Bulletin of the American Physical Society
2018 Annual Meeting of the Far West Section
Volume 63, Number 17
Thursday–Saturday, October 18–20, 2018; Cal State Fullerton, Fullerton, California
Session F03: Astrophysics and General Physics |
Hide Abstracts |
Chair: Joshua Smith, California State University, Fullerton Room: Titan Student Union Alverado B |
Saturday, October 20, 2018 2:00PM - 2:12PM |
F03.00001: Calculation of Primary Variables Affecting the g-mode Oscillations in Neutron Stars Megan L Barry, Prashanth Jaikumar Other than black holes, neutron stars are the only known source of gravitational waves. Unlike black holes, however, neutron stars contain matter at extremely high density. Thus, studying gravitational waves from neutron stars helps us discover new forms of matter. We study particular oscillations of neutron star matter driven by chemical gradients, called g-modes, that couple to gravitational waves. Using a theoretical model for the neutron star, we derive the trends in proton fraction with mass density and the Brunt-Väisälä frequency at which the g-mode oscillates. The trends confirm published results from literature for nuclear matter. We extend this benchmark to new regimes of dense matter that include a mixed phase of quark and nuclear matter. |
Saturday, October 20, 2018 2:12PM - 2:24PM |
F03.00002: Relativistic Tidal Deformations of Neutron Stars with Hybrid Equations of States Bryen E Irving, Marc Salinas, Thomas Klaehn, Jocelyn Samantha Read An exploration of how the tidal properties measured in gravitational waves (GWs) from coalescing neutron stars can be utilized to constrain the elusive neutron star (NS) equation of state (EoS) was conducted. Realistic EoS models that featured phase transitions to quark matter, governed by the vector interaction enhanced BAG (vBAG) model, were employed to simulate behavior that is more consistent with quantum chromodynamics (QCD) calculations. From these models, relations between the mass-weighted tidal deformability, Λeff, and the binary mass ratio, q = M2/M1, were analyzed to determine if a given EoS, meets the criterion determined by the GW170817 signal of 400 ≤ Λeff ≤ 800 for 0.7 ≤ q ≤ 1.0. By analyzing the tidal deformability of a single star, Λ, under the condition that Λ(1.4Msolar) ≤ 800 and 2.01Msolar ≤ max(M) ≤ 2.16Msolar, constraints to the EoS of the strongly-interacting dense matter on the interiors of NSs can be placed. We find that nuclear models of EoS with Λ(1.4Msolar) > 800 cannot easily be ruled out because a transition to quark matter can occur, which would result in a more compact hybrid configuration--thus a lower Λ. |
Saturday, October 20, 2018 2:24PM - 2:36PM |
F03.00003: Growth, Impact, Productivity, and Scaling in Research Institutions Zihao He, Keith Burghardt, Allon Percus, Kristina Lerman The past two decades have seen significant research into understanding scaling laws in biology, cities, and networks. We extend these observations to explore how research growth, productivity, impact, and collaborations scale with the size of research institutions by analyzing physics papers in APS journals (through 2017) and the Microsoft Academic Graph (MAG). The latter, one of the largest datasets of scholarly publications with the most complete citation data available, has never before been used to analyze the scaling laws of research activity. In both datasets we discover that while mean productivity per researcher is independent of institution size, a paper’s impact, the number of authors per paper, and the total number of collaborations per researcher, especially within an institution, all scale positively with institution size. Because the number of authors correlates with the paper’s impact, affiliation size appears to partly affect a paper’s impact by improving the ability for researchers to interact. Large institutions, in other words, provide an economy of scale to improve collaborations and research overall. We also discuss initial mechanistic models to explain the scaling laws we observe. |
Saturday, October 20, 2018 2:36PM - 2:48PM |
F03.00004: Is there a best way to measure? Perhaps: maximizing ephemeral information suggests the coarsest generating partition. Mikhael Semaan, Ryan G. James, James P. Crutchfield We imagine the act of measurement as that of partitioning (coarse graining) an underlying dynamical system, producing a sequence of symbols: the raw data. Provided we choose a generating partition—and there are many such choices—symbolic dynamics allows modeling that underlying system (in terms of its hidden states and a dynamic between them) from only this raw data. Taking the tent map as an example, we find that while the uncertainty generated by a single measurement—the Shannon entropy rate hμ—does not (by definition) depend on the choice of generating partition, the amount of that uncertainty which affects future measurements—the bound information bμ—does. Of the generating partitions, then, which should we choose? Is there a best one? Here, we offer an answer: preliminary evidence suggests the supremum over all partitions of the ephemeral information—rμ = hμ − bμ, uncertainty generated by a single measurement which does not affect the future—may be a dynamical invariant, effectively selecting the coarsest generating partition. |
Saturday, October 20, 2018 2:48PM - 3:00PM |
F03.00005: Abstract Withdrawn
|
Saturday, October 20, 2018 3:00PM - 3:12PM |
F03.00006: Coarse-Graining for Coupled Oscillators: A case study in discovering low-dimensional dynamics Jordan Snyder, Andrey Lokhov, Anatoly Zlotnik Quantitative science has produced successful models of the |
Saturday, October 20, 2018 3:12PM - 3:24PM |
F03.00007: Abstract Withdrawn
|
Saturday, October 20, 2018 3:24PM - 3:36PM |
F03.00008: Higher-dimernsional quantum hypergraph-product codes Weilei Zeng, Leonid P Pryadko The quantum hypergraph-product codes by Tillich and Zemor, and m-dimensional toric codes could be generalized into one family of codes. Those codes are isomorphic to the CSS codes generated by m-chain complex. A recursive formula is given for such construction, with explicit code parameters. This work is useful for constructing fault-tolerant quantum LDPC codes. |
Follow Us |
Engage
Become an APS Member |
My APS
Renew Membership |
Information for |
About APSThe American Physical Society (APS) is a non-profit membership organization working to advance the knowledge of physics. |
© 2024 American Physical Society
| All rights reserved | Terms of Use
| Contact Us
Headquarters
1 Physics Ellipse, College Park, MD 20740-3844
(301) 209-3200
Editorial Office
100 Motor Pkwy, Suite 110, Hauppauge, NY 11788
(631) 591-4000
Office of Public Affairs
529 14th St NW, Suite 1050, Washington, D.C. 20045-2001
(202) 662-8700