Fetching the paper…
Reading the bibliography…
During the accretion phase of a core-collapse supernovae, large amplitude turbulence is generated by the combination of the standing accretion shock instability and convection driven by neutrino heating.
L. Wolfenstein, “Neutrino oscillations in matter,” Phys. Rev. D , vol. 17, pp. 2369–2374, May 1978
1978
Earlier work this paper cites.
S. P. Mikheyev and A. Y. Smirnov, “Resonance enhancement of oscillations in matter and solar neutrino spectroscopy,” Yad. Fiz. , vol. 42, p. 1441, 1985, ( Sov. J. Nucl. Phys
1985
Earlier work this paper cites.
——, “Neutrino oscillations in matter with varying density,” in ’86 Massive Neutrinos in Astrophysics and in Particle Physics , O. Frackler and J. Trân Thanh Vân, Eds. Gif-sur-Yvette: Editions Frontières, 1986, p. 355
1986
Earlier work this paper cites.
P. Langacker, S. T. Petcov, G. Steigman, and S. Toshev, “Implications of the mikheyev-smirnov-wolfenstein (MSW) mechanism of amplification of neutrino oscillations in matter,” Nuclear Physics B , vol. 282, pp. 589–609, 1987
1987
Earlier work this paper cites.
R. F. Sawyer, “Neutrino oscillations in inhomogeneous matter.” Phys. Rev. , vol. 42, p. 3908, Dec. 1990
1990
Earlier work this paper cites.
G. Falkovich, “Bottleneck phenomenon in developed turbulence,” Physics of Fluids , vol. 6, pp. 1411–1414, Apr. 1994
1994
Earlier work this paper cites.
F. N. Loreti, Y.-Z. Qian, G. M. Fuller, and A. B. Balantekin, “Effects of random density fluctuations on matter enhanced neutrino flavor transitions in supernovae and implications for supernova dynamics and nucleosynthesis,” Phys. Rev. , vol. 52, p. 6664, 1995
1995
Earlier work this paper cites.
A. B. Balantekin, J. M. Fetter, and F. N. Loreti, “MSW effect in a fluctuating matter density,” Phys. Rev. D , vol. 54, pp. 3941–3951, Sep. 1996
1996
Earlier work this paper cites.
M. Liebendörfer, A. Mezzacappa, F.-K. Thielemann, O. E. Messer, W. R. Hix, and S. W. Bruenn, “Probing the gravitational well: No supernova explosion in spherical symmetry with general relativistic Boltzmann neutrino transport,” Phys. Rev. D , vol. 63, no. 10, p. 103004, May 2001
2001
Earlier work this paper cites.
A. Mezzacappa, M. Liebendörfer, O. E. Messer, W. R. Hix, F.-K. Thielemann, and S. W. Bruenn, “Simulation of the Spherically Symmetric Stellar Core Collapse, Bounce, and Postbounce Evolution of a Star of 13 Solar Masses with Boltzmann Neutrino Transport, and Its Implications for the Supernova Mechanism,” Physical Review Letters , vol. 86, pp. 1935–1938, Mar. 2001
2001
Earlier work this paper cites.
J. M. Blondin, A. Mezzacappa, and C. DeMarino, “Stability of Standing Accretion Shocks, with an Eye toward Core-Collapse Supernovae,” Astrophys. J. , vol. 584, pp. 971–980, Feb. 2003
2003
Earlier work this paper cites.
W. Dobler, N. E. Haugen, T. A. Yousef, and A. Brandenburg, “Bottleneck effect in three-dimensional turbulence simulations,” Phys. Rev. , vol. 68, no. 2, p. 026304, Aug. 2003
2003
Earlier work this paper cites.
P. A. Mazzali, K. S. Kawabata, K. Maeda, K. Nomoto, A. V. Filippenko, E. Ramirez-Ruiz, S. Benetti, E. Pian, J. Deng, N. Tominaga, Y. Ohyama, M. Iye, R. J. Foley, T. Matheson, L. Wang, and A. Gal-Yam, “An Asymmetric Energetic Type Ic Supernova Viewed Off-Axis, and a Link to Gamma Ray Bursts,” Science , vol. 308, pp. 1284–1287, May 2005
2005
Earlier work this paper cites.
R. Buras, M. Rampp, H.-T. Janka, and K. Kifonidis, “Two-dimensional hydrodynamic core-collapse supernova simulations with spectral neutrino transport. I. Numerical method and results for a 15 M ⊙ {\odot} star,” Astronomy & Astrophysics , vol. 447, pp. 1049–1092, Mar. 2006
2006
Earlier work this paper cites.
K. Kifonidis, T. Plewa, L. Scheck, H.-T. Janka, and E. Müller, “Non-spherical core collapse supernovae. II. The late-time evolution of globally anisotropic neutrino-driven explosions and their implications for SN 1987 A,” Astronomy & Astrophysics , vol. 453, pp. 661–678, Jul. 2006
2006
Earlier work this paper cites.
A. Friedland and A. Gruzinov, “Neutrino signatures of supernova turbulence,” 2006
2006
Earlier work this paper cites.
G. Fogli, E. Lisi, A. Mirizzi, and D. Montanino, “Damping of supernova neutrino transitions in stochastic shock-wave density profiles,” J. Cosm. Astropart. Phys. , vol. 0606, p. 012, Jun. 2006
2006
Earlier work this paper cites.
H. Duan, G. M. Fuller, J. Carlson, and Y.-Z. Qian, “Simulation of coherent non-linear neutrino flavor transformation in the supernova environment. i: Correlated neutrino trajectories,” Phys. Rev. , vol. 74, p. 105014, 2006
2006
Earlier work this paper cites.
——, “Coherent development of neutrino flavor in the supernova environment,” Phys. Rev. Lett. , vol. 97, p. 241101, 2006
2006
Earlier work this paper cites.
A. Burrows, L. Dessart, C. D. Ott, and E. Livne, “Multi-dimensional explorations in supernova theory,” Physics Reports , vol. 442, pp. 23–37, Apr. 2007
2007
Cited alongside, same era.
S. Choubey, N. P. Harries, and G. G. Ross, “Turbulent supernova shock waves and the sterile neutrino signature in megaton water detectors,” Phys. Rev. , vol. 76, no. 7, p. 073013, Oct. 2007
2007
Cited alongside, same era.
W. Iwakami, K. Kotake, N. Ohnishi, S. Yamada, and K. Sawada, “Three-Dimensional Simulations of Standing Accretion Shock Instability in Core-Collapse Supernovae,” Astrophysical Journal , vol. 678, pp. 1207–1222, May 2008
2008
Cited alongside, same era.
A. Esteban-Pretel, S. Pastor, R. Tomàs, G. G. Raffelt, and G. Sigl, “Mu-tau neutrino refraction and collective three-flavor transformations in supernovae,” Phys. Rev. D , vol. 77, no. 6, p. 065024, Mar. 2008
2008
Cited alongside, same era.
E. Endeve, C. Y. Cardall, R. D. Budiardja, A. Mezzacappa, and J. M. Blondin, “Turbulence and magnetic field amplification from spiral SASI modes in core-collapse supernovae,” Physica Scripta Volume T , vol. 155, no. 1, p. 014022, Jul. 2013
2013
Later among the works it cites.
J. P. Kneller and A. W. Mauney, “Does the finite size of the proto-neutron star preclude supernova neutrino flavor scintillation due to turbulence?” Phys. Rev. D. , vol. 88, no. 4, p. 045020, Aug. 2013
2013
Later among the works it cites.
——, “Consequences of large θ 13 \theta_{13} for the turbulence signatures in supernova neutrinos,” Phys. Rev. D , vol. 88, no. 2, p. 025004, Jul. 2013
2013
Later among the works it cites.
T. Lund and J. P. Kneller, “Combining collective, MSW, and turbulence effects in supernova neutrino flavor evolution,” Phys. Rev. D , vol. 88, no. 2, p. 023008, Jul. 2013
2013
Later among the works it cites.
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…
A. B. Balantekin, J. Gava, and C. Volpe, “Possible CP-violation effects in core-collapse supernovae,” Physics Letters B , vol. 662, pp. 396–404, May 2008
2008
Cited alongside, same era.
J. Gava and C. Volpe, “Collective neutrino oscillations in matter and CP violation,” Phys. Rev. D , vol. 78, no. 8, p. 083007, Oct. 2008
2008
Cited alongside, same era.
J. P. Kneller and G. C. McLaughlin, “Three flavor neutrino oscillations in matter: Flavor diagonal potentials, the adiabatic basis, and the CP phase,” Phys. Rev. D , vol. 80, no. 5, pp. 053 002–+, Sep. 2009
2009
Cited alongside, same era.
J. Kneller and C. Volpe, “Turbulence effects on supernova neutrinos,” Phys. Rev. D , vol. 82, no. 12, pp. 123 004–+, Dec. 2010
2010
Cited alongside, same era.
T. Fischer, S. C. Whitehouse, A. Mezzacappa, F.-K. Thielemann, and M. Liebendörfer, “Protoneutron star evolution and the neutrino-driven wind in general relativistic neutrino radiation hydrodynamics simulations,” Astron. and Astrophys. , vol. 517, p. A80, Jul. 2010
2010
Cited alongside, same era.
J. W. Murphy and C. Meakin, “A Global Turbulence Model for Neutrino-driven Convection in Core-collapse Supernovae,” ApJ. , vol. 742, p. 74, Dec. 2011
2011
Cited alongside, same era.
G. Reid, J. Adams, and S. Seunarine, “Collective neutrino oscillations in turbulent backgrounds,” Phys. Rev. D , vol. 84, no. 8, p. 085023, Oct. 2011
2011
Cited alongside, same era.
S. Chakraborty, T. Fischer, A. Mirizzi, N. Saviano, and R. Tomàs, “No Collective Neutrino Flavor Conversions during the Supernova Accretion Phase,” Physical Review Letters , vol. 107, no. 15, p. 151101, Oct. 2011
2011
Cited alongside, same era.
J. P. Kneller, G. C. McLaughlin, and K. M. Patton, “Stimulated Neutrino Transformation in Supernovae,” J. Phys. , vol. G40, p. 055002, 2013
2013
Later among the works it cites.
S. M. Couch and E. P. O’Connor, “High-resolution Three-dimensional Simulations of Core-collapse Supernovae in Multiple Progenitors,” Astrophys. J. , vol. 785, p. 123, Apr. 2014
2014
Later among the works it cites.
T. Handy, T. Plewa, and A. Odrzywołek, “Toward Connecting Core-collapse Supernova Theory with Observations. I. Shock Revival in a 15 M ⊙
2014
Later among the works it cites.
K. M. Patton, J. P. Kneller, and G. C. McLaughlin, “Stimulated Neutrino Transformation Through Turbulence,” Phys. Rev. , vol. D89, no. 7, p. 073022, 2014
2014
Later among the works it cites.
E. Abdikamalov, C. D. Ott, D. Radice, L. F. Roberts, R. Haas, C. Reisswig, P. Mösta, H. Klion, and E. Schnetter, “Neutrino-driven Turbulent Convection and Standing Accretion Shock Instability in Three-dimensional Core-collapse Supernovae,” Astrophys. J. , vol. 808, p. 70, Jul. 2015
2015
Later among the works it cites.
S. M. Couch and C. D. Ott, “The Role of Turbulence in Neutrino-driven Core-collapse Supernova Explosions,” Astrophys. J. , vol. 799, p. 5, Jan. 2015
2015
Later among the works it cites.
G. G. Katul, C. Manes, A. Porporato, E. Bou-Zeid, and M. Chamecki, “Bottlenecks in turbulent kinetic energy spectra predicted from structure function inflections using the Von Kármán-Howarth equation,” Phys. Rev. E , vol. 92, no. 3, p. 033009, Sep. 2015
2015
Later among the works it cites.
J. P. Kneller and N. V. Kabadi, “Sensitivity of neutrinos to the supernova turbulence power spectrum: Point source statistics,” Phys. Rev. D , vol. 92, no. 1, p. 013009, Jul. 2015
2015
Later among the works it cites.
——, “Stimulated neutrino transformation through turbulence on a changing density profile and application to supernovae,” Phys. Rev. , vol. D91, no. 2, p. 025001, 2015
2015
Later among the works it cites.
B. Müller, “The dynamics of neutrino-driven supernova explosions after shock revival in 2D and 3D,” MNRAS , vol. 453, pp. 287–310, Oct. 2015
2015
Later among the works it cites.
Y. Yang, J. P. Kneller, and K. M. Perkins, “Stimulated transitions due to arbitrary, Fourier decomposed, perturbing Hamiltonians,” ArXiv e-prints , Oct. 2015
2015
Later among the works it cites.
M. R. Drout, D. Milisavljevic, J. Parrent, R. Margutti, A. Kamble, A. M. Soderberg, P. Challis, R. Chornock, W. Fong, S. Frank, N. Gehrels, M. L. Graham, E. Hsiao, K. Itagaki, M. Kasliwal, R. P. Kirshner, D. Macomb, G. H. Marion, J. Norris, and M. M. Phillips, “The Double-peaked SN 2013ge: A Type Ib/c SN with an Asymmetric Mass Ejection or an Extended Progenitor Envelope,” Astrophys. J. , vol. 821, p. 57, Apr. 2016
2016
Later among the works it cites.
D. Radice, C. D. Ott, E. Abdikamalov, S. M. Couch, R. Haas, and E. Schnetter, “Neutrino-driven Convection in Core-collapse Supernovae: High-resolution Simulations,” Astrophys. J. , vol. 820, p. 76, Mar. 2016
2016
Later among the works it cites.
S. W. Bruenn, E. J. Lentz, W. R. Hix, A. Mezzacappa, J. A. Harris, O. E. B. Messer, E. Endeve, J. M. Blondin, M. A. Chertkow, E. J. Lingerfelt, P. Marronetti, and K. N. Yakunin, “The Development of Explosions in Axisymmetric Ab Initio Core-collapse Supernova Simulations of 12-25 M Stars,” Astrophys. J. , vol. 818, p. 123, Feb. 2016
2016
Later among the works it cites.
C. Patrignani et al. , “Review of Particle Physics,” Chin. Phys. , vol. C40, no. 10, p. 100001, 2016
2016
Later among the works it cites.