Improved model shows gamma rays and gold at merging neutron stars

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Improved model shows gamma rays and gold at merging neutron stars

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Post by notFritzArgelander »


Scopes: Refs: Orion ST80, SV 80EDA f7, TS 102ED f11 Newts: AWB 130mm, f5, Z12 f5; Cats: VMC110L, Intes MK66,VMC200L f9.75 EPs: KK Fujiyama Orthoscopics, 2x Vixen NPLs (40-6mm) and BCOs, Baader Mark IV zooms, TV Panoptics, Delos, Plossl 32-8mm. Mixed brand Masuyama/Astroplans Binoculars: Nikon Aculon 10x50, Celestron 15x70, Baader Maxbright. Mounts: Star Seeker IV, Vixen Porta II, Celestron CG5
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Re: Improved model shows gamma rays and gold at merging neutron stars

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Post by helicon »


Excellent vid. Thanks for the article notFritz.
-Michael
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Re: Improved model shows gamma rays and gold at merging neutron stars

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Post by Michael131313 »


Thanks nFA. Is there any way to estimate how much gold is produced?
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Re: Improved model shows gamma rays and gold at merging neutron stars

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Post by notFritzArgelander »


Michael131313 wrote: Thu Oct 22, 2020 5:53 pm Thanks nFA. Is there any way to estimate how much gold is produced?
Thanks for asking this question! This is a point of current study and some controversy: 'How much of the gold (and similar elements) is produced in supernovae versus neutron star mergers?' With that as background I passed over the article's (misleading!) reference to the study having something to do with gold production. Neither the ApJ abstract nor the arXiv preprint of the full article make any reference to the results of this study having anything to do with gold production! What the paper DOES have is a discussion of how r-process elements (like gold) might be formed in the ejecta.

https://iopscience.iop.org/article/10.3 ... 213/abb6ef
We investigate the influence of magnetic fields on the evolution of binary neutron star (BNS) merger remnants via three-dimensional (3D) dynamical-spacetime general-relativistic magnetohydrodynamic (MHD) simulations. We evolve a post-merger remnant with an initial poloidal magnetic field, resolve the magnetoturbulence driven by shear flows, and include a microphysical finite-temperature equation of state. A neutrino leakage scheme that captures the overall energetics and lepton number exchange is also included. We find that turbulence induced by the magnetorotational instability in the hypermassive neutron star (HMNS) amplifies magnetic field to beyond magnetar strength (1015 G). The ultra-strong toroidal field is able to launch a relativistic jet from the HMNS. We also find a magnetized wind that ejects neutron-rich material with a rate of ${\dot{M}}_{\mathrm{ej}}\simeq 1\times {10}^{-1}\,{M}_{\odot }\,{{\rm{s}}}^{-1}$. The total ejecta mass in our simulation is 5 × 10−3 M ⊙. This makes the ejecta from the HMNS an important component in BNS mergers and a promising source of r-process elements that can power a kilonova. The jet from the HMNS reaches a terminal Lorentz factor of ~5 in our highest-resolution simulation. The formation of this jet is aided by neutrino cooling preventing the accretion disk from protruding into the polar region. As neutrino pair-annihilation and radiative processes in the jet (which were not included in the simulations) will boost the Lorentz factor in the jet further, our simulations demonstrate that magnetars formed in BNS mergers are a viable engine for short gamma-ray bursts.
So the short answer to your question is "Yes!" A slightly longer answer is "Yes, but these researchers only computed the environment in which r-process elements (like gold) can be made and folks with nucleosynthesis codes can settle that."

From https://en.wikipedia.org/wiki/R-process ... ical_sites
Current astrophysical models suggest that a single neutron star merger event may have generated between 3 and 13 Earth masses of gold.[29]
Scopes: Refs: Orion ST80, SV 80EDA f7, TS 102ED f11 Newts: AWB 130mm, f5, Z12 f5; Cats: VMC110L, Intes MK66,VMC200L f9.75 EPs: KK Fujiyama Orthoscopics, 2x Vixen NPLs (40-6mm) and BCOs, Baader Mark IV zooms, TV Panoptics, Delos, Plossl 32-8mm. Mixed brand Masuyama/Astroplans Binoculars: Nikon Aculon 10x50, Celestron 15x70, Baader Maxbright. Mounts: Star Seeker IV, Vixen Porta II, Celestron CG5
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Re: Improved model shows gamma rays and gold at merging neutron stars

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Post by Michael131313 »


Thanks so much nFA. That is an amazing amount of gold. I assume that it is flung out into space, but do you think that it is coalesced and arrives at a place like Earth as a bunch, (of course if all of it came to Earth we would not be here and gold wouldn't be so precious 😆) or just spread out and is randomly distributed?
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Re: Improved model shows gamma rays and gold at merging neutron stars

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Post by notFritzArgelander »


Michael131313 wrote: Fri Oct 23, 2020 12:39 am Thanks so much nFA. That is an amazing amount of gold. I assume that it is flung out into space, but do you think that it is coalesced and arrives at a place like Earth as a bunch, (of course if all of it came to Earth we would not be here and gold wouldn't be so precious 😆) or just spread out and is randomly distributed?
It's spread out into the interstellar medium where it gets recycled into stars and planets or ...?
Scopes: Refs: Orion ST80, SV 80EDA f7, TS 102ED f11 Newts: AWB 130mm, f5, Z12 f5; Cats: VMC110L, Intes MK66,VMC200L f9.75 EPs: KK Fujiyama Orthoscopics, 2x Vixen NPLs (40-6mm) and BCOs, Baader Mark IV zooms, TV Panoptics, Delos, Plossl 32-8mm. Mixed brand Masuyama/Astroplans Binoculars: Nikon Aculon 10x50, Celestron 15x70, Baader Maxbright. Mounts: Star Seeker IV, Vixen Porta II, Celestron CG5
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Re: Improved model shows gamma rays and gold at merging neutron stars

#7

Post by Michael131313 »


Thanks once again nFA. That's what I thought but had to ask anyway.
ES AR 102 102mm, f/6.5, ES 254mm f/5 DOB, Obie 10x50, GSO SV 30mm, ES 68° 20mm, ES 82° 14mm, 11mm, 8.8 mm, 6.8mm, 4.7mm. Twilight 1 mount.
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