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The limitation of HSM exists in the inability to define the specific motivations of persuasion, which is why Chaiken expanded HSM to illustrate that heuristic and systematic processing can "serve defense-motivation, the desire to form or defend particular attitudinal positions, and impression- motivation, the desire to form or hold socially ...
Karl Schwarzschild (German: [kaʁl ˈʃvaʁtsʃɪlt] ⓘ; 9 October 1873 – 11 May 1916) was a German physicist and astronomer.. Schwarzschild provided the first exact solution to the Einstein field equations of general relativity, for the limited case of a single spherical non-rotating mass, which he accomplished in 1915, the same year that Einstein first introduced general relativity.
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Download as PDF; Printable version; ... Temporal motivation theory; ... Yale attitude change approach This page was last ...
In deriving the Schwarzschild metric, it was assumed that the metric was vacuum, spherically symmetric and static. The static assumption is unneeded, as Birkhoff's theorem states that any spherically symmetric vacuum solution of Einstein's field equations is stationary; the Schwarzschild solution thus follows
According to this theory, when somebody makes a judgment (of a target attribute) which is computationally complex, a rather more easily calculated heuristic attribute is substituted. [100] In effect, a difficult problem is dealt with by answering a rather simpler problem, without the person being aware this is happening. [ 97 ]
Under this theory, cooperating in everyday social situations tends to be successful, and as a result, cooperation is an internalized heuristic that is applied in unfamiliar social contexts, even those in which such behavior may not lead to the most personally advantageous result for the actor (such as a lab experiment).
The paler hyperbolas represent contours of the Schwarzschild r coordinate, and the straight lines through the origin represent contours of the Schwarzschild t coordinate. In general relativity , Kruskal–Szekeres coordinates , named after Martin Kruskal and George Szekeres , are a coordinate system for the Schwarzschild geometry for a black hole .