Richard E. Hughes Neutrinos; p.1 Neutrinos: Little Neutrons. Not!
Neutrinos (and Nucleosynthesis) from Accretion Disks...Accretion disk outflows are a “new” site...
Transcript of Neutrinos (and Nucleosynthesis) from Accretion Disks...Accretion disk outflows are a “new” site...
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Neutrinos (and Nucleosynthesis)
from Accretion Disks
Gail McLaughlin
North Carolina State University
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Explosions of Massive Stars:
What’s happening at the Center?
proto neutronstar core
shockoutflow
black hole, jet
neutrinos
accretion disk
Standard core core collapse SN Accretion disk SN, compact object
merger, gamma ray burst
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Explosions of Massive Stars:
Hydrodynamical Calculations
Core core collapse SN
Blondin & Mezzacappa (2007)
Gamma ray burst jet
Morsony, Lazzati, & Begelman (2007)
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Explosions of Massive Stars:
Where is the nuclear-neutrino physics?
proto neutronstar core
oscillationsneutrino
nucleosynthesis
of core
nuclear physics
neutrino
& emissionscattering
shockoutflow
neutrinos
accretion disk
black hole, jet
nucleosynthesis
neutrino oscillations
nuclear physicsof the disk
neutrino
& emission
scattering
Standard core core collapse SN Accretion disk SN, compact object
merger, gamma ray burst
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Neutrino surfaces:
GCM & R. Surman 2006
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Comparison of Spectra: PNS and low accretion rate disks
In the disk electron neutrinos and antineutrinos have similar energies to
the protoneutron star. Although few muon and tau neutrinos are
produced in “collapsar” type disks.
GCM & R Surman 2006
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Compact Object Merger Models
• Neutron star and black hole
spiral in
• Create an accretion disk
around a black hole
Surman et al 2009
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Importance of accretion disk neutrinos
1. important for energetics of object
2. in principle they are detectable
3. may help power gamma ray bursts
4. influence nucleosynthesis
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Disentangling the signal
Extreme: What if its not a “traditional” core collapse supernova?
Rates:
• Regular supernova ∼ 7000 events, 10 seconds
• Accretion Disk of M = 0.1M/M⊙, 1400 events, 10 seconds
• Black Hole - Neutron Star merger, 9000 events, 0.01 seconds
For events at 10 kpc.
Caballero et al 2009
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Applications to Gamma Ray Bursts
ν-ν annihilation and ν-e scattering
Kneller et al 2006
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Nucleosynthesis in Hot Outflows
Three types of environments
• proto-neutron star supernovae
• accretion disk supernovae
• compact object mergers
Several important types of nucleosynthesis
• r-process
• p-process
•56Ni - an ingredient in light curves
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Neutrino - Nucleosynthesis connection
If neutrinos have most of the energy in an object, they are key to
determining the astrophysical conditions.
Also, they determine the relative numbers of neutrons and protons...
• νe + n ↔ p + e−
• νe + p ↔ n + e+
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Nucleosynthesis in Hot Outflows
n,p →4 He → iron peak nuclei → heavier nuclei
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Nickel in Hot Outflows
n,p →4 He → iron peak nuclei → heavier nuclei
Surman et al 2009
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p-process in GRB’s
Accretion disk outflows are a “new” site for nucleosynthesis
Neutrinos also influence the for-
mation of the p-process elements,
though the neutron-to-proton ratio,
neutrino captures on protons and
neutrino captures on nuclei.
Kizivat et al., in preparation 2009
p-process
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Nucleosynthesis: Compact Object Merger Models
• Neutrino Emission Temper-
atures
• Electron and Anti-electron
Neutrinos
Surman et al 2009
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Accretion Flow Nucleosynthesis
Black Hole Neutron Star Merger
Schematic of events in outflow R-process occurs in the wind
Surman et al. 200817
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Summary
• Neutrinos from accretion disks have somewhat similar spectra to
PNS neutrinos
• Gamma ray bursts make a lot of nickel, and likely some other rare
elements
• Compact object mergers make the r-process in hot outflows
• Neutrinos play an important role in determining the type of
elements formed
• More to understand about astrophysical environment, neutrinos,
and nuclear data
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