<p>Neutrinos are typically produced in AGN jets through what we refer to as <em>hadronic processes</em>. 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:</p>

<ul>
<li>Ambient light within the jet</li>
<li>Emission from the accretion disk</li>
<li>Photons from the broad line region surrounding the AGN</li>
<li>Emission from the nearby dust torus</li>
</ul>

<p>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). <a href="https://ui.adsabs.harvard.edu/abs/2014PhRvD..90b3007M/abstract" rel="noreferrer">Murase et al. 2014</a> have an excellent diagram showing the possible sources of this radiation:</p>

<p><a href="https://i.sstatic.net/c7pLZ.png" rel="noreferrer"><img src="https://i.sstatic.net/c7pLZ.png" alt="Diagram of radiation sources around an active galactic nucleus"></a></p>

<p>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:<sup>1</sup>
<span class="math-container">$$\pi^0\to\gamma+\gamma$$</span>
However, it is quite possible for the proton-photon interactions to produce <em>charged</em> pions (<span class="math-container">$\pi^{\pm}$</span>), which then decay to muons and muon neutrinos (<a href="https://iopscience.iop.org/article/10.1086/346261/fulltext/56565.text.html" rel="noreferrer">Atoyan &amp; Dermer 2002</a>). 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.</p>

<hr>

<p><sup>1</sup> The other main set of gamma ray production pathways in the jets are the <em>leptonic processes</em>, where electrons and positrons transfer energy to ambient photons via the inverse Compton effect; see <a href="https://arxiv.org/abs/1604.05488" rel="noreferrer">Degrange &amp; Fontaine 2016</a>, which I found quite helpful when learning about those mechanisms.</p>

CC BY-SA 4.0
2019-12-24T18:45:07.463Z
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.
PSR-1937-21
CC BY-SA 4.0
2019-12-24T18:40:10.470Z
2019-12-24T18:40:10.470Z
HDE 226868
<p>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?</p>

<quasars><neutrinos><active-galaxy><particles><blazars>
How are neutrinos produced in blazar jets?
PSR-1937-21
# How are neutrinos produced in blazar jets?

(Asked by: username_0 on 2019-12-24)

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?

**Tags:** quasars, neutrinos, active-galaxy, particles, blazars


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## 1 answers

### Answer by username_1 on 2019-12-24. Score: 10

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](https://ui.adsabs.harvard.edu/abs/2014PhRvD..90b3007M/abstract) have an excellent diagram showing the possible sources of this radiation:

[![Diagram of radiation sources around an active galactic nucleus](https://i.sstatic.net/c7pLZ.png)](https://i.sstatic.net/c7pLZ.png)

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](https://iopscience.iop.org/article/10.1086/346261/fulltext/56565.text.html)). 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](https://arxiv.org/abs/1604.05488), which I found quite helpful when learning about those mechanisms.

> **Comments:**
> **username_0**: 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.  

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