SUMMARY
This discussion centers on the transformation of an acceleration vector under a basis change in the context of Schwarzschild spacetime. The original co-basis is defined as s_0= \sqrt{\frac{r-2m}{r}}dt, s_1=\sqrt{\frac{r}{r-2m}}\ dr, s_2=r\ d\theta, and s_3=r\sin(\theta)\ d\phi, with the 4-velocity of a stationary observer given by u^\mu=\partial_t. A boost in the r-direction leads to a new basis where the acceleration a_\mu is calculated to be zero, raising skepticism among participants regarding the validity of this result. The transformation is identified as equivalent to a shift from Schwarzschild to Painleve coordinates, which does not leave the metric unchanged.
PREREQUISITES
- Understanding of Schwarzschild spacetime and its metrics
- Familiarity with 4-velocity and 4-acceleration concepts in General Relativity
- Knowledge of covariant and contravariant tensors
- Experience with basis transformations in differential geometry
NEXT STEPS
- Study the implications of the Painleve coordinates on observer transformations in General Relativity
- Learn about the covariant derivative and its role in calculating 4-acceleration
- Explore the differences between covectors and vectors in the context of tensor calculus
- Investigate the invariance properties of metrics under various transformations in curved spacetime
USEFUL FOR
This discussion is beneficial for physicists, mathematicians, and students specializing in General Relativity, particularly those interested in the mathematical foundations of spacetime transformations and observer effects.