@article{malkus_mclaughlin_surman_2016, title={Symmetric and standard matter neutrino resonances above merging compact objects}, volume={93}, ISSN={["2470-0029"]}, DOI={10.1103/physrevd.93.045021}, abstractNote={Matter-neutrino resonances (MNR) can occur in environments where the flux of electron antineutrinos is greater than the flux of electron neutrinos. These resonances may result in dramatic neutrino flavor transformation. Compact object merger disks are an example of an environment where electron antineutrinos outnumber neutrinos. We study MNR resonances in several such disk configurations and find two qualitatively different types of matter-neutrino resonances: a standard MNR and a symmetric MNR. We examine the transformation that occurs in each type of resonance and explore the consequences for nucleosynthesis.}, number={4}, journal={PHYSICAL REVIEW D}, author={Malkus, A. and McLaughlin, G. C. and Surman, R.}, year={2016}, month={Feb} }
 @article{malkus_kneller_mclaughlin_surman_2015, title={Neutrino Oscillation Above a Black Hole Accretion Disk}, volume={1663}, ISSN={["0094-243X"]}, url={http://www.scopus.com/inward/record.url?eid=2-s2.0-85006201488&partnerID=MN8TOARS}, DOI={10.1063/1.4919479}, abstractNote={We examine neutrino oscillations in the context of an accretion disk surrounding a black hole. Because accretion disks produce large quantities of neutrinos, they may be home to interesting neutrino oscillation as well. We model accretion disks associated with stellar collapse for the sake of understanding neutrino oscillations. We find that the neutrino oscillations include phenomena seen in the protoneutron star setting as well as phenomena not seen elsewhere.}, journal={NUINT12: 8TH INTERNATIONAL WORKSHOP ON NEUTRINO-NUCLEUS INTERACTIONS IN THE FEW-GEV REGION}, author={Malkus, A. and Kneller, J. P. and McLaughlin, G. C. and Surman, R.}, year={2015} }
 @article{caballero_malkus_mclaughlin_surman_2014, title={The influence of neutrinos on the nucleosynthesis of accretion disc outflows}, volume={41}, ISSN={["1361-6471"]}, DOI={10.1088/0954-3899/41/4/044004}, abstractNote={We present a short review of recent progress on the influence of neutrinos on the nucleosynthesis from black hole accretion disc outflows. Discs that form from the end of life of rapidly rotating massive stars as well as discs that form from mergers will produce large numbers of neutrinos. These neutrinos influence the nucleosynthesis that occurs in hot accretion disc outflows. A variety of nucleosynthesis products can be produced in these outflows. We review work on nickel, p-process and r-process elements.}, number={4}, journal={JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS}, author={Caballero, O. L. and Malkus, A. C. and McLaughlin, G. C. and Surman, R. A.}, year={2014}, month={Apr} }
 @article{malkus_kneller_mclaughlin_surman_2013, title={vs and nucleosynthesis from accretion disks}, volume={1560}, ISSN={["0094-243X"]}, url={http://www.scopus.com/inward/record.url?eid=2-s2.0-84890021433&partnerID=MN8TOARS}, DOI={10.1063/1.4826787}, abstractNote={Black hole accretion disks may occur in certain core collapse supernovae or in mergers of compact objects. This environment produces a strong flux of electron neutrinos and electron antineutrinos. These neutrinos are instrumental in determining the types of elements produced in disk outflows. In this context, using the single angle approximation and a constant temperature disk, we report on calculations of neutrino flavor oscillations driven by neutrino self interactions. We comment on some impacts to element synthesis.}, journal={11TH CONFERENCE ON THE INTERSECTIONS OF PARTICLE AND NUCLEAR PHYSICS (CIPANP 2012)}, author={Malkus, A. and Kneller, J. P. and McLaughlin, G. C. and Surman, R.}, year={2013}, pages={336–340} }
 @article{malkus_kneller_mclaughlin_surman_2012, title={Neutrino oscillations above black hole accretion disks: Disks with electron-flavor emission}, volume={86}, ISSN={["1550-2368"]}, url={http://www.scopus.com/inward/record.url?eid=2-s2.0-84867260598&partnerID=MN8TOARS}, DOI={10.1103/physrevd.86.085015}, abstractNote={Department of Physics and Astronomy, Union College, Schenectady, NY 12308 USA(Dated: December 22, 2013)Black hole accretion disks can form through the collapse of rotating massive stars. These disksproduce large numbers of neutrinos and antineutrinos of electron flavor that can influence energeticsand nucleosynthesis. Neutrinos are produced in sufficient numbers that, after they are emitted, theycan undergo flavor transformation facilitated by the neutrino self interaction. We show that someof the neutrino flavor transformation phenomenology for accretion disks is similar to that of thesupernova case, but also, we find the disk geometry lends itself to different transformation behaviors.These transformations strongly influence the nucleosynthetic outcome of disk winds.}, number={8}, journal={PHYSICAL REVIEW D}, publisher={American Physical Society (APS)}, author={Malkus, A. and Kneller, J. P. and McLaughlin, G. C. and Surman, R.}, year={2012}, month={Oct} }