Publications by group members


[42] G. Guo, Y.-Z. Qian, M.-R. Wu, under review, [arXiv:2310.05137], "Effects of Annihilation with Low-Energy Neutrinos on High-Energy Neutrinos from Binary Neutron Star Mergers and Rare Core-Collapse Supernovae".
[41] T. Fischer, G. Guo, K. Langanke, G. Martinez-Pinedo, Y.-Z. Qian, M.-R. Wu, under review, [arXiv:2308.03962], "Neutrinos and nucleosynthesis of elements".
[40] Z. Xiong, M.-R. Wu, S. Abbar, et., al., Phys.Rev.D 108 (2023) 6, 063003, [arXiv:2307.11129], "Evaluating approximate asymptotic distributions for fast neutrino flavor conversions in a periodic 1D box".
[42] Y.-H. Lin, T.-H. Tsai, G.-L. Lin, et., al., Phys.Rev.D 108 (2023) 8, 083013, [arXiv:2307.03522], "Signatures of afterglows from light dark matter boosted by supernova neutrinos in current and future large underground detectors".
[41] Y. An, M.-R. Wu, G. Guo, et., al., under review, [arXiv:2306.07659], "R-process beta-decay neutrino flux from binary neutron star merger and collapsar".
[40] Z. Xiong, M.-R. Wu, Y.-Z. Qian, Phys.Rev.D 108 (2023) 4, 043007, [arXiv:2303.05906], "Symmetry and bipolar motion in collective neutrino flavor oscillations".


[39] G. Guo, Y.-Z. Qian, M.-R. Wu, Phys.Rev.D 108 (2023) 2, L021303, [arXiv:2212.08266], "Signature of Collapsars as Sources for High-energy Neutrinos and r-process Nuclei".
[38] Z. Xiong, L. Johns, M.-R. Wu, H. Duan, Phys.Rev.D 108 (2023) 8, 083002, [arXiv:2212.03750], "Collisional flavor instability in dense neutrino gases".
[37] Z. Xiong, M.-R. Wu, G. Martinez-Pinedo et. al., Phys.Rev.D 107 (2023) 8, 083016, [arXiv:2210.08254], "Evolution of collisional neutrino flavor instabilities in spherically symmetric supernova models".
[36] G. SigurĂ°arson, I. Tamborra, M.-R. Wu, Phys.Rev.D 106 (2022) 12, 123030, [arXiv:2209.07544], "Resonant Production of Light Sterile Neutrinos in Compact Binary Merger Remnants".
[35] Y.-H. Lin, W.-H. Wu, M.-R. Wu, H. T.-K. Wong, Phys.Rev.Lett. 130 (2023) 11, 111002, [arXiv:2206.06864], "Searching for Afterglow: Light Dark Matter boosted by Supernova Neutrinos".
[34] M.-R. Wu, P. Banerjee, AAPPS Bull. 32 (2022) 1, 19, [arXiv:2205.11806], "The Production of Actinides in Neutron Star Mergers".
[33] S. Richers, H. Duan, M.-R. Wu, et. al., PRD 106 (2022) 4, 043011, [arXiv:2205.06282], "Code comparison for fast flavor instability simulations".
[32] J. Carter et al (including H. Wibowo), PLB 833 (2022) 137374, [arXiv:2204.12170], "Damping of the isovector giant dipole resonance in 40,48Ca".
[31] O. Just, S. Abbar, M.-R. Wu, et. al., PRD 105 (2022) 8, 083024, [arXiv:2203.16559], "Fast neutrino conversion in hydrodynamic simulations of neutrino-cooled accretion disks".
[30] M. Q. Hlatshwayo, Y. Zhang, H. Wibowo, et. al., PRC 106 (2022) 2, 024319, [arXiv:2203.01478], "Simulating excited states of the Lipkin model on a quantum computer".
[29] M. George, C.-Y. Lin, M.-R. Wu, T. G. Liu, Z. Xiong, CPC 283 (2023) 108588, [arXiv:2203.012866], "COSEν: A Collective Oscillation Simulation Engine for Neutrinos".


[28] H. Wibowo, E. Litvinova, Phys.Rev.C 106 (2022) 4, 044304, [arXiv:2110.05749], "Nuclear Shell Structure in a Finite-Temperature Relativistic Framework".
[27] P. Banerjee, M.-R. Wu, Jeena S. K, MNRAS 512 (2022) 4, 4948, [arXiv:2110.05449], "Constraints on R-process Nucleosynthesis from 129I and 247Cm in the Early Solar System".
[26] M.-R. Wu, M. George, C.-Y. Lin, Z. Xiong, PRD 104 (2021) 10, 103003 ,[arXiv:2108.09886], "Collective fast neutrino flavor conversions in an 1D box: (I) initial condition and long-term evolution".
[25] A. A. Aziz et al (including M.-R. Wu), AAPPS Bull. 31 (2021) 1, 18, [arXiv:2108.03814], "Progress in nuclear astrophysics of east and southeast Asia".
[24] Y.-H. Lin, G.-L. Lin, PRD 104 (2021) 6, 063021, [arXiv:2102.11151], "Exploring dark sector parameters in light of neutron star temperatures".
[23] A. Sung, G. Guo, M.-R. Wu, PRD 103 (2021) 10, 103005, [arXiv:2102.04601], "Supernova Constraint on Self-Interacting Dark Sector Particles".


[22] A. Bauswein, G. Guo, J.-H. Lien, Y.-H. Lin, M.-R. Wu, Phys.Rev.D 107 (2023) 8, 083002 [arXiv:2012.11908], "Compact Dark Objects in Neutron Star Mergers".
[21] M. George, M.-R. Wu, I. Tamborra, et. al., PRD 102 (2020) 10, 103015 [arXiv:2009.04046], "Fast neutrino flavor conversion, ejecta properties, and nucleosynthesis in newly-formed hypermassive remnants of neutron-star mergers".
[20] T. Fischer, G. Guo, G. Martinez-Pinedo, et. al., PRD 102 (2020) 10, 100304, [arXiv:2008.13628], "Muonization of supernova matter".
[19] G. Guo, Y.-L. S. Tsai, M.-R. Wu, Qiang Yuan, PRD 102 (2020) 10, 103004, [arXiv:2008.12137], "Elastic and Inelastic Scattering of Cosmic-Rays on Sub-GeV Dark Matter".
[18] P. Banerjee, M.-R. Wu, Z. Yuan, ApJL 902 (2020) 2, L34, [arXiv:2007.04442], "Neutron Star Mergers as the Main Source of R-process: Natal Kicks And Inside-Out Evolution to The Rescue".
[17] G. Guo, G. Martinez-Pinedo, A. Lohs, et. al., Phys.Rev.D 102 (2020) 023037, [arXiv:2006.12051], "Charged-Current Muonic Reactions in Core-Collapse Supernovae".
[16] J. Tang, T.-C. Wang, M.-R. Wu, JCAP 10 (2020) 038, [arXiv:2005.09168], "Constraining sterile neutrinos by core-collapse supernovae with multiple detectors".
[15] A. M. Suliga, I. Tamborra, M.-R. Wu, JCAP 08 (2020) 018, [arXiv:2004.11389], "Lifting the core-collapse supernova bounds on keV-mass sterile neutrinos".
[14] G.-L. Lin and Y.-H. Lin, JCAP 08 (2020) 022, [arXiv:2004.05312], "Analysis on the black hole formations inside old neutron stars by isospin-violating dark matter with self-interaction".
[13] G. Guo, Y.-L. S. Tsai, M.-R. Wu, JCAP 10 (2020) 049, [arXiv:2004.03161], "Probing High-Energy Light Dark Matter with IceCube".
[12] T. Fischer, M.-R. Wu, B. Wehmeyer, et. al., Astrophys.J. 894 (2020) 9, [arXiv:2003.00972], "Core-collapse Supernova Explosions Driven by the Hadron-quark Phase Transition as a Rare r-process Site".


[11] G. Guo, Y.-Z. Qian, M.-R. Wu, Astrophys.J 890 (2020) 83, [arXiv:1911.07568], "Potential Connection Between IceCube Neutrinos and Late Bumps in Gamma-Ray Bursts".
[10] A. M. Suliga, I. Tamborra, M.-R. Wu, JCAP 1912 (2019) 019, [arXiv:1908.11382], "Tau lepton asymmetry by sterile neutrino emission -- Moving beyond one-zone supernova models".
[9] J. R. Westernacher-Schneider, E. O'Connor, E. O'Sullivan, et. al. (including M.-R. Wu), Phys. Rev. D 100 (2019) 12, [arXiv:1907.01138], "Multimessenger Asteroseismology of Core-Collapse Supernovae".
[8] M.-R. Wu, P. Banerjee, B. D. Metzger, et. al., Astrophys.J 880 (2019) 23, [arXiv:1905.03793], "Finding the remnants of the Milky Way's last neutron star mergers".
[7] Z. Xiong, M.-R. Wu, Y.-Z. Qian, Astrophys.J 880 (2019) 81, [arXiv:1904.09371], "Active-sterile Neutrino Oscillations in Neutrino-driven Winds: Implications for Nucleosynthesis".
[6] S. A. Giuliani, G. Martinez-Pinedo, M.-R. Wu, L. M. Robledo, PRC 102 (2020) 4, 045804, [arXiv:1904.03733], "Fission and the r-process nucleosynthesis of translead nuclei".
[5] A. Sung, H. Tu, M.-R. Wu, Phys. Rev. D99 (2019) 121305, [arXiv:1903.03793], "New constraint from supernova explosions on light particles beyond the Standard Model".

September 2017 - 2018

[4] M.-R. Wu, J. Barnes, G. Martinez-Pinedo, B. D. Metzger, PRL 122 (2019) 062701, [arXiv:1808.10459], "Fingerprints of heavy element nucleosynthesis in the late-time lightcurves of kilonovae".
[3] T. Fischer, G. Martinez-Pinedo, M.-R. Wu, A. Lohs, Y.-Z. Qian, PRC 101 (2020) 2, [arXiv:1804.10890], "Neutrino signal from proto-neutron star evolution: effects of opacities from charged current neutrino interactions and inverse neutron decay".
[2] T. Fischer, N.-U. F. Bastien, M.-R. Wu, P. Baklanov, E. Sorokina, S. Blinnikov, S. Typel, T. Klaehn, D. B. Blaschke, Nature Astronomy 2, 980 (2018), [arXiv:1712.08788], "Quark deconfinement as a supernova explosion engine for massive blue supergiant stars".
[1] M.-R. Wu, I. Tamborra, O. Just, and H.-T. Janka, Phys. Rev. D96, 123015 (2017), [arXiv:1711.00477], "Imprints of neutrino-pair flavor conversions on nucleosynthesis in ejecta from neutron-star merger remnants".