Chemical composition of relativistic neutron star jets?

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Discussion Overview

The discussion centers on the chemical composition of relativistic jets emitted from neutron stars, exploring how this composition may differ from the accretion material and what implications this has for understanding jet formation processes. The scope includes theoretical considerations, potential observational methods, and the implications of particle composition in high-velocity jets.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants inquire about the chemical composition of neutron star jets and suggest that differences from accretion material could provide insights into jet formation.
  • One participant references spectral analysis as a method to determine the chemical composition of jets and accretion, questioning where changes in composition might occur.
  • Another participant proposes that if jets are composed mainly of electrons and positrons, this could relate to neutron disintegration, but raises concerns about baryon number conservation.
  • Some argue that jets with velocities greater than 0.9c should primarily consist of small particles like electrons, positrons, and neutrinos, with larger atoms being present in minimal quantities.
  • There is a discussion about whether jets at such high velocities can contain a significant number of protons or other nuclei, with some expressing skepticism about the mass composition of these jets.
  • Participants mention cosmic rays and their composition, noting the presence of protons and nuclei at extreme energies, and question how this relates to the composition of neutron star jets.
  • One participant expresses uncertainty about the clarity of existing literature regarding the composition of jets, particularly concerning the presence of nuclei versus leptons.
  • There are mentions of the effects of magnetic fields on particle acceleration and charge within the jets, suggesting that the dynamics of the accretion disc may influence the jets' properties.

Areas of Agreement / Disagreement

Participants express a range of views regarding the composition of neutron star jets, with no consensus reached on the specifics of particle types or their implications. The discussion remains unresolved with multiple competing hypotheses presented.

Contextual Notes

Limitations include the dependence on observational data that may not yet be available, and the complexity of particle interactions at relativistic speeds, which may not be fully understood. The discussion also reflects uncertainty regarding the implications of baryon number conservation in the context of jet composition.

Bernie G
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Is there any good information about the chemical composition of relativistic jets from neutron stars? If the chemical composition of the jets was different from the accretion material it could shed light on the process that forms the jets.
 
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davenn said:
whilst not exactly what you are after, it may give you some enlightenment on the subject
http://arxiv.org/pdf/astro-ph/0305435v1.pdf Dave

Interesting link which illustrates the reason for my post. A neutron star or stellar black hole is only the size of an asteroid and hence can’t be resolved at hundreds of light years. The only features that can be seen/resolved are the jets and accretion, and glows from the surface. Analysis of the glows is very difficult. The mystery of neutron star relativistic jets is probably easier to understand than stellar back hole jets so neutron star observations could provide the answers for both.

Spectral analysis should reveal the chemical composition of the jets and the accretion. If they are different where does the change occur? Also the synchronization of the jets and accretion is easily observed, and if they are not synchronized it means a lot. The type of info I seek is like that in the following 2 links ….. where could the iron come from? Iron is what could be expected on the surface of a neutron star:

http://www.esa.int/Our_Activities/Space_Science/Black_hole_boasts_heavyweight_jets
http://www.astronomy.com/news/2015/08/neutron-stars-strike-back-at-black-holes-in-jet-contest
 
If the chemical composition of ultra relativistic jets was electrons and positrons, would it be possible for the disintegration of neutrons to produce this directly?
 
This is what I posted on another question, and think its relevant here:
IMHO if a jet has a velocity >0.9c it should be composed mostly of tiny particles like electrons, positrons, neutrinos, quarks, other leptons, etc. If full size atoms are present in a >0.9c jet they are probably small in quantity and just going along for the ride.
 
Bernie G said:
If the chemical composition of ultra relativistic jets was electrons and positrons, would it be possible for the disintegration of neutrons to produce this directly?
This would violate baryon number conservation.
Bernie G said:
IMHO if a jet has a velocity >0.9c it should be composed mostly of tiny particles like electrons, positrons, neutrinos, quarks, other leptons, etc. If full size atoms are present in a >0.9c jet they are probably small in quantity and just going along for the ride.
At the energies needed to accelerate particles to 0.9 c, atoms will rarely keep all their electrons, they are just stripped too easily. You still get protons and other nuclei.
 
mfb said:
At the energies needed to accelerate particles to 0.9 c, atoms will rarely keep all their electrons, they are just stripped too easily. You still get protons and other nuclei.

Yes, but do >0.9c jets have a representative number of protons or other nuclei? If so almost all the mass in the jet would be nuclei. It would be amazing to have a significant number of protons moving at 0.999c although it might not be so amazing to have occasional protons carried along in a 0.999 jet of lepton like particles.
 
Cosmic rays are mainly protons and a few other nuclei - with energies up to 1020 eV, or 0.9999999999999999999999999999999 c (iron at 1020 eV, digits counted). What is 0.999c compared to that?

Here are nuclei in jets
 
Amazing stuff, supernovae explosions squirting lots of nuclei. That link on jet composition isn't clear if there are a trace amounts or a lot of nuclei in that jet or if its mostly leptons. It would be good to know if >0.9c jets from neutron stars are mostly leptons and/or if they have a lot nuclei. That might shed some light on how can a neutron star produce >0.9c jets and where do the leptons come from?
 
  • #10
Well, my link goes to the description for the public, the actual publication will have more details (and also references to previous work done).
 
  • #11
I'm not knocking it, its a good link, thanks. Note the jet speed in that link is 0.66c. It would be amazing if most of the mass in a >0.9c jet were nuclei.
 
  • #12
mfb said:
This would violate baryon number conservation.
At the energies needed to accelerate particles to 0.9 c, atoms will rarely keep all their electrons, they are just stripped too easily. You still get protons and other nuclei.
If the jets near the accretion disc maintain a positive charge, eventually free electrons are going to be accelerated from the galaxy toward the charged jets. At perhaps some great distance they will recombine with it.

But I don't see how the base of the jets could initially have an overall neutral charge. The accretion disc must be embedded in a powerfully confining magnetic field that turns particles according to charge and mass.
 

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