A Study of Non-Canonical Lagrangian ()

Bhupendra Singh^{1}, Ranjit Kumar^{2}, Loukrakpam Kennedy Meitei^{2}

^{1}Department of Physics, Atmaram Sanatan Dharma College, University of Delhi, Delhi, India.

^{2}Department of Physics, Dyal Singh College, University of Delhi, Delhi, India.

**DOI: **10.4236/ns.2016.85024
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Non-canonical Lagrangian (Lagrangian with non-quadratic kinetic term) has been studied in the context of cosmology. In this work, the non-canonical Lagrangian with potential energy term has been discussed. We have obtained the periodic and solitary wave solutions for certain types of potential. The solutions obtained here may provide some new direction in the theory of phase transition, quantum field theory and related phenomena.

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Singh, B. , Kumar, R. and Kennedy Meitei, L. (2016) A Study of Non-Canonical Lagrangian. *Natural Science*, **8**, 211-215. doi: 10.4236/ns.2016.85024.

Received 7 January 2016; accepted 3 May 2016; published 6 May 2016

1. Introduction

Canonical Lagrangian has been studied in the context of classical mechanics, quantum field theory and other branches of physics. The standard form of canonical Lagrangian density is given by

(1)

Here and also action S is dimensionless then, Lagrangian density has dimension of and hence dimension of is M (here M stands for mass). Also we are considering the case of one time and one space dimension. Thus, where corresponds to time coordinate t, and corresponds to space coordinate x. Here the metric tensor is diagonal, and is given by

(2)

In this framework, Lagrangian density (1) can be written as

(3)

Here kinetic energy term is quadratic. Lagrangian density (1) has been extensively studied in the context of quantum field theory, theory of phase transition and other branches of physics [1] - [5] . In recent years, non canonical Lagrangian density has been used in the inflationary cosmological models [6] - [8] (see ref. [9] for further details). In the context of cosmological model, even in absence of any potential energy term, a general class of non-standard (i.e., non-quadratic) kinetic energy terms, for a scalar field, can drive an inflationary evolution of the same type as the usually considered potential driven inflation. The mathematical form of non canonical Lagrangian density is given by the following equation:

(4)

where is the potential and n is an integer. For, we get the usual Lagrangian of the scalar field theory. Also, note that the Equation (4) is Lorentz invariant for any value of n. The purpose of this work is to obtain the exact solution of Equation (4) in (1 + 1)-dimension for, and for the different potentials. For, Equation (4) takes the form

(5)

Also, we are using natural units in which and action is dimensionless. In this unit is dimensionless. The corresponding equation of motion is given by

(6)

Thus the Lagrangian density is given by

(7)

From here one can see that the kinetic energy is non-quadratic and that’s why the Lagrangian is known as non-canonical Lagrangian. The corresponding equation of motion is given by

(8)

Here represents the time derivative of field and represents the spatial derivative. Note that the equation of motion remain second order. Also, for a Lorentz invariant system once a static solution is known, moving solutions are obtained by transforming to a moving coordinate system [1] (we are interested in solitary and periodic wave solutions). Now for static case, the equation of motion becomes

(9)

Multiplying both sides by and integrating with respect to x, we obtain

(10)

where C is constant of integration. Let and vanishes at and hence. Thus finally we obtain

(11)

For in Equation (4), the corresponding equation of motion is given by

(12)

In the next section we will solve Equation (11) for some specific potentials. Also, Equation (11) cannot be solved for every potential. We will consider only those potentials for which Equation (11) can be integrated.

2. Solutions

In this section we are going to solve Equation (11) for the following potentials.

Case I: Let us first consider the potential

(13)

where is real constant and its dimension is. This potential is used in the theory of phase transition and is taken from reference [1] . For this potential, Equation (11) takes the form

(14)

After integrating this equation, we obtain

(15)

where is constant of integration. To solve the left hand integral, we substitute and after solving this integral, we obtain

(16)

For time dependent case, the corresponding solution can be obtained by Lorentz transformation

(17)

and hence

(18)

From this solution one can see that, for we obtain periodic solution and for, we obtain hyperbolic solution. The hyperbolic solution diverges for large x and t. Now the energy of the field is given by

(19)

where is energy density and is given by

(20)

where is momentum density and is time derivative of the field. Here

(21)

where is spatial derivative of the field. Using Equations ((20) and (21)), we obtain

(22)

(23)

For static case, we obtain

(24)

Using Equation (11), we get

(25)

Now

(26)

and hence

(27)

Note that, otherwise energy density becomes imaginary. The total energy is given by

(28)

For time dependent case, energy density is given by

(29)

For, and for the given potential Equation (16), we obtain from Equation (12) the following solution

(30)

which is a kink solitary wave solution [1] for. Thus in this case solution exist for. Energy density in this case is given by

(31)

The energy density is localised near. According to the definition of [1] , localised solutions are those solutions to the field equation whose energy density at any finite time t is localised in space and falls to zero at spatial infinity.

Case II: Here we will consider the potential of the form

(32)

In this case, the solution of time independent field equation is given by

(33)

Note that this solution is a solitary wave solution for. Similarly, the corresponding solution of time dependent case is given by

(34)

The energy density of time independent case is given by

(35)

and the energy density of time dependent case is given by

(36)

Thus the energy density is localised.

3. Concluding Remarks

In this work we have discussed the non-canonical lagrangian for different kinds of potential. We have obtained the periodic and solitary wave solutions. A comparison is also made between the solutions of canonical and non-canonical lagrangian. As one can see that for Equation (16), the solution exists only when whereas, for the same potential and for canonical Lagrangian, the solution exists for. Also the solution of non- canonical lagrangian is periodic and canonical lagrangian admits the solitary wave solution. Similarly for the potential (32), the non-canonical lagrangian admits the solitary wave solution for. Although non-canonical Lagrangian has been used in the inflationary model, the result obtained in this work may be used to explain the phenomena of phase transition and other quantum field theoretic model.

Acknowledgements

We would like to thank Sanil Unnikrishnan for helpful discussions.

NOTES

^{*}Corresponding author.

Conflicts of Interest

The authors declare no conflicts of interest.

[1] | Rajaraman, R. (1987) Solitons and Instanton: An Introduction to Solitons and Instantons in Quantum Field Theory. North-Holland. |

[2] | Dauxois and Peyrard (2006) Physics of Solitons. Cambridge University Press, Cambridge. |

[3] | Khare, A. and Saxena, A. (2006) Domain Wall and Periodic Solutions of Coupled 4 Models in an External Field. Journal of Mathematical Physics, 47, Article ID: 092902. http://dx.doi.org/10.1063/1.2345110 |

[4] | Khare, A. and Saxena, A. (2008) Domain Wall and Periodic Solutions of a Coupled 6 Model. Journal of Mathematical Physics, 49, Article ID: 063301. http://dx.doi.org/10.1063/1.2938691 |

[5] | Sanati, M. and Saxena, A. (1999) Half-Kink Lattice Solution of the 6 Model. Journal of Physics A: Mathematical and General, 32, 4311. http://dx.doi.org/10.1088/0305-4470/32/23/309 |

[6] | Armendáriz-Picón, C., Damour, T. and Mukhanov, V. (1999) k-Inflation. Physics Letters B, 458, 209-218. http://dx.doi.org/10.1016/S0370-2693(99)00603-6 |

[7] | Garriga, J. and Mukhanov, V.F. (1999) Perturbations in k-Inflation. Physics Letters B, 458, 219-225. http://dx.doi.org/10.1016/S0370-2693(99)00602-4 |

[8] | Unnikrishnan, S., Sahni, V. and Toporensky, A. (2012) Refining Inflation Using Non-Canonical Scalars. Journal of Cosmology and Astroparticle Physics, 2012, 018. http://dx.doi.org/10.1088/1475-7516/2012/08/018 |

[9] | Das, S. and Al Mamon, A. (2015) Cosmic Acceleration in Non-Canonical Scalar Field Model: An Interacting Scenario. Astrophysics and Space Science, 355, 371. (arXiv: 1407.1666v3 [gr-qc]) |

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