Geodesic Expansion: Finding the $\theta_{\pm}$ Factor

In summary, the conversation discusses the equations related to the definition of the vectors ##U_{\pm}## and the tensor ##P^a_b## in the context of black holes. It also looks at the expression for ##\theta_{\pm}## and the presence of the factor of ##\dfrac{1}{\sqrt{2}}## in the equations. The question asks about the origin of this factor and how to rewrite the second term in the equation for ##\theta_{\pm}##. The conversation is related to lectures and examples on black holes.
  • #1
ergospherical
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\begin{align*}
\mathrm{\mathbf{(a)}} \quad U_{\pm} \cdot U_{\pm} &= \dfrac{1}{2} (n_a n^a \pm 2 n_a m^a + m_a m^a) = \pm n_a m^a = 0 \\
U_+ \cdot U_- &= \dfrac{1}{2} (n_a n^a - m_a m^a) = \dfrac{1}{2} (-1-1) = -1 \\ \\

\mathrm{\mathbf{(b)}} \quad P^a_b &= \delta^a_b + U_{\mp}^a (U_{\pm})_b + U_{\pm}^a (U_{\mp})_b \\

&= \delta^a_b + \dfrac{1}{2} (n^a \mp m^a)(n_b \pm m_b) + \dfrac{1}{2} (n^a \pm m^a)(n_b \mp m_b) \\

&= \delta^a_b + n^a n_b - m^a m_b \\

&= h^a_b - m^a m_b \\ \\

\mathrm{\mathbf{(c)}} \quad \theta_{\pm} &= P^{ab} \nabla_a (U_{\pm})_b \\

&= \dfrac{1}{\sqrt{2}} (h^{ab} - m^a m^b) \nabla_a (n_b \pm m_b) \\

&= \dfrac{1}{\sqrt{2}} (h^{ab} - m^a m^b) (K_{ab} - n_a n^c \nabla_c n _b) \pm \dfrac{1}{\sqrt{2}} (h^{ab} - m^a m^b) (k_{ab} - m_a m^c \nabla_c m _b) \\

&= \dfrac{1}{\sqrt{2}} (h^{ab} - m^a m^b) K_{ab} - \dfrac{1}{\sqrt{2}} \underbrace{h^{ab} n_a}_{= \, 0} n^c \nabla_c n_b + \dfrac{1}{\sqrt{2}} m^b \underbrace{m^a n_a}_{= \, 0} n^c \nabla_c n_b \\

&\hspace{45pt} \pm \dfrac{1}{\sqrt{2}} (h^{ab} - m^a m^b) (k_{ab} - m_a m^c \nabla_c m _b) \\ \\

&= \dfrac{1}{\sqrt{2}} (h^{ab} - m^a m^b) K_{ab} \pm \dfrac{1}{\sqrt{2}} (h^{ab} - m^a m^b) (k_{ab} - m_a m^c \nabla_c m _b)
\end{align*}Why is there a factor of ##\dfrac{1}{\sqrt{2}}##, and how do you re-write the second term?
 
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  • #3
robphy said:
Is the [itex]\frac{1}{\sqrt{2}} [/itex] from the definition of [itex]U^a_{\pm}[/itex]?
Yeah, one thing I don't understand is why the ##\dfrac{1}{\sqrt{2}}## doesn't appear in the equation ##\theta_{\pm} = (h^{ab} - m^a m^b)K_{ab} \pm k## in the question.
 

FAQ: Geodesic Expansion: Finding the $\theta_{\pm}$ Factor

What is geodesic expansion?

Geodesic expansion is a mathematical method used in general relativity to calculate the distance between two points on a curved spacetime. It involves finding the shortest path between the two points, which is known as a geodesic, and then expanding the geodesic into a series of terms to calculate its length.

What is the $\theta_{\pm}$ factor in geodesic expansion?

The $\theta_{\pm}$ factor is a term that is used in the geodesic expansion formula to account for the curvature of spacetime. It is a function of the curvature and the distance between the two points being measured, and it helps to correct for any errors in the calculation caused by the curvature of spacetime.

Why is geodesic expansion important in general relativity?

Geodesic expansion is important in general relativity because it allows us to accurately calculate distances and make predictions about the behavior of objects in a curved spacetime. It is a fundamental tool in understanding the effects of gravity and the structure of the universe.

What are some applications of geodesic expansion?

Geodesic expansion has many applications in physics and astronomy. It is used to calculate the trajectories of objects in space, to study the curvature of spacetime in different regions of the universe, and to make predictions about the behavior of black holes and other massive objects.

Are there any limitations to geodesic expansion?

Geodesic expansion is a powerful tool, but it does have some limitations. It is most accurate in regions of spacetime with low curvature, and it becomes less accurate as the curvature increases. It also does not take into account quantum effects, so it cannot be used to accurately describe the behavior of very small particles.

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