Neutrinos from type Ia supernovae: The deflagration-to-detonation transition scenario

Wright, Warren P.; Nagaraj, Gautam; Kneller, James P.; Scholberg, Kate; Seitenzahl, Ivo R.

doi:10.1103/PhysRevD.94.025026

Title: Neutrinos from type Ia supernovae: The deflagration-to-detonation transition scenario

Abstract

It has long been recognized that the neutrinos detected from the next core-collapse supernova in the Galaxy have the potential to reveal important information about the dynamics of the explosion and the nucleosynthesis conditions as well as allowing us to probe the properties of the neutrino itself. The neutrinos emitted from thermonuclear—type Ia—supernovae also possess the same potential, although these supernovae are dimmer neutrino sources. For the first time, we calculate the time, energy, line of sight, and neutrino-flavor-dependent features of the neutrino signal expected from a three-dimensional delayed-detonation explosion simulation, where a deflagration-to-detonation transition triggers the complete disruption of a near-Chandrasekhar mass carbon-oxygen white dwarf. We also calculate the neutrino flavor evolution along eight lines of sight through the simulation as a function of time and energy using an exact three-flavor transformation code. We identify a characteristic spectral peak at ˜10 MeV as a signature of electron captures on copper. This peak is a potentially distinguishing feature of explosion models since it reflects the nucleosynthesis conditions early in the explosion. We simulate the event rates in the Super-K, Hyper-K, JUNO, and DUNE neutrino detectors with the SNOwGLoBES event rate calculation software and also compute the IceCube signal. Hyper-K willmore »« less

Authors:

Wright, Warren P. ^[1]; Nagaraj, Gautam ^[1]; Kneller, James P. ^[1]; Scholberg, Kate ^[2]; Seitenzahl, Ivo R. ^[3]

North Carolina State Univ., Raleigh, NC (United States)
Duke Univ., Durham, NC (United States)
Australian National Univ., Canberra, ACT (Australia); ARC Centre of Excellence for All-Sky Astrophysics (CAASTRO) (Australia)

Publication Date:: Tue Jul 19 00:00:00 EDT 2016

Research Org.:: North Carolina State University, Raleigh, NC (United States)

Sponsoring Org.:: USDOE Office of Science (SC), Nuclear Physics (NP)

OSTI Identifier:: 1325194

Alternate Identifier(s):: OSTI ID: 1264796

Grant/Contract Number:: SC0006417

Resource Type:: Journal Article: Accepted Manuscript

Journal Name:: Physical Review D

Additional Journal Information:: Journal Volume: 94; Journal Issue: 2; Journal ID: ISSN 2470-0010

Publisher:: American Physical Society (APS)

Country of Publication:: United States

Language:: English

Subject:: 79 ASTRONOMY AND ASTROPHYSICS; 73 NUCLEAR PHYSICS AND RADIATION PHYSICS; 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; neutrinos; thermonuclear supernova

Citation Formats


                    Wright, Warren P., Nagaraj, Gautam, Kneller, James P., Scholberg, Kate, and Seitenzahl, Ivo R. Neutrinos from type Ia supernovae: The deflagration-to-detonation transition scenario.  United States: N. p., 2016. 
        Web.  doi:10.1103/PhysRevD.94.025026.

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                    Wright, Warren P., Nagaraj, Gautam, Kneller, James P., Scholberg, Kate, & Seitenzahl, Ivo R. Neutrinos from type Ia supernovae: The deflagration-to-detonation transition scenario.  United States.  https://doi.org/10.1103/PhysRevD.94.025026

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                    Wright, Warren P., Nagaraj, Gautam, Kneller, James P., Scholberg, Kate, and Seitenzahl, Ivo R. 2016.  
        "Neutrinos from type Ia supernovae: The deflagration-to-detonation transition scenario".  United States.  https://doi.org/10.1103/PhysRevD.94.025026.  https://www.osti.gov/servlets/purl/1325194.

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@article{osti_1325194,

  title        = {Neutrinos from type Ia supernovae: The deflagration-to-detonation transition scenario},

  author       = {Wright, Warren P. and Nagaraj, Gautam and Kneller, James P. and Scholberg, Kate and Seitenzahl, Ivo R.},

  abstractNote = {It has long been recognized that the neutrinos detected from the next core-collapse supernova in the Galaxy have the potential to reveal important information about the dynamics of the explosion and the nucleosynthesis conditions as well as allowing us to probe the properties of the neutrino itself. The neutrinos emitted from thermonuclear—type Ia—supernovae also possess the same potential, although these supernovae are dimmer neutrino sources. For the first time, we calculate the time, energy, line of sight, and neutrino-flavor-dependent features of the neutrino signal expected from a three-dimensional delayed-detonation explosion simulation, where a deflagration-to-detonation transition triggers the complete disruption of a near-Chandrasekhar mass carbon-oxygen white dwarf. We also calculate the neutrino flavor evolution along eight lines of sight through the simulation as a function of time and energy using an exact three-flavor transformation code. We identify a characteristic spectral peak at ˜10 MeV as a signature of electron captures on copper. This peak is a potentially distinguishing feature of explosion models since it reflects the nucleosynthesis conditions early in the explosion. We simulate the event rates in the Super-K, Hyper-K, JUNO, and DUNE neutrino detectors with the SNOwGLoBES event rate calculation software and also compute the IceCube signal. Hyper-K will be able to detect neutrinos from our model out to a distance of ˜10 kpc. Here, at 1 kpc, JUNO, Super-K, and DUNE would register a few events while IceCube and Hyper-K would register several tens of events.},

  doi          = {10.1103/PhysRevD.94.025026},

  url          = {https://www.osti.gov/biblio/1325194},
  journal      = {Physical Review D},

  issn         = {2470-0010},

  number       = 2,

  volume       = 94,

  place        = {United States},

  year         = {Tue Jul 19 00:00:00 EDT 2016},

  month        = {Tue Jul 19 00:00:00 EDT 2016}

}

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Search for transient optical counterparts to high-energy IceCube neutrinos with Pan-STARRS1
journal, June 2019

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Title: Neutrinos from type Ia supernovae: The deflagration-to-detonation transition scenario

Abstract

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journal, August 2014

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journal, June 2009

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journal, December 2015

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journal, December 2012

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journal, August 1989

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journal, October 2012

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journal, June 2013

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journal, December 2006

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journal, August 2012

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journal, December 2015

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journal, June 2003

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journal, October 2006

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journal, March 1994

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journal, January 2012

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journal, November 2006

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journal, April 2008

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journal, August 2014

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journal, April 2011

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journal, February 2016

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journal, June 2007

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journal, August 1993

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journal, June 2012

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journal, November 2009

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journal, December 2011

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journal, November 2008

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journal, May 1978

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journal, August 2014

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journal, July 2005

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journal, September 1998

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journal, March 2016

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journal, June 2010

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journal, February 2007

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journal, January 2015

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journal, January 2000

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journal, January 2009

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journal, March 2006

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journal, April 2009

Seeing the Collision of a Supernova with its Companion star
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A possible model of supernovae: Detonation of12C
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A subgrid-scale model for deflagration-to-detonation transitions in Type Ia supernova explosion simulations: Numerical implementation
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EARLY RADIO AND X-RAY OBSERVATIONS OF THE YOUNGEST NEARBY TYPE Ia SUPERNOVA PTF 11kly (SN 2011fe)
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Study of the effect of neutrino oscillations on the supernova neutrino signal in the LVD detector
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New approaches to SNe Ia progenitors
journal, October 2014

Circumstellar Material in Type Ia Supernovae via Sodium Absorption Features
journal, August 2011

Core-collapse astrophysics with a five-megaton neutrino detector
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Detection of Circumstellar Material in a Normal Type Ia Supernova
journal, August 2007

Neutrino physics with the KamLAND detector
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The Reddening-Free Decline Rate Versus Luminosity Relationship for Type [CLC]Ia[/CLC] Supernovae
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Spectral analysis of the 91bg-like Type Ia SN 2005bl: low luminosity, low velocities, incomplete burning
journal, November 2009

A CHANDRASEKHAR MASS PROGENITOR FOR THE TYPE Ia SUPERNOVA REMNANT 3C 397 FROM THE ENHANCED ABUNDANCES OF NICKEL AND MANGANESE
journal, March 2015

Three-dimensional delayed-detonation models with nucleosynthesis for Type Ia supernovae
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When do neutrinos cease to oscillate?
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IceCube sensitivity for low-energy neutrinos from nearby supernovae
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Towards an understanding of Type Ia supernovae from a synthesis of theory and observations
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Three flavor neutrino oscillations in matter: Flavor diagonal potentials, the adiabatic basis, and the $C P$ phase
journal, September 2009

SUBCLASSES OF TYPE Ia SUPERNOVAE AS THE ORIGIN OF [ α /Fe] RATIOS IN DWARF SPHEROIDAL GALAXIES
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Double-detonation sub-Chandrasekhar supernovae: can minimum helium shell masses detonate the core?
journal, May 2010

Observing the next Galactic Supernova
journal, November 2013

Observation of a neutrino burst in coincidence with supernova 1987A in the Large Magellanic Cloud
journal, April 1987

Delay times and rates for Type Ia supernovae and thermonuclear explosions from double-detonation sub-Chandrasekhar mass models: Thermonuclear double-detonations as SNe Ia
journal, August 2011

Reconstructing the supernova bounce time with neutrinos in IceCube
journal, October 2009

Observation of a neutrino burst from the supernova SN1987A
journal, April 1987

Neutrino flavour transformation in supernovae
journal, September 2009

Phase effects in neutrino conversions during a supernova shock wave
journal, May 2007

Neutrino physics with JUNO
journal, February 2016

The UV/optical spectra of the Type Ia supernova SN 2010jn: a bright supernova with outer layers rich in iron-group elements
journal, January 2013

Supernova Type Ia progenitors from merging double white dwarfs: Using a new population synthesis model⋆
journal, October 2012

Collective Neutrino Oscillations
journal, November 2010

EVLA OBSERVATIONS CONSTRAIN THE ENVIRONMENT AND PROGENITOR SYSTEM OF Type Ia SUPERNOVA 2011fe
journal, April 2012

Search for Supernova Neutrino Bursts at Super‐Kamiokande
journal, November 2007

Nonadiabatic Level Crossing in Resonant Neutrino Oscillations
journal, September 1986

Solar abundance of manganese: a case for near Chandrasekhar-mass Type Ia supernova progenitors
journal, November 2013

PROSPECT OF STUDYING HARD X- AND GAMMA-RAYS FROM TYPE Ia SUPERNOVAE
journal, November 2012

VERY LATE PHOTOMETRY OF SN 2011fe
journal, November 2014

Core-Collapse Supernova Equations of State Based on Neutron star Observations
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Stellar weak interaction rates for intermediate-mass nuclei. II - A = 21 to A = 60
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A new open-source code for spherically symmetric stellar collapse to neutron stars and black holes
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