<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Mengke Li</title><link>https://mengkel.github.io/</link><description>Recent content on Mengke Li</description><generator>Hugo</generator><language>en</language><lastBuildDate>Wed, 30 Sep 2026 00:00:00 +0000</lastBuildDate><atom:link href="https://mengkel.github.io/index.xml" rel="self" type="application/rss+xml"/><item><title>Publications</title><link>https://mengkel.github.io/publications/</link><pubDate>Wed, 30 Sep 2026 00:00:00 +0000</pubDate><guid>https://mengkel.github.io/publications/</guid><description>&lt;!-- *For a full list, please also see my [Google Scholar](https://scholar.google.com/citations?user=sRYmqRwAAAAJ&amp;hl=en) or [ORCID](https://orcid.org/0000-0002-6373-7494) profile.* --&gt;&#10;&lt;hr&gt;&#10;&lt;h2 id="submitted" class="relative group"&gt;Submitted &lt;span class="absolute top-0 w-6 transition-opacity opacity-0 -start-6 not-prose group-hover:opacity-100"&gt;&lt;a class="group-hover:text-primary-300 dark:group-hover:text-neutral-700" style="text-decoration-line: none !important;" href="#submitted" aria-label="Anchor"&gt;#&lt;/a&gt;&lt;/span&gt;&lt;/h2&gt;&lt;!-- reversed so newer=1 at top, older=2 at bottom --&gt;&#10;&lt;ol reversed&gt;&#10;&lt;li&gt;&lt;strong&gt;&lt;a href="https://arxiv.org/html/2609.30408v1"&gt;Machine Learning β-decay Half-Life and Their Application to r-Process Observables&lt;/a&gt;&lt;/strong&gt;&lt;br&gt;&#10;M. Li, M. Mumpower, N. Vassh, R. Surman. &lt;em&gt;(submitted to The Astrophysical Journal, 2026)&lt;/em&gt;&lt;/li&gt;&#10;&lt;/ol&gt;&#10;&lt;hr&gt;&#10;&lt;h2 id="published" class="relative group"&gt;Published &lt;span class="absolute top-0 w-6 transition-opacity opacity-0 -start-6 not-prose group-hover:opacity-100"&gt;&lt;a class="group-hover:text-primary-300 dark:group-hover:text-neutral-700" style="text-decoration-line: none !important;" href="#published" aria-label="Anchor"&gt;#&lt;/a&gt;&lt;/span&gt;&lt;/h2&gt;&lt;!-- reversed counts down so newest=8 at top, oldest=1 at bottom --&gt;&#10;&lt;ol reversed&gt;&#10;&lt;li&gt;&lt;strong&gt;&#10;&lt;a href="https://iopscience.iop.org/article/10.3847/1538-4357/aea157"&gt;&#10;Neutron Economy in Late Time r-process Nucleosynthesis&lt;/a&gt;&lt;/strong&gt;&lt;br&gt;&#10;M. Li, B. Meyer.&lt;br&gt;&#10;&lt;em&gt;The Astrophysical Journal&lt;/em&gt; (2026)&lt;/li&gt;&#10;&lt;li&gt;&lt;strong&gt;&lt;a href="https://www.sciencedirect.com/science/article/pii/S0370269325008664"&gt;Implications of a Weakening N = 126 Shell Closure Away from Stability for r-Process Astrophysical Conditions&lt;/a&gt; &lt;/strong&gt;&lt;br&gt;&#10;M. Li, G. C. McLaughlin, R. Surman.&lt;br&gt;&#10;&lt;em&gt;Physics Letters B &lt;/em&gt;(2026)&lt;/li&gt;&#10;&lt;li&gt;&lt;strong&gt;&lt;a href="https://journals.aps.org/prresearch/abstract/10.1103/3x9p-64w7"&gt;&#10;Constraining Nuclear Mass Models Using r-Process Observables with Multi-objective Optimization&#10;&lt;/a&gt; &lt;/strong&gt;&lt;br&gt;&#10;M. Li, M. R. Mumpower, N. Vassh, W. S. Porter, R. Surman.&lt;br&gt;&#10;&lt;em&gt;Physical Review Research Letters &lt;/em&gt;(2025)&lt;/li&gt;&#10;&lt;li&gt;&lt;strong&gt;&#10;&lt;a href="https://iopscience.iop.org/article/10.3847/1538-4357/adb625/meta"&gt;&#10;Graph-based Recursive Relations for Computing and Analyzing r-Process Abundances&lt;/a&gt;&lt;/strong&gt;&lt;br&gt;&#10;M. Li, B. S. Meyer.&lt;br&gt;&#10;&lt;em&gt;The Astrophysical Journal&lt;/em&gt; (2025)&lt;/li&gt;&#10;&lt;li&gt;&lt;strong&gt;&#10;&lt;a href="https://journals.aps.org/prc/abstract/10.1103/PhysRevC.110.034321"&gt;&#10;Investigating the Effects of Precise Mass Measurements of Ru and Pd Isotopes on Machine Learning Mass Modeling&lt;/a&gt;&lt;/strong&gt;&lt;br&gt;&#10;W. S. Porter, B. Liu, D. Ray, A. A. Valverde, M. Li, M. R. Mumpower, et al.&lt;br&gt;&#10;&lt;em&gt;Physical Review C&lt;/em&gt; (2024)&lt;/li&gt;&#10;&lt;li&gt;&lt;strong&gt;&#10;&lt;a href="https://www.sciencedirect.com/science/article/pii/S0370269323007190"&gt;&#10;Atomic Masses with Machine Learning for the Astrophysical r-Process&#10;&lt;/a&gt;&lt;/strong&gt;&lt;br&gt;&#10;M. Li, T. M. Sprouse, B. S. Meyer, M. R. Mumpower.&lt;br&gt;&#10;&lt;em&gt;Physics Letters B&lt;/em&gt; (2024)&lt;/li&gt;&#10;&lt;li&gt;&lt;strong&gt;&#10;&lt;a href="https://www.frontiersin.org/journals/physics/articles/10.3389/fphy.2023.1198572/full"&gt; &#10;Bayesian Averaging for Ground State Masses of Atomic Nuclei in a Machine Learning Approach&lt;/a&gt;&lt;/strong&gt;&lt;br&gt;&#10;M. R. Mumpower, M. Li, T. M. Sprouse, B. S. Meyer, A. E. Lovell, A. Mohan.&lt;br&gt;&#10;&lt;em&gt;Frontiers in Physics&lt;/em&gt; (2023)&lt;/li&gt;&#10;&lt;li&gt;&lt;strong&gt;&#10;&lt;a href="https://link.aps.org/doi/10.1103/PhysRevC.106.035803"&gt;&#10;Dependence of (n,γ)–(γ,n) Equilibrium r-Process Abundances on Nuclear Physics&lt;/a&gt;&lt;/strong&gt;&lt;br&gt;&#10;M. Li, B. S. Meyer.&lt;br&gt;&#10;&lt;em&gt;Physical Review C&lt;/em&gt; (2022)&lt;/li&gt;&#10;&lt;/ol&gt;</description></item><item><title>Research</title><link>https://mengkel.github.io/research/</link><pubDate>Wed, 30 Sep 2026 00:00:00 +0000</pubDate><guid>https://mengkel.github.io/research/</guid><description>&lt;h2 id="research-overview" class="relative group"&gt;Research Overview &lt;span class="absolute top-0 w-6 transition-opacity opacity-0 -start-6 not-prose group-hover:opacity-100"&gt;&lt;a class="group-hover:text-primary-300 dark:group-hover:text-neutral-700" style="text-decoration-line: none !important;" href="#research-overview" aria-label="Anchor"&gt;#&lt;/a&gt;&lt;/span&gt;&lt;/h2&gt;&lt;p&gt;My research is in &lt;strong&gt;theoretical nuclear astrophysics&lt;/strong&gt;, with a focus on understanding the origins of heavy elements in the universe through nucleosynthesis processes occurring in extreme astrophysical environments such as neutron star mergers and core-collapse supernovae.&lt;/p&gt;&#10;&lt;p&gt;I combine nuclear theory, astrophysical simulations, and machine learning to connect properties of exotic nuclei with observable r-process signatures. My work uses nuclear mass models, beta-decay and reaction-rate calculations, reaction-network modeling, and data-driven methods to understand how nuclear uncertainties shape the elemental abundances observed in the Solar System and in metal-poor stars.&lt;/p&gt;</description></item><item><title>About</title><link>https://mengkel.github.io/about/</link><pubDate>Mon, 01 Jan 2024 00:00:00 +0000</pubDate><guid>https://mengkel.github.io/about/</guid><description>&lt;p&gt;Welcome! I am an &lt;a href="https://n3as.berkeley.edu/" target="_blank" rel="noreferrer"&gt;N3AS&lt;/a&gt; Postdoc Fellow working on &lt;strong&gt;theoretical nuclear astrophysics&lt;/strong&gt; at UC Berkeley. My research sits at the intersection of astrophysics, nuclear physics, and machine learning, exploring how exotic nuclear properties shape cosmic phenomena like &lt;em&gt;r&lt;/em&gt;-process nucleosynthesis and kilonova.&lt;/p&gt;&#10;&lt;p&gt;I received my PhD from Clemson University in December 2023, under the supervision of Prof. &lt;a href="https://www.clemson.edu/science/academics/departments/physics/about/profiles/mbradle" target="_blank" rel="noreferrer"&gt;Bradley Meyer&lt;/a&gt;. As a Postdoc Fellow, I am co-mentored by &lt;a href="https://physics.nd.edu/people/rebecca-surman/" target="_blank" rel="noreferrer"&gt;Rebecca Surman&lt;/a&gt; (University of Notre Dame), &lt;a href="https://physics.sciences.ncsu.edu/people/gcmclaug/" target="_blank" rel="noreferrer"&gt;Gail McLaughlin&lt;/a&gt; (NC State University) and &lt;a href="https://physics.berkeley.edu/people/faculty/dan-kasen" target="_blank" rel="noreferrer"&gt;Dan Kasen&lt;/a&gt; (UC Berkeley).&lt;/p&gt;</description></item><item><title>Mentorship</title><link>https://mengkel.github.io/teaching/</link><pubDate>Mon, 01 Jan 2024 00:00:00 +0000</pubDate><guid>https://mengkel.github.io/teaching/</guid><description>&lt;h2 id="mentoring" class="relative group"&gt;Mentoring &lt;span class="absolute top-0 w-6 transition-opacity opacity-0 -start-6 not-prose group-hover:opacity-100"&gt;&lt;a class="group-hover:text-primary-300 dark:group-hover:text-neutral-700" style="text-decoration-line: none !important;" href="#mentoring" aria-label="Anchor"&gt;#&lt;/a&gt;&lt;/span&gt;&lt;/h2&gt;&lt;ul&gt;&#10;&lt;li&gt;&lt;strong&gt;2025&lt;/strong&gt; — Research mentor for UC Berkeley undergraduate student Flora Wang&lt;/li&gt;&#10;&lt;li&gt;&lt;strong&gt;2024&lt;/strong&gt; — Career mentor for UC Berkeley undergraduate student Claire T. Chen&lt;/li&gt;&#10;&lt;/ul&gt;&#10;&lt;h2 id="teaching-experience" class="relative group"&gt;Teaching Experience &lt;span class="absolute top-0 w-6 transition-opacity opacity-0 -start-6 not-prose group-hover:opacity-100"&gt;&lt;a class="group-hover:text-primary-300 dark:group-hover:text-neutral-700" style="text-decoration-line: none !important;" href="#teaching-experience" aria-label="Anchor"&gt;#&lt;/a&gt;&lt;/span&gt;&lt;/h2&gt;&lt;ul&gt;&#10;&lt;li&gt;&#10;&lt;p&gt;&lt;strong&gt;Graduate Teacher of Record (Course Leader)&lt;/strong&gt; — Clemson University &lt;em&gt;(2022–2023)&lt;/em&gt;&lt;/p&gt;&#10;&lt;ul&gt;&#10;&lt;li&gt;Designed experimental laboratory modules and updated course curriculum.&lt;/li&gt;&#10;&lt;li&gt;Managed digital course materials, assignments, and gradebooks via Canvas LMS.&lt;/li&gt;&#10;&lt;li&gt;Coordinated grading criteria and course assessments to track learning outcomes.&lt;/li&gt;&#10;&lt;/ul&gt;&#10;&lt;/li&gt;&#10;&lt;li&gt;&#10;&lt;p&gt;&lt;strong&gt;Graduate Teaching Assistant&lt;/strong&gt; — Clemson University &lt;em&gt;(2018–2021)&lt;/em&gt;&lt;/p&gt;&#10;&lt;ul&gt;&#10;&lt;li&gt;Instructed introductory and intermediate physics lab sections (PHYS 2070, 2090, 2100, 2300).&lt;/li&gt;&#10;&lt;li&gt;Mentored students in experimental techniques, data reduction, and scientific writing.&lt;/li&gt;&#10;&lt;li&gt;Graded lab reports and assessments while providing detailed, constructive feedback.&lt;/li&gt;&#10;&lt;/ul&gt;&#10;&lt;/li&gt;&#10;&lt;/ul&gt;</description></item></channel></rss>