Difference Between Scalar Field Solutions in Curved Spacetime

In summary: Overall, any valid solutions to the wave equation can represent both particles and fields, but the specific form of the solution may vary depending on the physical situation.
  • #1
Tertius
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TL;DR Summary
A free scalar field solution for the situation of 1) static, and 2) homogeneous and isotropic yield either trigonometric or exponential solutions. The first would seem to be a harmonic oscillator, the second seems to be a simple field being dispersed across space. How can these be interpreted?
A general free field Lagrangian in curved spacetime (- + + +), is given by:
L = -1/2 ∇cΦ ∇cΦ - V(Φ)
when the derivative index is lowered, we obtain:
L = -1/2 gdcdΦ ∇cΦ - V(Φ)
then we can choose to replace V(Φ) with something like 1/2 b2 Φ2 so:
L = -1/2 gdcdΦ ∇cΦ - 1/2 b2 Φ2

** I will only give the fields and solutions in terms of t and x for simplicity (ignoring y and z). And because we are acting on a scalar the covariant derivatives can be replaced with partial derivatives.
Case 1: let's assume the field only changes with time (i.e. is homogeneous and isotropic), Φ(t,x) -> Φ(t), which then yields the Lagrangian (a Lagrangian that contains only non-derivative terms should have the field forced to equal 0):
L = -1/2 * -1 * ∂tΦ ∂tΦ - 1/2 b2 Φ2
which gives the equations of motion:
Φ''(t) = -1/2 b2Φ(t)
which can be easily solved for a general solution:
Φ(t) = c1cos(b t) + c2 sin(b t)

Case 2: let's assume the field only changes with space (i.e. is static), Φ(t,x) -> Φ(x), which then yields the Lagrangian:
L = -1/2 * 1 * ∂xΦ ∂xΦ - 1/2 b2 Φ2
which gives the equations of motion:
Φ''(x) = 1/2 b2Φ(x)
which can be easily solved for a general solution:
Φ(t) = c1ebx + c2e-bxIf the math I showed above doesn't have any glaring errors, this leads me to a few questions:
1) why would this field yield a trigonometric solution that clearly oscillates over time when the field is homogeneous and isotropic?
2) and why would it only yield an exponential decay/growth in the spatial direction?
3) I realize plane wave solutions derived using Fourier transform are often used as solutions, are they any more correct than these solutions? It seems like the plane wave solutions result in a vectorized wave that typically corresponds to particle behavior. are the solutions I gave valid for particles as well as fields? any insight here is appreciated.

 
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  • #2


1) The trigonometric solution arises because the field is homogeneous and isotropic, meaning it does not vary with position. This leads to a time-dependent solution, as the field can only vary with time. The oscillatory behavior is a result of the sine and cosine functions being periodic in nature.

2) The exponential solution arises because the field is static, meaning it does not vary with time. This leads to a spatially-dependent solution, as the field can only vary with position. The exponential behavior is a result of the exponential function being a solution to the differential equation.

3) The plane wave solutions derived using Fourier transform are often used because they are a convenient way to represent the solutions of the wave equation. They are also valid solutions, but they may not always be the most physically meaningful. The solutions you gave are valid for both particles and fields, but they may not always correspond to observable behavior. It is important to consider the physical interpretation of the solutions in addition to their mathematical validity.
 

FAQ: Difference Between Scalar Field Solutions in Curved Spacetime

What is a scalar field?

A scalar field is a mathematical concept used in physics to describe a quantity that has a single value at every point in space and time. Examples of scalar fields include temperature, pressure, and energy density.

How does a scalar field behave in curved spacetime?

In curved spacetime, a scalar field can vary in value depending on the curvature of space at a particular point. This means that the value of the scalar field can change as an object moves through space, unlike in flat spacetime where it remains constant.

What are the solutions to a scalar field in curved spacetime?

The solutions to a scalar field in curved spacetime depend on the specific equations used to describe the curvature of space. Some common solutions include the Schwarzschild solution, which describes the gravitational field around a spherically symmetric object, and the Kerr solution, which describes the spacetime around a rotating object.

How do scalar field solutions in curved spacetime differ from those in flat spacetime?

In flat spacetime, the scalar field is constant and does not vary with position. In curved spacetime, the scalar field can vary in value and behavior depending on the curvature of space. Additionally, the equations used to describe scalar field solutions in curved spacetime are more complex and involve the concept of curvature.

What are the practical applications of understanding the difference between scalar field solutions in curved and flat spacetime?

Understanding the behavior of scalar fields in curved spacetime is crucial in many areas of physics, including general relativity and cosmology. It allows us to make accurate predictions about the behavior of matter and energy in the presence of strong gravitational fields, such as those near black holes. Additionally, understanding these differences can help us better understand the fundamental nature of space and time.

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