.png" xlink:type="simple"/></inline-formula> Assuming<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x52.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x53.png" xlink:type="simple"/></inline-formula>, the infinitesimal criterion for invariance of the form (12) results in a system of overdetermined nonlinear determining equations which is split in the powers of in powers of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x52.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x54.png" xlink:type="simple"/></inline-formula> as given below;</p><p>1:</p><disp-formula id="scirp.62402-formula1493"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x55.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x56.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.62402-formula1494"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x57.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x58.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.62402-formula1495"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x59.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x60.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.62402-formula1496"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x61.png"  xlink:type="simple"/></disp-formula><p>The solution of these determining equations yields the admitted nonclassical symmetry generator given by</p><disp-formula id="scirp.62402-formula1497"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x62.png"  xlink:type="simple"/></disp-formula><p>The associated ISC is given by</p><disp-formula id="scirp.62402-formula1498"><label>(14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x63.png"  xlink:type="simple"/></disp-formula><p>Using governing equation and the ISC (14) simultaneously one may eliminate <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x64.png" xlink:type="simple"/></inline-formula> to get the equation</p><disp-formula id="scirp.62402-formula1499"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x65.png"  xlink:type="simple"/></disp-formula><p>Employing a change of variables <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x66.png" xlink:type="simple"/></inline-formula> then Equation (15) reduces to</p><disp-formula id="scirp.62402-formula1500"><label>(16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x67.png"  xlink:type="simple"/></disp-formula><p>We introduce the “modified” Hopf-Cole transformation given by</p><disp-formula id="scirp.62402-formula1501"><label>(17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x68.png"  xlink:type="simple"/></disp-formula><p>to simplify Equation (16). Upon substituting (17) into Equation (16), it turns out that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x69.png" xlink:type="simple"/></inline-formula> must satisfy an algebraic equation</p><disp-formula id="scirp.62402-formula1502"><label>(18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x70.png"  xlink:type="simple"/></disp-formula><p>Hence</p><disp-formula id="scirp.62402-formula1503"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x71.png"  xlink:type="simple"/></disp-formula><p>and so Equation (16) transforms to a linear third ODE</p><disp-formula id="scirp.62402-formula1504"><label>(19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x72.png"  xlink:type="simple"/></disp-formula><p>The solution to Equation (19) is given by</p><disp-formula id="scirp.62402-formula1505"><label>(20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x73.png"  xlink:type="simple"/></disp-formula><p>Substituting backwards for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x74.png" xlink:type="simple"/></inline-formula>, produces</p><disp-formula id="scirp.62402-formula1506"><label>(21)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x75.png"  xlink:type="simple"/></disp-formula><p>Solving for the arbitrary functions, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x76.png" xlink:type="simple"/></inline-formula>, Equation (21) is substituted back into the ISC given by Equation (14). Hence, we obtain in terms of the original variables the general nonclassical symmetry exact solution given by</p><disp-formula id="scirp.62402-formula1507"><label>(22)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x77.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x78.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x79.png" xlink:type="simple"/></inline-formula> are arbitrary constants. Solutions (22) is depicted in Figures 1-3.</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Population frequency over time and space given solution (22). Here, the parameters are given by<img data-original="http://html.scirp.org/file/4-8302663x81.png" /></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-8302663x80.png"/></fig><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Population dynamics as time progresses over space given solution (22). Here, the parameters are given by<img data-original="http://html.scirp.org/file/4-8302663x83.png" /></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-8302663x82.png"/></fig><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Impact on the population frequency as time evolves given solution (22). Here, the parameters are given by<img data-original="http://html.scirp.org/file/4-8302663x85.png" /></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-8302663x84.png"/></fig><p>If the source term is given by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x86.png" xlink:type="simple"/></inline-formula> then<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x86.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x87.png" xlink:type="simple"/></inline-formula>, gives rise to the equation</p><disp-formula id="scirp.62402-formula1508"><label>(23)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x88.png"  xlink:type="simple"/></disp-formula><p>In this case, the exact (group-invariant) solution will be given by,</p><disp-formula id="scirp.62402-formula1509"><label>(24)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x89.png"  xlink:type="simple"/></disp-formula></sec><sec id="s4_2"><title>4.2. Nonclassical Symmetry Reduction Given n &#185; 1</title><p>Suppose that one considers a more general case, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x90.png" xlink:type="simple"/></inline-formula>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x90.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x91.png" xlink:type="simple"/></inline-formula>. The governing equation then becomes</p><disp-formula id="scirp.62402-formula1510"><label>(25)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x92.png"  xlink:type="simple"/></disp-formula><p>Following the steps above, the admitted genuine nonclassical symmetry is given by</p><disp-formula id="scirp.62402-formula1511"><label>(26)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x93.png"  xlink:type="simple"/></disp-formula><p>The associated ISC is given by</p><disp-formula id="scirp.62402-formula1512"><label>(27)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x94.png"  xlink:type="simple"/></disp-formula><p>Eliminating <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x95.png" xlink:type="simple"/></inline-formula> using (25) and (27) one obtains</p><disp-formula id="scirp.62402-formula1513"><label>(28)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x96.png"  xlink:type="simple"/></disp-formula><p>Introducing the transformation <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x97.png" xlink:type="simple"/></inline-formula> yields</p><disp-formula id="scirp.62402-formula1514"><label>(29)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x98.png"  xlink:type="simple"/></disp-formula><p>In this case, it turns out that the “modified” Hopf-Cole transformation should be given by</p><disp-formula id="scirp.62402-formula1515"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x99.png"  xlink:type="simple"/></disp-formula><p>as such the transformed Equation (29) becomes a solvable linear third order ODE</p><disp-formula id="scirp.62402-formula1516"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x100.png"  xlink:type="simple"/></disp-formula><p>In terms of the original variables the exact solution is given by</p><disp-formula id="scirp.62402-formula1517"><label>(30)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x101.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x102.png" xlink:type="simple"/></inline-formula> are arbitrary functions of t. Without loss of generality, set <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x103.png" xlink:type="simple"/></inline-formula> and then solving for the rest of the arbitrary functions by substituting Equation (30) into the ISC corresponding to this case. Then, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x103.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x104.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x103.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x104.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x105.png" xlink:type="simple"/></inline-formula> can be found to be</p><disp-formula id="scirp.62402-formula1518"><label>(31)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x106.png"  xlink:type="simple"/></disp-formula><p>or</p><disp-formula id="scirp.62402-formula1519"><label>(32)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x107.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.62402-formula1520"><label>(33)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x108.png"  xlink:type="simple"/></disp-formula><p>If<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x109.png" xlink:type="simple"/></inline-formula>, then the problem is equivalent to the one considered in [<xref ref-type="bibr" rid="scirp.62402-ref3">3</xref>] and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x109.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x110.png" xlink:type="simple"/></inline-formula> yields the problem discussed in the previous section.</p></sec></sec><sec id="s5"><title>5. Classical Lie Point Symmetry Reductions</title><sec id="s5_1"><title>5.1. Classical Lie Point Symmetry Reductions Given n = 1</title><p>We consider the case where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x111.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x111.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x112.png" xlink:type="simple"/></inline-formula> in Equation (6). In this case the admitted Lie algebra is three dimensional and spanned by the vector fields</p><disp-formula id="scirp.62402-formula1521"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x113.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.62402-formula1522"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x114.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.62402-formula1523"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x115.png"  xlink:type="simple"/></disp-formula><p>It is easy to show that this Lie algebra is closed. Reductions are possible by any linear combination of these symmetries. Usually one may determine the optimal system of subalgebras of these classical Lie point symmetries to determine reductions which are not connected by any point transformation. However here we restrict analysis to three cases only. Note that symmetry generator <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x116.png" xlink:type="simple"/></inline-formula> led to hard to solve reductions and thus its use is omitted.</p><sec id="s5_1_1"><title>5.1.1. Reduction by X<sub>2</sub></title><p>The corresponding characteristic equations corresponding to this scaling symmetry are given by</p><disp-formula id="scirp.62402-formula1524"><label>(34)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x117.png"  xlink:type="simple"/></disp-formula><p>and the functional form of thew group-invariant solutions is given by</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x118.png" xlink:type="simple"/></inline-formula>where f satisfies the ODE<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x118.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x119.png" xlink:type="simple"/></inline-formula> (35)We obtain<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x118.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x119.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x120.png" xlink:type="simple"/></inline-formula> (36)and so, the group-invariant solution for the governing equation is given by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x118.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x119.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x120.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x121.png" xlink:type="simple"/></inline-formula> (37)The solution in Equation (37) is depicted in <xref ref-type="fig" rid="fig4">Figure 4</xref> and <xref ref-type="fig" rid="fig5">Figure 5</xref>. Given the source term<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x118.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x119.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x120.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x121.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x122.png" xlink:type="simple"/></inline-formula>, with k being an arbitrary constant we obtain</p><fig-group id="fig4"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Impact on the population frequency over time and displacement given solution (37). Here,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x124.png" xlink:type="simple"/></inline-formula></title></caption><fig id ="fig4_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-8302663x123.png"/></fig></fig-group><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> Impact on the population frequency given solution (37). Here, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x126.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x126.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x127.png" xlink:type="simple"/></inline-formula></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-8302663x125.png"/></fig><disp-formula id="scirp.62402-formula1525"><label>(38)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x128.png"  xlink:type="simple"/></disp-formula><p>The transformation, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x129.png" xlink:type="simple"/></inline-formula>can be made to Equation (38) to give</p><disp-formula id="scirp.62402-formula1526"><label>(39)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x130.png"  xlink:type="simple"/></disp-formula><p>In terms of the original variables the exact (group-invariant) solution for Equation (38) is given by</p><disp-formula id="scirp.62402-formula1527"><label>(40)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x131.png"  xlink:type="simple"/></disp-formula></sec><sec id="s5_1_2"><title>5.1.2. Reduction by X<sub>1</sub></title><p>The time translation symmetry leads to the steady state problems with the model given by the modified Emden- Fowler equation of the form</p><disp-formula id="scirp.62402-formula1528"><label>(41)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x132.png"  xlink:type="simple"/></disp-formula><p>The transformation <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x133.png" xlink:type="simple"/></inline-formula> reduces the ODE (41) into the Emden-Fowler equation</p><disp-formula id="scirp.62402-formula1529"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x134.png"  xlink:type="simple"/></disp-formula><p>which is hard to solve exactly. Note that ODE (41) admits the scaling symmetry which may be used to reduce the order this equation by one.</p></sec><sec id="s5_1_3"><title>5.1.3. Reduction by the Combination <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x135.png" xlink:type="simple"/></inline-formula></title><p>To construct the exact (group-invariant) solution we consider the linear combination of symmetries <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x136.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x136.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x137.png" xlink:type="simple"/></inline-formula> The characteristic equation corresponding to this combination is given by</p><disp-formula id="scirp.62402-formula1530"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x138.png"  xlink:type="simple"/></disp-formula><p>The basis of invariants is given by</p><disp-formula id="scirp.62402-formula1531"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x139.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.62402-formula1532"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x140.png"  xlink:type="simple"/></disp-formula><p>Let <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x141.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x141.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x142.png" xlink:type="simple"/></inline-formula> Thus the functional form of the group-invariant solution is given by</p><disp-formula id="scirp.62402-formula1533"><label>(42)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x143.png"  xlink:type="simple"/></disp-formula><p>where F satisfies the second order ODE</p><disp-formula id="scirp.62402-formula1534"><label>(43)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x144.png"  xlink:type="simple"/></disp-formula><p>Equation (43) admits the following rotation symmetry,</p><disp-formula id="scirp.62402-formula1535"><label>(44)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x145.png"  xlink:type="simple"/></disp-formula><p>We implement the method of differential invariants to reduce the order of Equation (43) by one. The first prolongation of X is given by</p><disp-formula id="scirp.62402-formula1536"><label>(45)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x146.png"  xlink:type="simple"/></disp-formula><p>The characteristic equations are given by,</p><disp-formula id="scirp.62402-formula1537"><label>(46)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x147.png"  xlink:type="simple"/></disp-formula><p>The invariants are therefore, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x148.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x148.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x149.png" xlink:type="simple"/></inline-formula>. Writing <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x148.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x149.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x150.png" xlink:type="simple"/></inline-formula> <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x148.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x149.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x150.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x151.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x148.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x149.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x150.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x151.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x152.png" xlink:type="simple"/></inline-formula> we obtain the reduced equation</p><disp-formula id="scirp.62402-formula1538"><label>(47)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x153.png"  xlink:type="simple"/></disp-formula><p>A further simplification can be made to Equation (47), whereby<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x154.png" xlink:type="simple"/></inline-formula>. Therefore Equation (47) can be written as,</p><disp-formula id="scirp.62402-formula1539"><label>(48)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x155.png"  xlink:type="simple"/></disp-formula><p>Suppose<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x156.png" xlink:type="simple"/></inline-formula>, then Equation (48) becomes variable separable and the solution for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x156.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x157.png" xlink:type="simple"/></inline-formula> can be found. Substituting back for G gives,</p><disp-formula id="scirp.62402-formula1540"><label>(49)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x158.png"  xlink:type="simple"/></disp-formula><p>wherein an integration constant vanished for simplicity.</p><p>In terms of the original variables we obtain a group-invariant (particular) solution given by</p><disp-formula id="scirp.62402-formula1541"><label>(50)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-8302663x159.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x160.png" xlink:type="simple"/></inline-formula> is an arbitrary constant. The ODE (47) is difficult to solve exactly when<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x160.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x161.png" xlink:type="simple"/></inline-formula>. Solution (50) is depicted in <xref ref-type="fig" rid="fig6">Figure 6</xref>.</p></sec></sec><sec id="s5_2"><title>5.2. Classical Lie Point Symmetry Reduction Given n &#185; 1</title><p>In this case, Equation (25) admits a two dimensional Lie symmetry algebra spanned by the base vectors</p><fig id="fig6"  position="float"><label><xref ref-type="fig" rid="fig6">Figure 6</xref></label><caption><title> Impact on the population frequency given solution (50). Here,<img data-original="http://html.scirp.org/file/4-8302663x163.png" /></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-8302663x162.png"/></fig><disp-formula id="scirp.62402-formula1542"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x164.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.62402-formula1543"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x165.png"  xlink:type="simple"/></disp-formula><sec id="s5_2_1"><title>5.2.1. Reduction by X<sub>1</sub></title><p>The time translation led to the steady state problem given by the Emden-Fowler type ODE</p><disp-formula id="scirp.62402-formula1544"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x166.png"  xlink:type="simple"/></disp-formula><p>Which is harder to solve exactly.</p></sec><sec id="s5_2_2"><title>5.2.2. Reduction by X<sub>2</sub></title><p>Reduction by this symmetry generator led to a functional form of the group-invariant solution given by</p><disp-formula id="scirp.62402-formula1545"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x167.png"  xlink:type="simple"/></disp-formula><p>which is in fact separation of variables. Here F satisfies the first order ODE</p><disp-formula id="scirp.62402-formula1546"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x168.png"  xlink:type="simple"/></disp-formula><p>which has a solution</p><disp-formula id="scirp.62402-formula1547"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x169.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x170.png" xlink:type="simple"/></inline-formula> is an integration constant. Thus we obtain</p><disp-formula id="scirp.62402-formula1548"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x171.png"  xlink:type="simple"/></disp-formula></sec></sec></sec><sec id="s6"><title>6. A Note on Conservation Laws of Equation (25)</title><p>It is worth noting that Equation (25) has the conservation laws given by the conserved vectors</p><disp-formula id="scirp.62402-formula1549"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x172.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.62402-formula1550"><graphic  xlink:href="http://html.scirp.org/file/4-8302663x173.png"  xlink:type="simple"/></disp-formula><p>provided <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-8302663x174.png" xlink:type="simple"/></inline-formula> which implies a linear heat equation with spatial dependent diffusion term. These combination of conserved vectors is obtained by both direct and multiplier methods.</p></sec><sec id="s7"><title>7. Some Discussions and Concluding Remarks</title><p>In this paper, we have used both classical and nonclassical symmetry methods to construct the exact solutions. Some new group-invariant (exact) solutions for reaction diffusion equation with spatially dependent diffusivity and the coefficient of the source term have been constructed using both classical and nonclassical symmetry techniques. Figures 1-6 depict the change in mutant population with respect to either time or space or both. The effects of the parameters appearing in the plotted exact solutions on the population are displayed. We have introduced the modified Hopf-Cole transformation to transform a nonlinear second order ODE to a simpler to solve linear third order ODE. To the best of our knowledge, this transformation has never been used in the recorded literature.</p></sec><sec id="s8"><title>Cite this paper</title><p>KirstenLouw,Raseelo J.Moitsheki, (2015) Group-Invariant Solutions for the Generalised Fisher Type Equation. 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