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Public university governing boards exist to serve the people of their states. It should, therefore, be easy for the public to know what governing bodies are doing. University governance, however, isn't always as transparent as it should be. Often, the public is given little advance notice of when and where meetings will be held and what issues will be discussed. One of the silver linings of the pandemic was an increase in governance transparency. Governing boards began live-streaming meetings that hadn't previously been available for remote viewing. Many meetings, including committee and subcommittee meetings, became publicly available via live stream. Some schools even recorded and posted those meetings for later public viewing online. This was a positive step in transparency because, aside from a global pandemic, members of the public do not always have the ability to physically attend meetings in person. Another positive practice adopted during the pandemic was the policy of conducting votes by roll call. Taking votes by roll call, and later recording those votes in the meeting minutes, ensures accuracy. Unfortunately, as universities transitioned back to meeting in person, some of the gains in transparency have been abandoned. Those practices should be restored and made permanent board policy, along with additional transparency measures.

American colleges and universities are failing at civic education. Too many graduates are ignorant of basic facts about American history and institutions. According to its most recent report on what colleges and universities teach students, the American Council of Trustees and Alumni (ACTA) found that only 214 institutions out of 1,135 (about 19 percent) require a foundational course in U.S. government or history. Even history majors often are not required to study American history. Universities aren't just failing to teach students about their country's history and constitutional structure, many actively propagate distorted and erroneous depictions of American history. Furthermore, these universities have reimagined "civics education" as a form of political activism. An honest grounding in American history and principles will enable students to become knowledgeable, responsible, and engaged citizens. It will allow them to both understand their constitutional rights and respect those of others. And it may awaken in them an appreciation of the freedoms they enjoy and a sense of duty to preserve them.

The ongoing efforts to optimize Li-ion batteries led to the interest in intercalation of nanoscale layered compounds, including bilayer graphene. Its lithium intercalation has been demonstrated recently but the mechanisms underpinning the storage capacity remain poorly understood. Here, using magnetotransport measurements, we report in-operando intercalation dynamics of bilayer graphene. Unexpectedly, we find four distinct intercalation stages that correspond to well-defined Li-ion densities. We refer to these stages as 'in-plane', with no in-plane analogues in bulk graphite. The fully intercalated bilayers represent a stoichiometric compound C14LiC14 with a Li density of 2.7x10^{14} cm^{-2}, notably lower than fully intercalated graphite. Combining the experimental findings and DFT calculations, we show that the critical step in bilayer intercalation is a transition from AB to AA stacking which occurs at a density of 0.9x10^{14} cm^{-2}. Our findings reveal the mechanism and limits for electrochemical intercalation of bilayer graphene and suggest possible avenues for increasing the Li storage capacity., Comment: 30 pages, 17 figures

We report on the thermodynamic and transport properties of the rare-earth Zintl compound Eu$_5$Sn$_2$As$_6$, which orders as a canted antiferromagnetic magnetic semiconductor at 10.3~K. The system also displays a complex cascade of magnetic phases arising from geometric and magnetic exchange frustration, with high sensitivity to the application and direction of small magnetic fields. At low temperature, Eu$_5$Sn$_2$As$_6$ exhibits negative colossal magnetoresistance of up to a factor of $6\times10^3$. This may be a lower bound as the conductivity appears to be shunted by an unknown conduction channel, causing the resistivity to saturate. Mechanisms for the low temperature saturation of resistivity are discussed., Comment: 11 pages, 5 figures in main text, 5 appendices

The study of quantum magnetism in frustrated triangular lattices has promised the discovery of exotic excitations emerging from many-body entanglement, like the quantum spin liquid. This field is vexed by the interplay of disorder, correlations and long-range order, whose properties are challenging to control and disentangle. We study the entropy-carrying excitations of a leading candidate in this search, the material NaYbSe$_2$, as a function of site dilution to directly address this challenge. We map the evolution of the entangled spins across the percolation transition, showing unequivocal evidence for the presence of an energy gap in the excitations of the system. However, we also show that this gap onsets at the percolation transition where disorder is the greatest, strongly suggesting that it is unlikely be associated with a quantum spin liquid. Instead we suggest the more universal scenario of a short-range ordered state with entropy-carrying boundaries., Comment: 7 pages, 3 figures

Noise resilience of quantum information processing is a crucial precondition to reach the fault-tolerance threshold. While resilience to many types of noise can be achieved through suitable control schemes, resilience to amplitude noise seems to be elusive within the common harmonic approximation for the bus mode of trapped ions. We show that weak an-harmonicities admit control schemes that achieve amplitude noise-resilience consistent with state-of-the-art experimental requirements, and that the required an-harmonicities can be achieved with current standards of micro-structured traps or even the intrinsically an-harmonic Coulomb interaction.

In magnetic topological insulators, spontaneous time-reversal symmetry breaking by intrinsic magnetic order can open an energy gap in the topological surface spectrum. In the resulting state, exotic properties like axion electrodynamics, the quantum anomalous Hall effect, and other topological magnetoelectric responses are expected to emerge. A detailed understanding of the magnetic order and its coupling to the topological surface states is essential to harness and tune these properties. Here, we leverage near-resonant electric quadrupole optical second harmonic generation to probe magnetic fluctuations in the candidate axion insulator EuSn$_2$(As,P)$_2$ across its antiferromagnetic phase boundary. We observe a pronounced dimensional crossover in the quantum decoherence induced by magnetic fluctuations, where two-dimensional in-plane ferromagnetic correlations at high temperatures give way to three-dimensional long-range order at the N\'eel temperature. We also observe the breaking of rotational symmetry within the long-range-ordered antiferromagnetic state and map out the resulting spatial domain structure. More generally, we demonstrate the unique capabilities of nonlinear optical spectroscopy to study quantum coherence and fluctuations in magnetic quantum materials.

The transformation of time between the surface of the Earth, the solar system barycenter, and the surface of the Moon involves relativistic corrections. For solar system Barycentric Dynamical Time (TDB), we also require that there be no rate difference between Terrestrial Time (TT) and TDB. The IAU has addressed these transformations with several resolutions. A series of robotic and crewed landings on the Moon are planned. The analogous transformation between TDB and time on the surface of the Moon (TL) needs a review and discussion. In this paper, we compute the rate terms involved in that transformation. We also present the TDB-compatible spatial scale and Lorentz contraction of Moon-centered positional coordinates. These transformations have been implemented in the JPL programs used to generate ephemerides of the Moon and planets. Finally, we provide expressions that can be used to synchronize TT and TL using either TDB or TT. The relevant transformations contain a small secular drift between the two time scales, along with additional small periodic terms that can be numerically evaluated using the solar system and lunar ephemerides., Comment: 15 pages, 3 tables

For linear regression models with cross-section or panel data, it is natural to assume that the disturbances are clustered in two dimensions. However, the finite-sample properties of two-way cluster-robust tests and confidence intervals are often poor. We discuss several ways to improve inference with two-way clustering. Two of these are existing methods for avoiding, or at least ameliorating, the problem of undefined standard errors when a cluster-robust variance matrix estimator (CRVE) is not positive definite. One is a new method that always avoids the problem. More importantly, we propose a family of new two-way CRVEs based on the cluster jackknife. Simulations for models with two-way fixed effects suggest that, in many cases, the cluster-jackknife CRVE combined with our new method yields surprisingly accurate inferences. We provide a simple software package, twowayjack for Stata, that implements our recommended variance estimator.

Correlated materials may exhibit unusually high resistivity increasing linearly in temperature, breaking through the Mott-Ioffe-Regel bound, above which coherent quasiparticles are destroyed. The fate of collective charge excitations, or plasmons, in these systems is a subject of debate. Several studies suggest plasmons are overdamped while others detect unrenormalized plasmons. Here, we present direct optical images of low-loss hyperbolic plasmon polaritons (HPPs) in the correlated van der Waals metal MoOCl2. HPPs are plasmon-photon modes that waveguide through extremely anisotropic media and are remarkably long-lived in MoOCl2. Many-body theory supported by photoemission results reveals that MoOCl2 is in an orbital-selective and highly incoherent Peierls phase. Different orbitals acquire markedly different bonding-antibonding character, producing a highly-anisotropic, isolated Fermi surface. The Fermi surface is further reconstructed and made partly incoherent by electronic interactions, renormalizing the plasma frequency. HPPs remain long-lived in spite of this, allowing us to uncover previously unseen imprints of electronic correlations on plasmonic collective modes., Comment: 32 pages, 16 figures

We study cluster-robust inference for binary response models. Inference based on the most commonly-used cluster-robust variance matrix estimator (CRVE) can be very unreliable. We study several alternatives. Conceptually the simplest of these, but also the most computationally demanding, involves jackknifing at the cluster level. We also propose a linearized version of the cluster-jackknife variance matrix estimator as well as linearized versions of the wild cluster bootstrap. The linearizations are based on empirical scores and are computationally efficient. Throughout we use the logit model as a leading example. We also discuss a new Stata software package called logitjack which implements these procedures. Simulation results strongly favor the new methods, and two empirical examples suggest that it can be important to use them in practice.

Semiconducting transition metal dichalcogenides (MX$_2$) occur in 2H and rhombohedral (3R) polytypes, respectively distinguished by anti-parallel and parallel orientation of consecutive monolayer lattices. In its bulk form, 3R-MX$_2$ is ferroelectric, hosting an out-of-plane electric polarisation, the direction of which is dictated by stacking. Here, we predict that twin boundaries, separating adjacent polarization domains with reversed built-in electric fields, are able to host two-dimensional electrons and holes with an areal density reaching $\sim 10^{13} {\rm cm}^{-2}$. Our modelling suggests that n-doped twin boundaries have a more promising binding energy than p-doped ones, whereas hole accumulation is stable at external surfaces of a twinned film. We also propose that assembling pairs of mono-twin films with a `magic' twist angle $\theta^*$ that provides commensurability between the moir\'e pattern at the interface and the accumulated carrier density, should promote a regime of strongly correlated states of electrons, such as Wigner crystals, and we specify the values of $\theta^*$ for homo- and heterostructures of various TMDs., Comment: 12 pages, 8 Figures

Algorithmic bias is a major issue in machine learning models in educational contexts. However, it has not yet been studied thoroughly in Asian learning contexts, and only limited work has considered algorithmic bias based on regional (sub-national) background. As a step towards addressing this gap, this paper examines the population of 5,986 students at a large university in the Philippines, investigating algorithmic bias based on students' regional background. The university used the Canvas learning management system (LMS) in its online courses across a broad range of domains. Over the period of three semesters, we collected 48.7 million log records of the students' activity in Canvas. We used these logs to train binary classification models that predict student grades from the LMS activity. The best-performing model reached AUC of 0.75 and weighted F1-score of 0.79. Subsequently, we examined the data for bias based on students' region. Evaluation using three metrics: AUC, weighted F1-score, and MADD showed consistent results across all demographic groups. Thus, no unfairness was observed against a particular student group in the grade predictions., Comment: Published in proceedings of the 17th Educational Data Mining Conference (EDM 2024)

Materials that transition between metal and insulator, the two opposing states that distinguish all solids, are fascinating because they underlie many mysteries in the physics of the solid state. In 1T-TaS$_{2}$, the metal-insulator transition is linked to a series of metastable states of a chiral charge density wave whose basic nature is still an open question. In this work, we show that pulses of current through these materials create current-carrying boundary channels that distinguish the metallic and insulating states. We demonstrate electrical control of these channels' properties, suggesting their formation could be due to the complex interplay of the formation of domain walls and the viscous flow of electrons. Our findings show that physical boundaries play a key role in the properties of the metastable states of the metal-insulator transition, highlighting new possibilities for in-situ electrical design and active manipulation of electrical components.

Higher education serves many purposes. One purpose dominates, however: to students, their parents, future employers, government officials, and many academic administrators, higher education is all about preparing students for the professional workforce. Other requirements, such as general education programs, are considered to be of lesser importance. In many cases, they are designed solely to support the primary goal of training professionals, providing generalized skills that can be translated to many professions. Yet treating general education programs as secondary constitutes a great loss of opportunity, as well-designed programs have the potential to help students become better citizens, deeper thinkers, and more moral people. In this report, the author explores actual learning processes at a primary level and shows why a tightly crafted general education that deliberately connects various types of knowledge and learning is vastly superior to one that that allows students wide latitude to choose among unconnected courses that may appear to be interesting at the time but offer little long-term insight. And is also preferable to one that attempts to teach skills without bothering with the content involved. This report should be read--and acted upon--by all policymakers, administrators, and academics who are truly concerned with the quality of education that colleges and universities provide.

The surest measure of a successful college or university is the academic success of its students. True academic success requires incoming students to be academically prepared for college rigor, and is demonstrated by the availability of high-quality academic programs and evidence of personal and professional growth in the years after students' graduation. Institutions that churn out students with low-quality--yet costly--degrees or who set up students for failure by whittling down academic standards, are setting them up for long-term economic and personal hardship. This is why academic transparency is crucial. Academic transparency is truth in advertising. One of the simplest ways to practice academic transparency is to make syllabi publicly accessible by posting them online before registration for classes begins. Doing so serves multiple purposes. Firstly, it allows students to make more informed decisions about what classes they should take. Secondly, the sunlight provided by having their syllabi publicly viewable may encourage professors to cull truly rigorous coursework. Finally, it allows lawmakers to see what kind of education is being offered at taxpayer-supported institutions. This and other academic transparency measures outlined in this report should be standard practice for every public college and university.

Antiferromagnets have attracted significant attention in the field of magnonics, as promising candidates for ultralow-energy carriers for information transfer for future computing. The role of crystalline orientation distribution on magnon transport has received very little attention. In multiferroics such as BiFeO$_3$ the coupling between antiferromagnetic and polar order imposes yet another boundary condition on spin transport. Thus, understanding the fundamentals of spin transport in such systems requires a single domain, a single crystal. We show that through Lanthanum(La) substitution, a single ferroelectric domain can be engineered with a stable, single-variant spin cycloid, controllable by an electric field. The spin transport in such a single domain displays a strong anisotropy, arising from the underlying spin cycloid lattice. Our work shows a pathway to understand the fundamental origins of spin transport in such a single domain multiferroic., Comment: 15 pages, 9 figure

Within the first few hundreds of millions of years, many physical processes sculpt the eventual properties of young planets. NASA's TESS mission has surveyed young stellar associations across the entire sky for transiting planets providing glimpses into the various stages of planetary evolution. Using our own detection pipeline, we search a magnitude-limited sample of 7219 young stars ($\leq$200 Myr) observed in the first four years of TESS for small (2-8 R$_\oplus$), short period (1.6-20 days) transiting planets. The completeness of our survey is characterized by a series of injection and recovery simulations. Our analysis of TESS 2-minute cadence and Full Frame Image (FFI) light curves recover all known TOIs, as well as four new planet candidates not previously identified as TOIs. We derive an occurrence rate of $35^{+13}_{-10}$% for mini-Neptunes and $27^{+10}_{-8}$% for super-Neptunes from the 2-minute cadence data, and $22^{+8.6}_{-6.8}$% for mini-Neptunes and $13^{+3.9}_{-4.9}$% for super-Neptunes from FFI data. To independently validate our results, we compare our survey yield with the predicted planet yield assuming Kepler planet statistics. We consistently find a mild increase in the occurrence of super-Neptunes and a significant increase in the occurrence of Neptune-sized planets with orbital periods of 6.2-12 days when compared to their mature counterparts. The young planet distribution from our study is most consistent with evolution models describing the early contraction of hydrogen-dominated atmospheres undergoing atmospheric escape and inconsistent with heavier atmosphere models offering only mild radial contraction early on., Comment: Accepted to AJ. Updated version after proofing. 24 pages, 13 figures, 3 tables

This work explores the different shapes that can be realized by the one-particle velocity distribution functions (VDFs) associated with the fourth-order maximum-entropy moment method. These distributions take the form of an exponential of a polynomial of the particle velocity, with terms up to the fourth-order. The 14- and 21-moment approximations are investigated. Various non-equilibrium gas states are probed throughout moment space. The resulting maximum-entropy distributions deviate strongly from the equilibrium VDF, and show a number of lobes and branches. The Maxwellian and the anisotropic Gaussian distributions are recovered as special cases. The eigenvalues associated with the maximum-entropy system of transport equations are also illustrated for some selected gas states. Anisotropic and/or asymmetric non-equilibrium states are seen to be associated with a non-uniform spacial propagation of perturbations.

Small, close-in exoplanets are divided into two sub-populations: super-Earths and sub-Neptunes. Most super-Earths are thought to have lost their primordially accreted hydrogen-dominated atmospheres via thermally driven winds. We consider the global chemical equilibrium of super-Earths and the lasting impacts of their fleeting hydrogen atmospheres. We find that hydrogen is efficiently sequestered into the interior, oxidising iron and endogenously producing $\sim0.5-1.0\%$ water by mass. As the atmospheres of super-Earths are continuously sculpted by mass loss and chemical equilibration, they remain hydrogen-dominated by mole (number) fraction but become steam-dominated by mass, which may be observable with JWST for planets transitioning across the radius valley. One of the main effects of efficient sequestration of hydrogen into the interior is to produce an under-dense bulk interior compared to that of Earth. We predict bulk densities of super-Earths to be $\sim 5.0 \text{ g cm}^{-3}$ for a $1M_\oplus$ planet, which is consistent with high-precision mass measurements and also population-level inference analyses from atmospheric escape models., Comment: 16 pages, 4 figures. Accepted for publication in ApJ. Comments welcome

Maximum-entropy moment methods allow for the modelling of gases from the continuum regime to strongly rarefied conditions. The development of approximated solutions to the entropy maximization problem has made these methods computationally affordable. In this work, we apply a fourth-order maximum-entropy moment method to the study of supersonic rarefied flows. For such conditions, we compare the maximum-entropy solutions to results obtained from the kinetic theory of gases at different Knudsen numbers. The analysis is performed for both a simplified model of a gas with a single translational degree of freedom (5-moment system) and for a typical gas with three degrees of freedom (14-moment system). The maximum-entropy method is applied to the study of the Sod shock-tube problem at various rarefaction levels, and to the simulation of two-dimensional low-collisional crossed supersonic jets. We show that, in rarefied supersonic conditions, it is important to employ accurate estimates of the wave speeds. Since analytical expressions are not presently available, we propose an approximation, valid for the 14-moment system. In these conditions, the solution of the maximum-entropy system is shown to realize large degrees of non-equilibrium and to approach the Junk subspace, yet provides a good overall accuracy and agreement with the kinetic theory. Numerical procedures for reaching second-order accurate discretizations are discussed, as well as the implementation of the 14-moment solver on Graphics Processing Units (GPUs).

The radius valley, i.e., a dearth of planets with radii between 1.5 and 2 Earth radii, provides insights into planetary formation and evolution. Using homogenously revised planetary parameters from Kepler 1-minute short cadence light curves, we remodel transits of 72 small planets mostly orbiting low-mass stars, improving the precision and accuracy of planet parameters. By combining this sample with a similar sample of planets around higher-mass stars, we determine the depth of the radius valley as a function of stellar mass. We find that the radius valley is shallower for low-mass stars compared to their higher mass counterparts. Upon comparison, we find that theoretical models of photoevaporation under-predict the number of planets observed inside the radius valley for low-mass stars: with decreasing stellar mass, the predicted fraction of planets inside the valley remains approximately constant whereas the observed fraction increases. We argue that this provides evidence for the presence of icy planets around low-mass stars. Alternatively, planets orbiting low-mass stars undergo more frequent collisions and scatter in the stars' high-energy output may also cause planets to fill the valley. We predict that more precise mass measurements for planets orbiting low mass stars would be able to distinguish between these scenarios., Comment: 19 pages, accepted for publication in MNRAS

A wide range of implicit time integration methods, including multi-step, implicit Runge-Kutta, and Galerkin finite-time element schemes, is evaluated in the context of chaotic dynamical systems. The schemes are applied to solve the Lorenz equations, the equation of motion of a Duffing oscillator, and the Kuramoto-Sivashinsky system, with the goal of finding the most computationally efficient method that results in the least expensive model for a chosen level of accuracy. It is found that the quasi-period of a chaotic system strongly limits the time-step size that can be used in the simulations, and all schemes fail once the time-step size reaches a significant fraction of that period. In these conditions, the computational cost per time-step becomes one of the most important factors determining the efficiency of the schemes. The cheaper, second-order schemes are shown to have an advantage over the higher-order schemes at large time-step sizes, with one possible exception being the fourth-order continuous Galerkin scheme. The higher-order schemes become more efficient than the lower-order schemes as accuracy requirements tighten. If going beyond the second-order is necessary for reasons other than computational efficiency, the fourth-order methods are shown to perform better than the third-order ones at all time-step sizes., Comment: 38 pages, 15 figures

The atmospheres of small, close-in exoplanets are vulnerable to rapid mass-loss during protoplanetary disc dispersal via a process referred to as `boil-off', in which confining pressure from the local gas disc reduces, inducing atmospheric loss and contraction. We construct self-consistent models of planet evolution during gaseous core accretion and boil-off. As the surrounding disc gas dissipates, we find that planets lose mass via subsonic breeze outflows which allow causal contact to exist between disc and planet. Planets initially accrete of order $\sim 10\%$ in atmospheric mass, however, boil-off can remove $\gtrsim 90\%$ of this mass during disc dispersal. We show that a planet's final atmospheric mass fraction is strongly dictated by the ratio of cooling timescale to disc dispersal timescale, as well as the planet's core mass and equilibrium temperature. With contributions from core cooling and radioactivity, we show that core luminosity eventually leads to the transition from boil-off to core-powered mass-loss. We find that smaller mass planets closest to their host star may have their atmospheres completely stripped through a combination of boil-off and core-powered mass-loss during disc dispersal, implying the existence of a population-level radius gap emerging as the disc disperses. We additionally consider the transition from boil-off/core-powered mass-loss to X-ray/EUV (XUV) photoevaporation by considering the penetration of stellar XUV photons below the planet's sonic surface. Finally, we show that planets may open gaps in their protoplanetary discs during the late stages of boil-off, which may enhance mass-loss rates., Comment: 18 pages, 8 figures. Accepted for publication in MNRAS

We look for signatures of the Hu-Sawicki f(R) modified gravity theory, proposed to explain the observed accelerated expansion of the universe; in observations of the galaxy distribution, the cosmic microwave background (CMB), and gravitational lensing of the CMB. We study constraints obtained by using observations of only the CMB primary anisotropies, before adding the galaxy power spectrum and its cross-correlation with CMB lensing. We show that cross-correlation of the galaxy distribution with lensing measurements is crucial to breaking parameter degeneracies, placing tighter constraints on the model. In particular, we set a strong upper limit on $\log{\lvert f_{R_0}\lvert }<-4.61$ at 95% confidence level. This means that while the model may explain the accelerated expansion, its impact on large-scale structure closely resembles General Relativity. Studies of this kind with future data sets will probe smaller potential deviations from General Relativity., Comment: 11 pages, 11 figures, submitted to A&A

Historically, higher learning was based on the study of the Great Works of thought of the Western canon. These works span a broad range of time, from the Classical period, to early Christianity, and the Enlightenment, all the way to the 20th century. Presently, close study of Great Works is less common at most mainstream colleges and universities. Depending on the general education programs at a given institution, or students' particular course work, it is very possible for students to graduate from college with little to no exposure to the foundational texts of Plato, Aristotle, Homer, or Dante, to name a few. If students desire a deep and broad understanding of the Great Works, they must actively seek it out. Although Great Works-specific coursework is less available, however they do still exist. The Martin Center researched 48 academic programs that involve a close study of Great Books of Western thought. Although some of the programs in this report are not advertised as Great Books programs, their curricula include an in-depth study of core texts. Uniting these programs is a desire for wisdom and understanding, and the belief that engaging with the Great Books can aid in this pursuit.

Numerous degree programs throughout the UNC System equip students with the requisite knowledge and skills for meaningful careers that generate excellent returns for both alumni and the North Carolina economy. This talent pool attracts businesses and residents to the state, expanding job opportunities, further developing the labor force, and fostering economic growth. Recent data from the Texas Public Policy Foundation (TPPF) on post-graduation debt and income, however, suggest that a substantial proportion of programs fail to generate satisfactory economic outcomes that reasonably enable alumni to pay back their student loan debt. The TPPF data demonstrate the performance of more than 900 bachelor's, master's, professional, and doctoral degree programs across North Carolina. By categorizing these programs based on the debt and income of their graduates, we are able to identify those programs that are most in need of oversight, reform, or closure. The report also allows prospective students and their families to make better-informed decisions regarding their college and later careers. Unlike resources that merely review the potential income for types of programs generally, the report provides detailed information on income and debt for specific programs at specific schools in North Carolina, providing a uniquely high-resolution picture of the financial risks and opportunities faced by UNC students today.