Possible Early Linear Acceleration of Proto-neutron Stars via Asymmetric Neutrino Emission in Core-collapse Supernovae
Abstract
In this Letter we present the result of an axisymmetric core-collapse supernovae simulation conducted with appropriate treatments of neutrino transport and proper motions of proto-neutron stars (PNSs), in which a remarkable PNS acceleration is observed in association with asymmetric neutrino emissions 300 ms after bounce. We find that these asymmetric neutrino emissions play important roles in the acceleration of PNSs in this phase. The correlation between the PNS proper motion and the asymmetric ejecta is similar to that in a neutron star (NS) kick of hydrodynamic origin. Both electron-type neutrinos (ν e) and their anti-particles ($${\bar{\nu }}_{{\rm{e}}}$$) have a ~10% level of asymmetry between the northern and southern hemispheres, while other heavy-leptonic neutrinos (ν x ) have much a smaller asymmetry of ~1%. The emissions of $${\bar{\nu }}_{{\rm{e}}}$$ and ν x are higher in the hemisphere of stronger shock expansion, whereas the ν e emission is enhanced in the opposite hemisphere: in total, the neutrinos carry some linear momentum to the hemisphere of the stronger shock expansion. This asymmetry is attributed to the non-spherical distribution of electron-fraction (Y e ) in the envelope of PNS. Although it is similar to lepton-emission self-sustained asymmetry, the Y e asymmetry seems to be associated with the PNS motion: the latter triggers lateral circular motions in the envelope of PNS by breaking the symmetry of the matter distribution there, which is then sustained by a combination of convection, lateral neutrino diffusion, and matter-pressure gradient. Our findings may have an influence on the current theories on the NS kick mechanism, although long-term simulations are required to assess their impact on later evolution.
- Authors:
-
- Princeton Univ., NJ (United States)
- Numazu College of Technology (Japan)
- Waseda Univ., Tokyo (Japan)
- Publication Date:
- Research Org.:
- Univ. of California, Oakland, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC)
- OSTI Identifier:
- 1612914
- Grant/Contract Number:
- SC0018297
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal. Letters (Online)
- Additional Journal Information:
- Journal Name: The Astrophysical Journal. Letters (Online); Journal Volume: 880; Journal Issue: 2; Journal ID: ISSN 2041-8213
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; astronomy & astrophysics; hydrodynamics; neutrinos; radiative transfer; supernovae
Citation Formats
Nagakura, Hiroki, Sumiyoshi, Kohsuke, and Yamada, Shoichi. Possible Early Linear Acceleration of Proto-neutron Stars via Asymmetric Neutrino Emission in Core-collapse Supernovae. United States: N. p., 2019.
Web. doi:10.3847/2041-8213/ab30ca.
Nagakura, Hiroki, Sumiyoshi, Kohsuke, & Yamada, Shoichi. Possible Early Linear Acceleration of Proto-neutron Stars via Asymmetric Neutrino Emission in Core-collapse Supernovae. United States. https://doi.org/10.3847/2041-8213/ab30ca
Nagakura, Hiroki, Sumiyoshi, Kohsuke, and Yamada, Shoichi. Wed .
"Possible Early Linear Acceleration of Proto-neutron Stars via Asymmetric Neutrino Emission in Core-collapse Supernovae". United States. https://doi.org/10.3847/2041-8213/ab30ca. https://www.osti.gov/servlets/purl/1612914.
@article{osti_1612914,
title = {Possible Early Linear Acceleration of Proto-neutron Stars via Asymmetric Neutrino Emission in Core-collapse Supernovae},
author = {Nagakura, Hiroki and Sumiyoshi, Kohsuke and Yamada, Shoichi},
abstractNote = {In this Letter we present the result of an axisymmetric core-collapse supernovae simulation conducted with appropriate treatments of neutrino transport and proper motions of proto-neutron stars (PNSs), in which a remarkable PNS acceleration is observed in association with asymmetric neutrino emissions 300 ms after bounce. We find that these asymmetric neutrino emissions play important roles in the acceleration of PNSs in this phase. The correlation between the PNS proper motion and the asymmetric ejecta is similar to that in a neutron star (NS) kick of hydrodynamic origin. Both electron-type neutrinos (ν e) and their anti-particles (${\bar{\nu }}_{{\rm{e}}}$) have a ~10% level of asymmetry between the northern and southern hemispheres, while other heavy-leptonic neutrinos (ν x ) have much a smaller asymmetry of ~1%. The emissions of ${\bar{\nu }}_{{\rm{e}}}$ and ν x are higher in the hemisphere of stronger shock expansion, whereas the ν e emission is enhanced in the opposite hemisphere: in total, the neutrinos carry some linear momentum to the hemisphere of the stronger shock expansion. This asymmetry is attributed to the non-spherical distribution of electron-fraction (Y e ) in the envelope of PNS. Although it is similar to lepton-emission self-sustained asymmetry, the Y e asymmetry seems to be associated with the PNS motion: the latter triggers lateral circular motions in the envelope of PNS by breaking the symmetry of the matter distribution there, which is then sustained by a combination of convection, lateral neutrino diffusion, and matter-pressure gradient. Our findings may have an influence on the current theories on the NS kick mechanism, although long-term simulations are required to assess their impact on later evolution.},
doi = {10.3847/2041-8213/ab30ca},
journal = {The Astrophysical Journal. Letters (Online)},
number = 2,
volume = 880,
place = {United States},
year = {2019},
month = {7}
}
Web of Science
Works referenced in this record:
Three-dimensional neutrino-driven supernovae: Neutron star kicks, spins, and asymmetric ejection of nucleosynthesis products
journal, April 2013
- Wongwathanarat, A.; Janka, H. -Th.; Müller, E.
- Astronomy & Astrophysics, Vol. 552
Theoretical support for the hydrodynamic mechanism of pulsar kicks
journal, November 2010
- Nordhaus, J.; Brandt, T. D.; Burrows, A.
- Physical Review D, Vol. 82, Issue 10
Variational study for the equation of state of asymmetric nuclear matter at finite temperatures
journal, March 2013
- Togashi, H.; Takano, M.
- Nuclear Physics A, Vol. 902
A Detailed Comparison of Multidimensional Boltzmann Neutrino Transport Methods in Core-collapse Supernovae
journal, October 2017
- Richers, Sherwood; Nagakura, Hiroki; Ott, Christian D.
- The Astrophysical Journal, Vol. 847, Issue 2
Delayed pulsar kicks from the emission of sterile neutrinos
journal, June 2008
- Kusenko, Alexander; Mandal, Bhabani Prasad; Mukherjee, Alok
- Physical Review D, Vol. 77, Issue 12
A Comparison of two- and Three-Dimensional Neutrino-Hydrodynamics Simulations of Core-Collapse Supernovae
journal, April 2014
- Takiwaki, Tomoya; Kotake, Kei; Suwa, Yudai
- The Astrophysical Journal, Vol. 786, Issue 2
High birth velocities of radio pulsars
journal, May 1994
- Lyne, A. G.; Lorimer, D. R.
- Nature, Vol. 369, Issue 6476
The Explosion Mechanism of Core-Collapse Supernovae: Progress in Supernova Theory and Experiments
journal, January 2015
- Foglizzo, Thierry; Kazeroni, Rémi; Guilet, Jérôme
- Publications of the Astronomical Society of Australia, Vol. 32
A new equation of state for core-collapse supernovae based on realistic nuclear forces and including a full nuclear ensemble
journal, July 2017
- Furusawa, S.; Togashi, H.; Nagakura, H.
- Journal of Physics G: Nuclear and Particle Physics, Vol. 44, Issue 9
Direct Measurement of Neutron Star Recoil in the Oxygen‐rich Supernova Remnant Puppis A
journal, November 2007
- Winkler, P. Frank; Petre, Robert
- The Astrophysical Journal, Vol. 670, Issue 1
Pulsar kicks from a dark-matter sterile neutrino
journal, November 2003
- Fuller, George M.; Kusenko, Alexander; Mocioiu, Irina
- Physical Review D, Vol. 68, Issue 10
Birth and Evolution of Isolated Radio Pulsars
journal, May 2006
- Faucher‐Giguere, Claude‐Andre; Kaspi, Victoria M.
- The Astrophysical Journal, Vol. 643, Issue 1
Asymmetric neutrino emission and formation of rapidly moving pulsars
journal, January 1993
- Bisnovatyi-Kogan, G. S.
- Astronomical & Astrophysical Transactions, Vol. 3, Issue 4
Pulsar kicks by anisotropic neutrino emission from quark matter in strong magnetic fields
journal, July 2008
- Sagert, I.; Schaffner-Bielich, J.
- Astronomy & Astrophysics, Vol. 489, Issue 1
The Velocity Distribution of Isolated Radio Pulsars
journal, March 2002
- Arzoumanian, Z.; Chernoff, D. F.; Cordes, J. M.
- The Astrophysical Journal, Vol. 568, Issue 1
Multidimensional supernova simulations with approximative neutrino transport: II. Convection and the advective-acoustic cycle in the supernova core
journal, December 2007
- Scheck, L.; Janka, H. -Th.; Foglizzo, T.
- Astronomy & Astrophysics, Vol. 477, Issue 3
A statistical study of 233 pulsar proper motions
journal, July 2005
- Hobbs, G.; Lorimer, D. R.; Lyne, A. G.
- Monthly Notices of the Royal Astronomical Society, Vol. 360, Issue 3
Three-Dimensional Boltzmann Hydro code for core Collapse in Massive Stars. i. Special Relativistic Treatments
journal, September 2014
- Nagakura, Hiroki; Sumiyoshi, Kohsuke; Yamada, Shoichi
- The Astrophysical Journal Supplement Series, Vol. 214, Issue 2
Intermediate-mass Elements in Young Supernova Remnants Reveal Neutron Star Kicks by Asymmetric Explosions
journal, March 2018
- Katsuda, Satoru; Morii, Mikio; Janka, Hans-Thomas
- The Astrophysical Journal, Vol. 856, Issue 1
Multidimensional supernova simulations with approximative neutrino transport: I. Neutron star kicks and the anisotropy of neutrino-driven explosions in two spatial dimensions
journal, September 2006
- Scheck, L.; Kifonidis, K.; Janka, H. -Th.
- Astronomy & Astrophysics, Vol. 457, Issue 3
Simulations of Core-collapse Supernovae in Spatial Axisymmetry with Full Boltzmann Neutrino Transport
journal, February 2018
- Nagakura, Hiroki; Iwakami, Wakana; Furusawa, Shun
- The Astrophysical Journal, Vol. 854, Issue 2
Comparing Neutron Star Kicks to Supernova Remnant Asymmetries
journal, July 2017
- Holland-Ashford, Tyler; Lopez, Laura A.; Auchettl, Katie
- The Astrophysical Journal, Vol. 844, Issue 1
The hydrodynamic origin of neutron star kicks: Neutron star kicks
journal, April 2012
- Nordhaus, J.; Brandt, T. D.; Burrows, A.
- Monthly Notices of the Royal Astronomical Society, Vol. 423, Issue 2
Comparing Treatments of Weak Reactions with Nuclei in Simulations of Core-collapse Supernovae
journal, February 2019
- Nagakura, Hiroki; Furusawa, Shun; Togashi, Hajime
- The Astrophysical Journal Supplement Series, Vol. 240, Issue 2
Hydrodynamical Neutron-star Kicks in Electron-capture Supernovae and Implications for the CRAB Supernova
journal, September 2018
- Gessner, Alexandra; Janka, Hans-Thomas
- The Astrophysical Journal, Vol. 865, Issue 1
Getting Its Kicks: A VLBA Parallax for the Hyperfast Pulsar B1508+55
journal, August 2005
- Chatterjee, S.; Vlemmings, W. H. T.; Brisken, W. F.
- The Astrophysical Journal, Vol. 630, Issue 1
Self-Sustained Asymmetry of Lepton-Number Emission: a new Phenomenon During the Supernova Shock-Accretion Phase in Three Dimensions
journal, August 2014
- Tamborra, Irene; Hanke, Florian; Janka, Hans-Thomas
- The Astrophysical Journal, Vol. 792, Issue 2
Physics of Core-Collapse Supernovae in Three Dimensions: A Sneak Preview
journal, October 2016
- Janka, Hans-Thomas; Melson, Tobias; Summa, Alexander
- Annual Review of Nuclear and Particle Science, Vol. 66, Issue 1
Neutron Star Kicks by the Gravitational Tug-boat Mechanism in Asymmetric Supernova Explosions: Progenitor and Explosion Dependence
journal, March 2017
- Janka, Hans-Thomas
- The Astrophysical Journal, Vol. 837, Issue 1
The evolution and explosion of massive stars
journal, November 2002
- Woosley, S. E.; Heger, A.; Weaver, T. A.
- Reviews of Modern Physics, Vol. 74, Issue 4
Two-dimensional hydrodynamic core-collapse supernova simulations with spectral neutrino transport: II. Models for different progenitor stars
journal, September 2006
- Buras, R.; Janka, H. -Th.; Rampp, M.
- Astronomy & Astrophysics, Vol. 457, Issue 1
A new Multi-Dimensional General Relativistic Neutrino Hydrodynamics code for Core-Collapse Supernovae. ii. Relativistic Explosion Models of Core-Collapse Supernovae
journal, August 2012
- Müller, Bernhard; Janka, Hans-Thomas; Marek, Andreas
- The Astrophysical Journal, Vol. 756, Issue 1
The Status of Multi-Dimensional Core-Collapse Supernova Models
journal, January 2016
- Müller, B.
- Publications of the Astronomical Society of Australia, Vol. 33
Three-dimensional Boltzmann-Hydro Code for Core-collapse in Massive Stars. II. The Implementation of Moving-mesh for Neutron Star Kicks
journal, April 2017
- Nagakura, Hiroki; Iwakami, Wakana; Furusawa, Shun
- The Astrophysical Journal Supplement Series, Vol. 229, Issue 2
Pulsar Recoil by Large-Scale Anisotropies in Supernova Explosions
journal, January 2004
- Scheck, L.; Plewa, T.; Janka, H. -Th.
- Physical Review Letters, Vol. 92, Issue 1
Two-dimensional hydrodynamic core-collapse supernova simulations with spectral neutrino transport: I. Numerical method and results for a 15
journal, February 2006
- Buras, R.; Rampp, M.; Janka, H. -Th.
- Astronomy & Astrophysics, Vol. 447, Issue 3
Pulsar kicks by anisotropic neutrino emission from quark matter in strong magnetic fields
text, January 2007
- Sagert, I.; Schaffner-Bielich, J.
- arXiv
Delayed pulsar kicks from the emission of sterile neutrinos
text, January 2008
- Kusenko, Alexander; Mandal, Bhabani Prasad; Mukherjee, Alok
- arXiv
Theoretical Support for the Hydrodynamic Mechanism of Pulsar Kicks
text, January 2010
- Nordhaus, J.; Brandt, T. D.; Burrows, A.
- arXiv
Three-dimensional neutrino-driven supernovae: Neutron star kicks, spins, and asymmetric ejection of nucleosynthesis products
text, January 2012
- Wongwathanarat, A.; Janka, H. -Th.; Mueller, E.
- arXiv
Variational study for the equation of state of asymmetric nuclear matter at finite temperatures
text, January 2013
- Togashi, H.; Takano, M.
- arXiv
Self-sustained asymmetry of lepton-number emission: A new phenomenon during the supernova shock-accretion phase in three dimensions
text, January 2014
- Tamborra, Irene; Hanke, Florian; Janka, Hans-Thomas
- arXiv
The explosion mechanism of core-collapse supernovae: progress in supernova theory and experiments
text, January 2015
- Foglizzo, Thierry; Kazeroni, Rémi; Guilet, Jérôme
- arXiv
Three-dimensional Boltzmann-Hydro code for core-collapse in massive stars II. The Implementation of moving-mesh for neutron star kicks
text, January 2016
- Nagakura, Hiroki; Iwakami, Wakana; Furusawa, Shun
- arXiv
Simulations of core-collapse supernovae in spatial axisymmetry with full Boltzmann neutrino transport
text, January 2017
- Nagakura, Hiroki; Iwakami, Wakana; Furusawa, Shun
- arXiv
Comparing Neutron Star Kicks to Supernova Remnant Asymmetries
text, January 2017
- Holland-Ashford, Tyler; Lopez, Laura A.; Auchettl, Katie
- arXiv
A new equation of state for core-collapse supernovae based on realistic nuclear forces and including a full nuclear ensemble
text, January 2017
- Furusawa, S.; Togashi, H.; Nagakura, H.
- arXiv
Comparing treatments of weak reactions with nuclei in simulations of core-collapse supernovae
text, January 2018
- Nagakura, Hiroki; Furusawa, Shun; Togashi, Hajime
- arXiv
Pulsar kicks from a dark-matter sterile neutrino
text, January 2003
- Fuller, George M.; Kusenko, Alexander; Mocioiu, Irina
- arXiv
A statistical study of 233 pulsar proper motions
text, January 2005
- Hobbs, G.; Lorimer, D. R.; Lyne, A. G.
- arXiv
Getting Its Kicks: A VLBA Parallax for the Hyperfast Pulsar B1508+55
text, January 2005
- Chatterjee, S.; Vlemmings, W. H. T.; Brisken, W. F.
- arXiv
Asymmetric neutrino emision and formation of rapidly moving pulsars
text, January 1997
- Bisnovatyi-Kogan, G. S.
- arXiv
Works referencing / citing this record:
Fast-pairwise Collective Neutrino Oscillations Associated with Asymmetric Neutrino Emissions in Core-collapse Supernovae
journal, November 2019
- Nagakura, Hiroki; Morinaga, Taiki; Kato, Chinami
- The Astrophysical Journal, Vol. 886, Issue 2