Fast radio bursts from space have baffled scientists for years
nbcnews.com
nbcnews.com
I read this sort of thing now and then over the years, and I'm not sure I understand it, or if it is misleading.
What is an "object"? Could an "object" be part of a stellar object, or is it necessarily the whole thing? It seems like surely some event can happen on the Sun in less time than it takes for light to pass across it, just like radio waves on earth can be modulated in less time than it takes for them to pass across the planet.
Maybe it's obvious what an "object" is, but I feel like the statement that it has to be under 200 miles wide is promoting the assumption that it has to be a neutron star, or perhaps a black hole. But does it?
The article only refers to repeating FBR-s but that's a known things for years now.
So for FRBs, we get the received brightness, and if we can measure the distance, we can use the basic inverse square scaling to estimate how much energy it had at the source. (Why inverse square? Because the area of a sphere is 4 pi R^2 - if you go twice as far away, the signal is spread out over 4 times the area, and so on.)
The key problem is a distance estimate for the FRBs - we have a pretty precise measurement for FRB 121102 because we identified its host galaxy and measured the redshift to that galaxy, so we know how far away it is. That's now been done for 2 other sources. For the rest, we can use the pulse dispersion, which measures the integrated column density of electrons along the line of sight, along with models for our galaxy and the intergalactic medium, to get some idea. It's not as good, but better than nothing.
The problem is, while you can reduce the energy requirement by making the beams narrow, that increases the total number of sources by the same factor. When we say that there are between 5000-10,000 FRBs all over the sky every single day, we are referring to FRBs beamed towards us. If you apply a 10% beam, your energy requirement drops by 10x, sure, but the source count goes up by 10x.
Right now, we don't have a large enough plausible progenitor population, even at 1x, for these FRBs. It's a really fun problem.
[1] See, e.g, the Methods section in https://www.nature.com/articles/nature20797 (or https://arxiv.org/abs/1701.01098)
> power the world for three centuries
Our sun for example is emitting enough energy in all directions to power the world for 300 years (over the course of 300 years), and most of it misses us.
Our sun isn't particularly impressive in terms of energy and such compared to other astro-objects, so I feel like these kinda of events releasing so much energy are to be expected.
I think you're saying any amount of energy can be produced by any amount of power, if the amount of time is unspecified. Which is true, but not substantive.
Specifically to radio astronomy: https://en.wikipedia.org/wiki/Luminosity#Radio_luminosity