- A black hole is a region of spacetime where gravity is so strong that nothing, including light or other electromagnetic waves, has enough energy to escape it. The theory of general relativity predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of no escape is called the event horizon. Although it has a great effect on the fate and circumstances of an object crossing it, it has no locally detectable features according to general relativity. In many ways, a black hole acts like an ideal black body, as it reflects no light. Moreover, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a black body of a temperature inversely proportional to its mass. This temperature is of the order of billionths of a kelvin for stellar black holes, making it essentially impossible to observe directly.
- How to reverse engineer an analog chip: the TDA7000 FM radio receiver (righto.com)
Have you ever wanted to reverse engineer an analog chip from a die photo? Wanted to understand what’s inside the “black box” of an integrated circuit? In this article, I explain my reverse engineering process, using the Philips TDA7000 FM radio receiver chip as an example. This chip was the first FM radio receiver on a chip.1 It was designed in 1977—an era of large transistors and a single layer of metal—so it is much easier to examine than modern chips. Nonetheless, the TDA7000 is a non-trivial chip with over 100 transistors. It includes common analog circuits such as differential amplifiers and current mirrors, along with more obscure circuits such as Gilbert cell mixers.