Karl Schwarzschild
Karl Schwarzschild | |
|---|---|
 Karl Schwarzschild (1873–1916) | |
| Born | 9 October 1873 |
| Died | 11 May 1916 (aged 42)[1]: Script error: The function "hyphen2dash" does not exist.  Potsdam, German Empire |
| Nationality | German |
| Alma mater | Ludwig-Maximilians-Universität München |
| Scientific career | |
| Fields | Physics Astronomy |
| Influenced | Martin Schwarzschild |
| Signature | |
 | |
Karl Schwarzschild (9 October 1873 – 11 May 1916) was a German physicist and astronomer.
Best known for his solution to Einstein's equations of general relativity, which describes the gravitational field outside a non-rotating black hole with no magnetic field.
The equation describes how a particle moves space near this black hole (using spherical coordinates).
[math]\displaystyle{ (ds)^2=-c^2(1-\frac{r_s}{r})(dt)^2+\frac{1}{(1-\frac{r_s}{r})}(dr)^2+r^2(d\theta)^2+r^2\sin^2(\theta)(d\phi)^2 }[/math]
ds is the path it follows
dt is the change in time
dr is the change in radius
d[math]\displaystyle{ \theta }[/math] and d[math]\displaystyle{ \phi }[/math] are the change in angle
[math]\displaystyle{ \theta }[/math] is also the angle
[math]\displaystyle{ r_s }[/math] is the set radius limit of the heavy object
r is how close the travelling object is to the heavy object
c is the speed of light
This equation is also known as the Schwarzschild metric or Schwarzschild solution.[2]
Karl Schwarzschild Media
Schwarzschild at the Fourth Conference International Union for Cooperation in Solar Research at Mount Wilson Observatory, 1910
Karl Schwarzschild's grave at Stadtfriedhof (Göttingen)
The Kepler problem in general relativity, using the Schwarzschild metric
Boundary region of Schwarzschild interior and exterior solution
References
- ↑ Biography of Karl Schwarzschild by Indranu Suhendro, The Abraham Zelmanov Journal, 2008, Volume 1.
- ↑ Czerniawski, Jan. [1], The possibility of a simple derivation of the Schwarzschild metric. Retrieved on 10 May, 2020.