Multimessenger asteroseismology of core-collapse supernovae

Westernacher-Schneider, John Ryan; O’Connor, Evan; O’Sullivan, Erin; Tamborra, Irene; Wu, Meng-Ru; Couch, Sean M.; Malmenbeck, Felix

doi:10.1103/physrevd.100.123009

Title: Multimessenger asteroseismology of core-collapse supernovae

Journal Article · Wed Dec 11 00:00:00 EST 2019 · Physical Review. D.

DOI:https://doi.org/10.1103/physrevd.100.123009· OSTI ID:1802775

^[1];

^[2]; O’Sullivan, Erin ^[2];

^[3];

^[4];

^[5]; Malmenbeck, Felix ^[6]

Univ. of Arizona, Tucson, AZ (United States); Univ. of Guelph, ON (Canada); Perimeter Inst. for Theoretical Physics, Waterloo, ON (Canada); Univ. of Copenhagen (Denmark)
Stockholm Univ. (Sweden)
Univ. of Copenhagen (Denmark)
Academia Sinica, Taipei (Taiwan); Univ. of Copenhagen (Denmark)
Michigan State Univ., East Lansing, MI (United States)
KTH Royal Inst. of Technology, Stockholm (Sweden)

In this work we investigate correlated gravitational wave and neutrino signals from rotating core-collapse supernovae with simulations. Using an improved mode identification procedure based on mode function matching, we show that a linear quadrupolar mode of the core produces a dual imprint on gravitational waves and neutrinos in the early post-bounce phase of the supernova. The angular harmonics of the neutrino emission are consistent with the mode energy around the neutrinospheres, which points to a mechanism for the imprint on neutrinos. Thus, neutrinos carry information about the mode amplitude in the outer region of the core, whereas gravitational waves probe deeper in. We also find that the best-fit mode function has a frequency bounded above by ~420 Hz , and yet the mode’s frequency in our simulations is ~15 % higher, due to the use of Newtonian hydrodynamics and a widely used pseudo-Newtonian gravity approximation. This overestimation is particularly important for the analysis of gravitational wave detectability and asteroseismology, pointing to limitations of pseudo-Newtonian approaches for these purposes, possibly even resulting in excitation of incorrect modes. In addition, mode frequency matching (as opposed to mode function matching) could be resulting in mode misidentification in recent work. Lastly, we evaluate the prospects of a multimessenger detection of the mode using current technology. The detection of the imprint on neutrinos is most challenging, with a maximum detection distance of ~ 1 kpc using the IceCube Neutrino Observatory. The maximum distance for detecting the complementary gravitational wave imprint is ~ 5 kpc using Advanced LIGO at design sensitivity.

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Research Organization:: Michigan State Univ., East Lansing, MI (United States)

Sponsoring Organization:: Kavli Foundation; Danish National Research Foundation (DNRF); Swedish Research Council (VR); Villum Foundation; Knud Højgaard Foundation; German Research Foundation (DFG); Taiwan Ministry of Science and Technology (MOST); USDOE Office of Science (SC), Nuclear Physics (NP)

Grant/Contract Number:: SC0015904; SC0017955; 107-2119-M-001-038

OSTI ID:: 1802775

Journal Information:: Physical Review. D., Vol. 100, Issue 12; ISSN 2470-0010

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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