9
$\begingroup$

I was watching the press release about measuring neutrinos and gamma rays from a distant blazar. One of the presenters mentioned that the neutrinos are associated with very high energy protons caught up in the jet produced by the galactic nucleus. What I don't understand is what interation(s) is producing the neutrinos in this scenario. What sort of particles must the protons be interacting with to produce these neutrinos?

$\endgroup$
10
$\begingroup$

Neutrinos are typically produced in AGN jets through what we refer to as hadronic processes. Protons are accelerated to relativistic speeds and interact with nearby photons. Depending on the particular type of AGN, there are a number of possible sources of these photons:

  • Ambient light within the jet
  • Emission from the accretion disk
  • Photons from the broad line region surrounding the AGN
  • Emission from the nearby dust torus

As I understand it, contributions from the latter two sources are less prominent in blazars, although they may play an important role in the radio-loud flat spectrum radio quasars (FSRQs). Murase et al. 2014 have an excellent diagram showing the possible sources of this radiation:

Diagram of radiation sources around an active galactic nucleus

The photons interact with the protons in the jet and produce other hadrons, typically pions. Neutral pions decay to a pair of photons, one key mechanism of gamma ray production in AGN jets:1 $$\pi^0\to\gamma+\gamma$$ However, it is quite possible for the proton-photon interactions to produce charged pions ($\pi^{\pm}$), which then decay to muons and muon neutrinos (Atoyan & Dermer 2002). The muons decay to electrons, while the muon neutrinos may be observed here on Earth. This appears to have been the source of the neutrino detected by IceCube in 2018, originating from the blazar TXS 0506+056.


1 The other main set of gamma ray production pathways in the jets are the leptonic processes, where electrons and positrons transfer energy to ambient photons via the inverse Compton effect; see Degrange & Fontaine 2016, which I found quite helpful when learning about those mechanisms.

| improve this answer | |
$\endgroup$
  • 1
    $\begingroup$ this is excellent. Thanks so much. Will read the articles you linked to though I suspect much of the content is well above my pay grade at this point. $\endgroup$ – PSR-1937-21 Dec 24 '19 at 18:45

Your Answer

By clicking “Post Your Answer”, you agree to our terms of service, privacy policy and cookie policy

Not the answer you're looking for? Browse other questions tagged or ask your own question.