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Neutrinos and from Hole Disks

Gail McLaughlin North Carolina State University

1 Neutrino Astrophysics • What do neutrinos do in astrophysical environments? • What do neutrinos in a core collapse do? • What do neutrinos in a gamma ray burst do? • What do neutrinos in a compact object merger do? Nuclear Astrophysics • What is the origin of the elements? • Where are the heaviest elements made? • What elements are made in compact object mergers/ stellar explosions?

2 - Accretion Disk Neutrinos

• black hole - accretion disks form in some supernovae, compact object mergers and gamma ray bursts • νs important for disk energetics • νs in principle are detectable • νs may help power gamma ray bursts • νs influence nucleosynthesis

3 Explosions of Massive : What’s happening at the Center?

black hole, jet shock outflow

neutrinos

accretion disk

proto neutron core

Standard core core collapse SN Accretion disk SN, compact object merger, gamma ray burst

4 Explosions of Massive Stars: Hydrodynamical Calculations

Core core collapse SN Gamma ray burst jet

Blondin & Mezzacappa (2007) Morsony, Lazzati, & Begelman (2007)

5 Explosions of Massive Stars: Where is the nuclear-neutrino physics?

neutrino nucleosynthesis oscillations black hole, jet shock nucleosynthesis outflow neutrino oscillations neutrinos

accretion disk neutrino neutrino nuclear physics scattering scattering of the disk nuclear physics proto neutron & emission star core & emission of core

Standard core core collapse SN Accretion disk SN, compact object merger, gamma ray burst

6 Neutrino surfaces:

GCM & R. Surman 2006

7 Comparison of Spectra: PNS and low accretion rate disks

Electron neutrinos and antineutrinos from disks have similar energies to neutrinos from protoneutron stars.

GCM & R Surman 2006

8 Compact Object Merger Models

and black hole spiral in • Create an accretion disk around a black hole

Surman et al 2009

9 Neutrino Detection

Extreme: What if the next direct supernova neutrino detection is 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

10 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

11 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

+ • ν¯e + p ↔ n + e

12 Nucleosynthesis in Hot Outflows n,p →4 He → iron peak nuclei → heavier nuclei

13 Nickel in Hot Outflows n,p →4 He → iron peak nuclei → heavier nuclei

Surman et al 2010

14 Neutrinos and light p-nucleosynthesis

Thought to occur in supernovae and in accretion disk outflows ν-p process p-process

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103 i, /Y i Y 102

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100 40 45 50 55 60 65 70 75 80 85 90 95 100 Number A

Frohlich et al 2007, Kizivat et al 2010

15 Pruet et al, Surman et al 2005, 2010 Nucleosynthesis: Compact Object Merger Models

• Neutrino Emission Temper- atures • Electron and Anti-electron Neutrinos

Surman et al 2009

16 Hot Outflow Nucleosynthesis Black Hole Neutron Star Merger

Schematic of events in outflow R-process occurs in the

Surman et al. 2008 17 Improvements needed in the treatment of Disk Neutrinos

• hydrodynamic calculations • general relativistic effects • neutrino transport • neutrino flavor transforma- tion

Neutrino bending, figure by Liliana Caballero

18 Summary • Neutrinos from accretion disks have somewhat similar spectra to proto-neutron star 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 and neutrinos

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