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1. Upgrading the Submillimeter Array: wSMA and beyond

Author

Grimes, Paul K., Keating, Garrett K., Blundell, Raymond, Christensen, Robert D., Gurwell, Mark, Kovacs, Attila, Norton, Timothy, Paine, Scott N., Rao, Ramprasad, Tong, Edward C. -Y., Weintroub, Jonathan, Wilner, David, Wilson, Robert W., Zeng, Lingzhen, and Zhang, Qizhou

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The Submillimeter Array (SMA) is an array of 8 antennas operating at millimeter and submillimeter wavelengths on Maunakea, Hawaii, operated by the Smithsonian Astrophysical Observatory and Academia Sinica Institute of Astronomy and Astrophysics, Taiwan. Over the past several years, we have been preparing a major upgrade to the SMA that will replace the aging original receiver cryostats and receiver cartridges with all new cryostats and new 230 and 345 GHz receiver designs. This wideband upgrade (wSMA) will also include significantly increased instantaneous bandwidth, improved sensitivity, and greater capabilities for dual frequency observations. In this paper, we will describe the wSMA receiver upgrade and status, as well as the future upgrades that will be enabled by the deployment of the wSMA receivers., Comment: To be published in the proceedings of SPIE Astronomical Telescopes + Instrumentation 2024, paper number 13096-122

Published
2024

5. Conclusion

Author

Forgács, István, Kovács, Attila, Forgács, István, and Kovács, Attila

Published
2024
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9. Creating Cyber Resiliency in Critical Infrastructures

Author

Kovacs, Attila Mate, Masys, Anthony J., Editor-in-Chief, Bichler, Gisela, Advisory Editor, Bourlai, Thirimachos, Advisory Editor, Johnson, Chris, Advisory Editor, Karampelas, Panagiotis, Advisory Editor, Leuprecht, Christian, Advisory Editor, Morse, Edward C., Advisory Editor, Skillicorn, David, Advisory Editor, Yamagata, Yoshiki, Advisory Editor, Kovács, Tünde Anna, editor, Nyikes, Zoltán, editor, Berek, Tamás, editor, Daruka, Norbert, editor, and Tóth, László, editor

Published
2024
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11. Deep Learning-Derived Myocardial Strain

Author

Kwan, Alan C., Chang, Ernest W., Jain, Ishan, Theurer, John, Tang, Xiu, Francisco, Nadia, Haddad, Francois, Liang, David, Fábián, Alexandra, Ferencz, Andrea, Yuan, Neal, Merkely, Béla, Siegel, Robert, Cheng, Susan, Kovács, Attila, Tokodi, Márton, and Ouyang, David

Published
2024
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12. Significant Disagreement Between Conventional Parameters and 3D Echocardiography-Derived Ejection Fraction in the Detection of Right Ventricular Systolic Dysfunction and Its Association With Outcomes

Author

Tolvaj, Máté, Kovács, Attila, Radu, Noela, Cascella, Andrea, Muraru, Denisa, Lakatos, Bálint, Fábián, Alexandra, Tokodi, Márton, Tomaselli, Michele, Gavazzoni, Mara, Perelli, Francesco, Merkely, Béla, Badano, Luigi P., and Surkova, Elena

Published
2024
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18. RVENet: A Large Echocardiographic Dataset for the Deep Learning-Based Assessment of Right Ventricular Function

Author

Magyar, Bálint, Tokodi, Márton, Soós, András, Tolvaj, Máté, Lakatos, Bálint Károly, Fábián, Alexandra, Surkova, Elena, Merkely, Béla, Kovács, Attila, Horváth, András, Goos, Gerhard, Founding Editor, Hartmanis, Juris, Founding Editor, Bertino, Elisa, Editorial Board Member, Gao, Wen, Editorial Board Member, Steffen, Bernhard, Editorial Board Member, Yung, Moti, Editorial Board Member, Karlinsky, Leonid, editor, Michaeli, Tomer, editor, and Nishino, Ko, editor

Published
2023
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20. Cardiac radiation improves ventricular function in mice and humans with cardiomyopathy

Author

Pedersen, Lauren N., Valenzuela Ripoll, Carla, Ozcan, Mualla, Guo, Zhen, Lotfinaghsh, Aynaz, Zhang, Shiyang, Ng, Sherwin, Weinheimer, Carla, Nigro, Jessica, Kovacs, Attila, Diab, Ahmed, Klaas, Amanda, Grogan, Felicia, Cho, Yoonje, Ataran, Anahita, Luehmann, Hannah, Heck, Abigail, Kolb, Kollin, Strong, Lori, Navara, Rachita, Walls, Gerard M., Hugo, Geoff, Samson, Pamela, Cooper, Daniel, Reynoso, Francisco J., Schwarz, Julie K., Moore, Kaitlin, Lavine, Kory, Rentschler, Stacey L., Liu, Yongjian, Woodard, Pamela K., Robinson, Clifford, Cuculich, Phillip S., Bergom, Carmen, and Javaheri, Ali

Published
2023
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28. Modelling the feeding process for aluminium production

Author

Kovacs, Attila, Breward, Christopher, Münch, Andreas, Oliver, James, Nordgård-Hansen, Ellen, Manger, Eirik, and Halvorsen, Svenn Anton

Subjects
669, Applied mathematics, Mathematical models
Abstract

In this thesis, we build and solve various mathematical models to describe the interplay between alumina particles and a cryolite bath that takes place in a Hall-Héroult cell, which is the foundational process for aluminium production. We aim to understand the heat and mass transfer mechanisms taking place in order to gather insights into the aluminium production process and use these insights to suggest process improvements. First, we examine the problem of adding a cold alumina particle to a bath of hot cryolite. We develop a spherically symmetric model to describe heat and mass transfer between the particle and the surrounding material, allowing for freezing and melting of the cryolite close to the particle and its subsequent dissolution. We solve this model numerically using the method of lines using the early-time asymptotic solution to initiate the numerical scheme. We explore the behaviour as we vary the key dimensionless parameters. We also consider the model in the limits of small superheat and of small Stefan number. Using these asymptotic solutions, we find approximate expressions for the freezing, melting, and dissolution timescales, with freezing being the fastest effect and dissolution the slowest. Also, using the early-time solution, we determine constraints on the parameters for which shell growth is possible. Our results predict that increasing the superheat or decreasing the particle size should decrease the time it takes for a particle to dissolve, in accordance with practical experience. Furthermore, we note that the temperature changes are localised to a 5--10 particle radii. Second, we formulate a one-dimensional model for the phase-changing infiltration into a porous alumina raft placed on top of the cryolite. We simplify our model in the limit of small superheat. We solve the equations using the same approach as in Chapter 2 with the method of lines, using the early-time asymptotic solution to initiate the numerical scheme. We find that the early-time problem can exhibit a stable and an unstable solution and in certain parameter regions, these solutions disappear altogether. Furthermore, depending on the heat loss through the top of the raft, the model can undergo a discontinuous change in behaviour which corresponds to the clogging of the pore space. Additionally, near clogging, we find power-law behaviour of the frozen cryolite fraction and the location of the infiltration and solidification fronts. Third, we formulate a model for the disintegration of a spherical clump of alumina particles. We solve the problem numerically with the method of lines and see that, for certain parameters, the solution behaves like a travelling dissolution front, while in other regimes there is bulk dissolution. We investigate the travelling dissolution front by using the method of matched asymptotic expansions to reduce the full problem. The asymptotic expressions match well with the numerical solutions up to the order that would be expected. In Chapter 5 we formulate a model for the phase-changing infiltration into a spherical clump of alumina particles, which physically corresponds to a larger batch that is entirely enclosed by the cryolite. We find that many of the results in Chapter 3 carry over, such as the multiple solutions for early time, the late time clogging, or the fact that the phase-changing front is slower than the isothermal one. The presence of clogging in this model is especially interesting as it is caused by the slowing down of the front, as opposed to the cooling at the top, which was the case in Chapter 3. Finally, we summarize the findings and offer possible extensions to our models in Chapter 6 and present our mathematical findings in an approachable way in Chapter 7. The alumina feeding is a process with many interacting parts producing complex behaviour. In this thesis we shed light on a few problems, but the research is not over.

Published
2020

29. 2 mm GISMO Observations of the Galactic Center. II. A Nonthermal Filament in the Radio Arc and Compact Sources

Author

Staguhn, Johannes, Arendt, Richard G., Dwek, Eli, Morris, Mark R., Yusef-Zadeh, Farhad, Benford, Dominic J., Kovács, Attila, and Gonzalez-Quiles, Junellie

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

We have used the Goddard IRAM 2-Millimeter Observer (GISMO) with the 30 m IRAM telescope to carry out a 2 mm survey of the Galaxy's central molecular zone (CMZ). These observations detect thermal emission from cold ISM dust, thermal free-free emission from ionized gas, and nonthermal synchrotron emission from relatively flat-spectrum sources. Archival data sets spanning $3.6 \mu$m to 90 cm are used to distinguish different emission mechanisms. After the thermal emission of dust is modeled and subtracted, the remaining 2 mm emission is dominated by free-free emission, with the exception of the brightest nonthermal filament (NTF) that runs though the middle of the bundle of filaments known as the Radio Arc. This is the shortest wavelength at which any NTF has been detected. The GISMO observations clearly trace this NTF over a length of ~0.2$^\circ$, with a mean 2 mm spectral index which is steeper than at longer wavelengths. The 2 mm to 6 cm (or 20 cm) spectral index steepens from $\alpha \approx -0.2$ to $-0.7$ as a function distance from the Sickle H II region, suggesting that this region is directly related to the NTF. A number of unresolved (at $21''$) 2 mm sources are found nearby. One appears to be thermal dust emission from a molecular cloud that is associated with an enigmatic radio point source whose connection to the Radio Arc is still debated. The morphology and colors at shorter IR wavelengths indicate other 2 mm unresolved sources are likely to be compact H II regions., Comment: 17 pages, 11 figures. Accepted for publication in the ApJ

Published
2019
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30. 2 mm GISMO Observations of the Galactic Center. I. Dust Emission

Author

Arendt, Richard G., Staguhn, Johannes, Dwek, Eli, Morris, Mark R., Yusef-Zadeh, Farhad, Benford, Dominic J., Kovács, Attila, and Gonzalez-Quiles, Junellie

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

The Central Molecular Zone (CMZ), covering the inner ~1$^\circ$ of the Galactic plane has been mapped at 2 mm using the GISMO bolometric camera on the 30 m IRAM telescope. The $21''$ resolution maps show abundant emission from cold molecular clouds, from star forming regions, and from one of the Galactic center nonthermal filaments. In this work we use the Herschel Hi-GAL data to model the dust emission across the Galactic center. We find that a single-temperature fit can describe the 160 -- 500 $\mu$m emission for most lines of sight, if the long-wavelength dust emissivity scales as $\lambda^{-\beta}$ with $\beta \approx 2.25$. This dust model is extrapolated to predict the 2 mm dust emission. Subtraction of the model from the GISMO data provides a clearer look at the 2 mm emission of star-forming regions and the brightest nonthermal filament., Comment: 18 pages, 15 figures. Accepted for publication in the ApJ

Published
2019
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31. Microwave multiplexing on the Keck Array

Author

Cukierman, Ari, Ahmed, Zeeshan, Henderson, Shawn, Young, Edward, Yu, Cyndia, Barkats, Denis, Brown, David, Chaudhuri, Saptarshi, Cornelison, James, D'Ewart, John M., Dierickx, Marion, Dober, Bradley J., Dusatko, John, Fatigoni, Sofia, Filippini, Jeff P., Frisch, Josef C., Haller, Gunther, Halpern, Mark, Hilton, Gene C., Hubmayr, Johannes, Irwin, Kent D., Karkare, Kirit S., Karpel, Ethan, Kernasovskiy, Sarah A., Kovac, John M., Kovacs, Attila, Kuenstner, Stephen E., Kuo, Chao-Lin, Li, Dale, Mates, John A. B., Smith, Stephen, Germaine, Tyler St., Ullom, Joel N., Vale, Leila R., Van Winkle, Daniel D., Vasquez, Jesus, Willmert, Justin, Zeng, Lingzhen, Ade, P. A. R., Amiri, M., Thakur, R. Basu, Bischoff, C. A., Bock, J. J., Boenish, H., Bullock, E., Buza, V., Cheshire, J., Connors, J., Crumrine, M., Duband, L., Hall, G., Harrison, S., Hildebrandt, S. R., Hui, H., Kang, J., Kefeli, S., Lau, K., Megerian, K. G., Moncelsi, L., Namikawa, T., Nguyen, H. T., O'Brient, R., Palladino, S., Pryke, C., Racine, B., Reintsema, C. D., Richter, S., Schillaci, A., Schwarz, R., Sheehy, C. D., Soliman, A., Steinbach, B., Sudiwala, R. V., Thompson, K. L., Tucker, C., Turner, A. D., Umilta, C., Vieregg, A. G., Wandui, A., Weber, A. C., Wiebe, D. V., Wu, W. L. K., Yang, H., Yoon, K. W., and Zhang, C.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

We describe an on-sky demonstration of a microwave-multiplexing readout system in one of the receivers of the Keck Array, a polarimetry experiment observing the cosmic microwave background at the South Pole. During the austral summer of 2018-2019, we replaced the time-division multiplexing readout system with microwave-multiplexing components including superconducting microwave resonators coupled to radio-frequency superconducting quantum interference devices at the sub-Kelvin focal plane, coaxial-cable plumbing and amplification between room temperature and the cold stages, and a SLAC Microresonator Radio Frequency system for the warm electronics. In the range 5-6 GHz, a single coaxial cable reads out 528 channels. The readout system is coupled to transition-edge sensors, which are in turn coupled to 150-GHz slot-dipole phased-array antennas. Observations began in April 2019, and we report here on an initial characterization of the system performance., Comment: 9 pages, 11 figures, Accepted by the Journal of Low Temperature Physics (Proceedings of the 18th International Workshop on Low Temperature Detectors)

Published
2019
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33. Constraining the Active Galactic Nucleus and Starburst Properties of the IR-luminous Quasar Host Galaxy APM 08279+5255 at Redshift 4 with SOFIA

Author

Leung, T. K. Daisy, Hayward, Christopher C., Casey, Caitlin M., Staguhn, Johannes, Kovacs, Attila, and Dowell, C. Darren

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

We present far-IR photometry and infrared spectrum of the z=3.9114 quasar/starburst composite system APM 08279+5255 obtained using the Stratospheric Observatory for Infrared Astronomy (SOFIA)/HAWC+ and the Spitzer Space Telescope Infrared Spectrograph (IRS). We decompose the IR-to-radio spectral energy distribution (SED), sampled in 51 bands, using (i) a model comprised of two-temperature modified blackbodies (MBB) and radio power-laws and (ii) a semi-analytic model, which also accounts for emission from a clumpy torus. The latter is more realistic but requires a well-sampled SED, as possible here. In the former model, we find temperatures of T_warm = 296^17_15 K and T_cold = 110^3_3 K for the warm and cold dust components, respectively. This model suggests that the cold dust component dominates the FIR energy budget (66%) but contributes only 17% to the total IR luminosity. Based on the torus models, we infer an inclination angle of i=15^8_8 degree and the presence of silicate emission, in accordance with the Type-1 active galactic nucleus nature of APM 08279+5255. Accounting for the torus' contribution to the FIR luminosity, we find a lensing-corrected star formation rate of SFR=3075x(4/mu_L) Msun yr^-1. We find that the central quasar contributes 30% to the FIR luminosity but dominates the total IR luminosity (93%). The 30% correction is in contrast to the 90% reported in previous work. In addition, the IR luminosity inferred from the torus model is a factor of two higher. These differences highlight the importance of adopting physically motivated models to properly account for IR emission in high-z quasars, which is now possible with SOFIA/HAWC+., Comment: 14 pages, 6 figures, 2 tables, accepted to ApJ

Published
2019
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34. Sustained alternate-day fasting potentiates doxorubicin cardiotoxicity

Author

Ozcan, Mualla, Guo, Zhen, Valenzuela Ripoll, Carla, Diab, Ahmed, Picataggi, Antonino, Rawnsley, David, Lotfinaghsh, Aynaz, Bergom, Carmen, Szymanski, Jeff, Hwang, Daniel, Asnani, Aarti, Kosiborod, Mikhail, Zheng, Jie, Hayashi, Robert J., Woodard, Pamela K., Kovacs, Attila, Margulies, Kenneth B., Schilling, Joel, Razani, Babak, Diwan, Abhinav, and Javaheri, Ali

Published
2023
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36. SOFIA - HIRMES: Looking forward to the HIgh-Resolution Mid-infrarEd Spectrometer

Author

Richards, Samuel N., Moseley, Samuel H., Stacey, Gordon, Greenhouse, Matthew, Kutyrev, Alexander, Arendt, Richard, Atanasoff, Hristo, Banks, Stuart, Brekosky, Regis P., Brown, Ari-David, Bulcha, Berhanu, Cazeau, Tony, Choi, Michael, Colazo, Felipe, Engler, Chuck, Hadjimichael, Theodore, Hays-Wehle, James, Henderson, Chuck, Hsieh, Wen-Ting, Huang, Jeffrey, Jenstrom, Iver, Kellogg, Jim, Kimball, Mark, Kovacs, Attila, Leiter, Steve, Maher, Steve, McMurray, Robert, Melnick, Gary J., Mentzell, Eric, Mikula, Vilem, Miller, Timothy M., Nagler, Peter, Nikola, Thomas, Oxborrow, Joseph, Pontoppidan, Klaus M., Rangwala, Naseem, Rhodes, Alan, Roberge, Aki, Rosner, Stefan, Rostem, Karwan, Rustemeyer, Nancy, Sharp, Elmer, Sparr, Leroy, Stevanovic, Dejan, Taraschi, Peter, Temi, Pasquale, Vacca, William D., de Lorenzo, Jordi Vila Hernandez, Wohler, Bill, Wollack, Edward J., and Wilks, Shannon

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The HIgh-Resolution Mid-infrarEd Spectrometer (HIRMES) is the 3rd Generation Instrument for the Stratospheric Observatory For Infrared Astronomy (SOFIA), currently in development at the NASA Goddard Space Flight Center (GSFC), and due for commissioning in 2019. By combining direct-detection Transition Edge Sensor (TES) bolometer arrays, grating-dispersive spectroscopy, and a host of Fabry-Perot tunable filters, HIRMES will provide the ability for High Resolution (R~100,000), Mid-Resolution (R~10,000), and Low-Resolution (R~600) slit-spectroscopy, and 2D Spectral Imaging (R~2000 at selected wavelengths) over the 25 - 122 {\mu}m mid-far infrared waveband. The driving science application is the evolution of proto-planetary systems via measurements of water-vapor, water-ice, deuterated hydrogen (HD), and neutral oxygen lines. However, HIRMES has been designed to be as flexible as possible to cover a wide range of science cases that fall within its phase-space, all whilst reaching sensitivities and observing powers not yet seen thus far on SOFIA, providing unique observing capabilities which will remain unmatched for decades., Comment: Accepted to the Journal of Astronomical Instrumentation (SOFIA Special Edition) on 11th November 2018

Published
2018

37. Apolipoprotein M Attenuates Anthracycline Cardiotoxicity and Lysosomal Injury

Author

Guo, Zhen, Valenzuela Ripoll, Carla, Picataggi, Antonino, Rawnsley, David R., Ozcan, Mualla, Chirinos, Julio A., Chendamarai, Ezhilarasi, Girardi, Amanda, Riehl, Terrence, Evie, Hosannah, Diab, Ahmed, Kovacs, Attila, Hyrc, Krzysztof, Ma, Xiucui, Asnani, Aarti, Shewale, Swapnil V., Scherrer-Crosbie, Marielle, Cowart, Lauren Ashley, Parks, John S., Zhao, Lei, Gordon, David, Ramirez-Valle, Francisco, Margulies, Kenneth B., Cappola, Thomas P., Desai, Ankit A., Pedersen, Lauren N., Bergom, Carmen, Stitziel, Nathan O., Rettig, Michael P., DiPersio, John F., Hajny, Stefan, Christoffersen, Christina, Diwan, Abhinav, and Javaheri, Ali

Published
2023
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41. Two-hit mouse model of heart failure with preserved ejection fraction combining diet-induced obesity and renin-mediated hypertension

Author

Berger, Justin H, primary, Shi, Yuji, additional, Matsuura, Timothy R., additional, Batmanov, Kirill, additional, Chen, Xian, additional, Tam, Kelly, additional, Marshall, Mackenzie, additional, Kue, Richard, additional, Patel, Jiten, additional, Taing, Renee, additional, Callaway, Russell, additional, Griffin, Joanna, additional, Kovacs, Attila, additional, Shanthappa, Dinesh Hirenallur, additional, Miller, Russell, additional, Zhang, Bei, additional, Flach, Rachel Roth, additional, and Kelly, Daniel P, additional

Published
2024
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42. The assessment of the seismic effect produced by the blasting works in the Măgura Sârbi Brănișca Quarry

Author

Gheorghiosu Edward, Robert Laslo, Kovacs Attila, and Ilici Ștefan

Subjects
Engineering (General). Civil engineering (General), TA1-2040
Abstract

In addition to the technical and economic advantages of blasting rocks from open-pit mining, this method of extraction can produce effects with a direct impact in the area near the quarry. Blasting works generates effects such as seismic waves that cause vibrations, rock throws, noise and toxic gases. When their intensity and scope are not systematically evaluated and analysed, blasting works can cause serious consequences for people, civil / industrial buildings, the environment, thus affecting the health of the population and the stability / integrity of the buildings / slopes in the vicinity of the mining operations. The paper presents design / determination methods of areas where explosives may / may not be used in conditions of maximum safety in terms of seismic intensity, thus protecting the population and the civil / industrial objectives in the area of the mining work.

Published
2024
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43. SOFIA/HAWC+ detection of a gravitationally lensed starburst galaxy at $z$ = 1.03

Author

Ma, Jingzhe, Brown, Arianna, Cooray, Asantha, Nayyeri, Hooshang, Messias, Hugo, Timmons, Nicholas, Staguhn, Johannes, Temi, Pasquale, Dowell, C. Darren, Wardlow, Julie, Fadda, Dario, Kovacs, Attila, Riechers, Dominik, Oteo, Ivan, Wilson, Derek, and Perez-Fournon, Ismael

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

We present the detection at 89 $\mu$m (observed frame) of the {\it Herschel}-selected gravitationally lensed starburst galaxy HATLASJ1429-0028 (also known as G15v2.19) in 15 minutes with the High-resolution Airborne Wideband Camera-plus (HAWC+) onboard the Stratospheric Observatory for Infrared Astronomy (SOFIA). The spectacular lensing system consists of an edge-on foreground disk galaxy at $z$ = 0.22 and a nearly complete Einstein ring of an intrinsic ultra-luminous infrared galaxy at $z$ = 1.03. Is this high IR luminosity powered by pure star formation (SF) or also an active galactic nucleus (AGN)? Previous nebular line diagnostics indicate that it is star-formation dominated. We perform a 27-band multi-wavelength spectral energy distribution modeling (SED) including the new SOFIA/HAWC+ data to constrain the fractional AGN contribution to the total IR luminosity. The AGN fraction in the IR turns out to be negligible. In addition, J1429-0028 serves as a testbed for comparing SED results from different models/templates and SED codes (MAGPHYS, SED3FIT, and CIGALE). We stress that star formation history is the dominant source of uncertainty in the derived stellar mass (as high as a factor of $\sim$ 10) even in the case of extensive photometric coverage. Furthermore, the detection of a source at $z$ $\sim$ 1 with SOFIA/HAWC+ demonstrates the potential of utilizing this facility for distant galaxy studies including the decomposition of SF/AGN components, which cannot be accomplished with other current facilities., Comment: 8 pages, 3 figures; accepted for publication in ApJ

Published
2018
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44. Chaotic dynamics in the planar gravitational many-body problem with rigid body rotations

Author

Kwiecinski, James A., Kovacs, Attila, Krause, Andrew L., Planella, Ferran Brosa, and Van Gorder, Robert A.

Subjects
Astrophysics - Earth and Planetary Astrophysics, Nonlinear Sciences - Chaotic Dynamics
Abstract

The discovery of Pluto's small moons in the last decade brought attention to the dynamics of the dwarf planet's satellites. With such systems in mind, we study a planar $N$-body system in which all the bodies are point masses, except for a single rigid body. We then present a reduced model consisting of a planar $N$-body problem with the rigid body treated as a 1D continuum (i.e. the body is treated as a rod with an arbitrary mass distribution). Such a model provides a good approximation to highly asymmetric geometries, such as the recently observed interstellar asteroid 'Oumuamua, but is also amenable to analysis. We analytically demonstrate the existence of homoclinic chaos in the case where one of the orbits is nearly circular by way of the Melnikov method, and give numerical evidence for chaos when the orbits are more complicated. We show that the extent of chaos in parameter space is strongly tied to the deviations from a purely circular orbit. These results suggest that chaos is ubiquitous in many-body problems when one or more of the rigid bodies exhibits non-spherical and highly asymmetric geometries. The excitation of chaotic rotations does not appear to require tidal dissipation, obliquity variation, or orbital resonance. Such dynamics give a possible explanation for routes to chaotic dynamics observed in $N$-body systems such as the Pluto system where some of the bodies are highly non-spherical., Comment: 23 pages, 7 figures

Published
2018
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50. Worldwide Disparities in Recovery of Cardiac Testing 1 Year Into COVID-19

Author

Einstein, Andrew J., Paez, Diana, Dondi, Maurizio, Better, Nathan, Cerci, Rodrigo, Dorbala, Sharmila, Karthikeyan, Ganesan, Pascual, Thomas N.B., Shaw, Leslee J., Villines, Todd C., Vitola, Joao V., Williams, Michelle C., Pynda, Yaroslav, Hinterleitner, Gerd, Lu, Yao, Morozova, Olga, Xu, Zhuoran, Hirschfeld, Cole B., Cohen, Yosef, Erinne, Ikenna, Malkovskiy, Eli, Randazzo, Michael, Sewanan, Lorenzo, Shetty, Mrinali, Choi, Andrew, Lopez-Mattei, Juan, Parwani, Purvi, Goda, Artan, Shirka, Ervina, Bouyoucef, Salah, Chelghoum, Lydia, Mansouri, Farouk, Medjahedi, Abdelkader, Naili, Qais, Ridouh, Mokhtar, Alasia, Diego, Alberghina, Lucia, Aramayo, Natalia, Buchara, Diego, Busso, Franco Gabriel, Bustos Rivadero, Jose Javier, Camilletti, Jorge, Campanelli, Hugo, Campisi, Roxana, Castro, Ricardo Belisario, Daicz, Mariana, del Riego, Horacio, Dragonetti, Laura, Echazarreta, Diego, Erriest, Juan, Faccio, Fernando, Facello, Adolfo, Gallegos, Hugo, Geronazzo, Ricardo, Glait, Horacio, Hasbani, Victor, Jäger, Victor, Lewkowicz, Julio Manuel, Lotti, Jose, Maciel, Neiva, Masoli, Osvaldo, Mastrovito, Edgardo, Medus, Maria, Merani, Maria Fernanda, Molteni, Susana, Montecinos, Marcos, Parisi, Gustavo, Sueldo, Claudio Pereyra, Perez de Arenaza, Diego, Quintana, Luis, Radzinschi, Alejandro, Redruello, Marcela, Rodríguez, Marina, Rojas, Horacio, Acuña, Arturo Romero, Schere, Daniel, Traverso, Sonia, Vazquez, Gustavo, Zeffiro, Susana, Sakanyan, Mari, Beuzeville, Scott, Boktor, Raef, Crowley, Michael, Downie, D'Arne, Dwivedi, Girish, Elison, Barry, Farouque, Omar, Jasper, Kim, Joshi, Subodh, Lee, Joseph, Lee, Kenneth, Lui, Elaine, Mcconachie, Peter, Meaker, Joanne, Nandurkar, Dee, Neill, Johanne, O'Rourke, Edward, O'Sullivan, Patricia, Pandos, George, Premaratne, Manuja, Prior, David, Rutherford, Natalie, Saunders, Connor, Taubman, Kim, Tauro, Andrew, Taylor, Andrew, Theuerle, James, Thomas, Paul, Tow, Jonathan, Upton, Anthony, Vamadevan, Shankar, Wayne, Victor, Wegner, Eva Alina, Wong, David, Younger, John, Beitzke, Dietrich, Feuchtner, Gudrun, Sommer, Oliver, Weiss, Konrad, Maroz-Vadalazhskaya, Natallia, Tserakhau, Uladzimir, Homans, Filip, Van De Heyning, Caroline M., Araujo, Raúl, Soldat-Stankovic, Valentina, Stankovic, Sinisa, Almeida, Augusto, Anselmi, Carlos, Azevedo, Guilherme S.A., Bittencourt, Marcio Sommer, Pianta, Diego Bromfman, Cabeda, Estevan, Carreira, Lara, Coelho, Igor, de Amorim Fernandes, Fernando, de Lorenzo, Andrea, Delgado, Roberta, Erthal, Fernanda, Fernandes, Fabio, Fernandes, Juliano, Ferreira de Souza, Thiago, Foppa, Murilo, Matos Alves, Wilson Furlan, Gontijo, Cibele, Gottlieb, Ilan, Grossman, Gabriel, Albernaz Siqueira, Maria Helena, Nomura, Cesar Higa, Koga, Katia Hiromoto, Lima, Ronaldo, Lopes, Rafael, Marçal Filho, Hugo Humberto, Masiero, Paulo, Mastrocola, Luiz, Menezes de Siqueira, Maria Eduarda, Mesquita, Claudio, Naves, Danilo, Penna, Filipe, Pinto, Ibraim, Rocha, Thércio, Rocha, Juliana Leal, Rodrigues, Alfredo, Salioni, Leila, Sanches, Adelina, Santos, Marcelo, Da Silva, Leonardo Sara, Schvartzman, Paulo, Matushita, Cristina Sebastião, Senra, Tiago, Silva, Marcelo, Soares, Carlos Eduardo, Spiro, Bernardo, Suaide Silva, Carlos Eduardo, Torres, Rafael, Monte, Guilherme Urpia, Vilela, Andrea, Villa, Alexandre Volney, Vitola, Joao, Voss, Themissa, Waltrick, Roberto, Zapparoli, Marcello, Naseer, Hamid, Garcheva-Tsacheva, Marina, Ouattara, Tiémégna Florence, Thou, Sarameth, Varoeun, Soley, Abikhzer, Gad, Beanlands, Rob, Chetrit, Michael, Dabreo, Dominique, Dennie, Carole, Friedrich, Matthias, Hafez, Mohmmed Nassoh, Hanneman, Kate, Miller, Robert, Oikonomou, Anastasia, Roifman, Idan, Small, Gary, Tandon, Vikas, Trivedi, Adwait, White, James, Zukotynski, Katherine, Alay, Rita, Concha, Carmen, Massardo, Teresa, Abad, Pedro, Anzola, Kelly, Arturo, Harold, Benitez, Luis, Cadena, Alberto, Zamudio, Carlos Caicedo, Calderón, Antonio, Gutierrez Villamil, Claudia T., Jaimes, Claudia, Londono, Juan L., Lopez, Nelson, 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Bawinile, Hlongwa, Khanyisile, Kaplan, Mitchell, Lakhi, Hoosen, Milos, Katarina, Modiselle, Moshe, More, Stuart, Muambadzi, Ntanganedzeni, Scholtz, Leonie, Barreiro-Perez, Manuel, Blanco, Isabel, Broncano, Jordi, Camarero, Alicia, Casáns-Tormo, Irene, De Haro, Javier, Flotats, Albert, García, Elia, Mendiguchia, Ceferino Gutierrez, Jimenez-Heffernan, Amelia, Leta, Ruben, Diaz, Javier Lopez, Vega, Luis Lumbreras, Manovel-Sánchez, Ana, Monzonis, Amparo Martinez, Patrut, Bianca, Pubul, Virginia, Perez, Ricardo Ruano, Zeidan, Nahla, Nanayakkara, Damayanthi, Suliman, Ahmed, Engblom, Henrik, Murtadha, Mustafa, Ostenfeld, Ellen, Simonsson, Magnus, Alkadhi, Hatem, Buechel, Ronny Ralf, Burger, Peter, Gräni, Christoph, Kamani, Christel, Kawel-Böhm, Nadine, Klaeser, Bernd, Manka, Robert, Prior, John, Kaewchur, Tawika, Khiewvan, Benjapa, Kositwattanarerk, Arpakorn, Namwongprom, Sirianong, Thientunyakit, Tanyaluck, Sayman, Haluk Burcak, Yüksel, Mahmut, Sebikali, Mugisha Julius, Okello, Emmy, Korol, Pavlo, Noverko, Iryna, Satyr, Maryna, Ahmad, Tahir, Alfakih, Khaled, Andrade, Ivo, Buckingham, Susan, Bularga, Anda, Carpenter, John-Paul, Cole, Graham, Cusack, David, David, Sarojini, Davis, Patrick, Fairbairn, Timothy, Ghosh, Arjun, Ramkumar, Prasad Guntur, Hamilton, Mark, Haque, Faisal, Hudson, Benjamin, Johnstone, Annette, Karthikeyan, V.J., Kay, Mike, Khan, Mohammad Ali, Kitt, Jamie, Low, Chen Sheng, Mcalindon, Elisa, Mccreavy, David, Morrissey, Brian, Motwani, Manish, Na, Dilip, Nicol, Edward, Patel, Dilip, Rodrigues, Jonathan, Rofe, Chris, Schofield, Rebecca, Semple, Thomas, Sheikh, Azeem, Sinha, Apurva, Subedi, Deepak, Topping, William, Tweed, Katherine, Underwood, Stephen Richard, Weir-Mccall, Jonathan, Zuhairy, Hamed, Abbasi, Taimur, Abohashem, Shady, Abramson, Sandra, Al-Mallah, Mouaz, Kumar, Mohan Ashok, Balmer-Swain, Mallory, Berman, Daniel, Bernheim, Adam, Bhatti, Sabha, Biederman, Robert, Bieging, Erik, Bingham, Scott, Bloom, Stephen, Blue, Sean, Borges, Andressa, Branch, Kelley, Bravo, Paco, Buddhe, Sujatha, Budoff, Matthew, Bullock-Palmer, Renée, Cahill, Michael, Candela, Candace, Cao, Jane, Chatterjee, Saurav, Chatzizisis, Yiannis, Chaudhuri, Nita Ray, Cheezum, Michael, Chelliah, Anjali, Chen, Tiffany, Chen, Marcus, Chen, Lu, Chokshi, Aalap, Chung, Jina, Danciu, Sorin, DeSisto, William, Dilorenzo, Michael, Doukky, Rami, Duvall, William, Ferencik, Maros, Foster, Cameron, Fuisz, Anthon, Gannon, Michael, German, David, Gerson, Myron, Geske, Jeffrey, Hage, Fadi, Haider, Agha, Haider, Sofia, Hamirani, Yasmin, Hassen, Karen, Hendel, Robert, Henkel, Jacqueline, Horgan, Stephen, Hyun, Mark, Janardhanan, Rajesh, Jerome, Scott, Kalra, Dinesh, Kassop, David, Kinkhabwala, Mona, Kinzfogl, George, Koch, Bernard, Koweek, Lynne, Krepp, Joseph, Kwon, Younghoon, Layer, Jay, Lesser, John, Leung, Steve, Lisske, Bernadette, Magurany, Kathleen, Markowitz, Jeremy, Mccullough, Brenda, Moalemi, Azita, Moffitt, Chanan, Montanez, Juan, Moore, Warren, Morayati, Shamil, Mossa-Basha, Mahmud, Mrsic, Zorana, Murthy, Venkatesh, Nagpal, Prashant, Nelson, Katarina, Nijjar, Prabhjot, O’Quinn, Rupal, Passen, Edward, Patel, Toral, Patil, Pravin, Pursnani, Amit, Quachang, Nancy, Rabbat, Mark, Ranjan, Pragya, Lozano, Patricia Rodriguez, Schemmer, Mary, Seifried, Rebecca, Shah, Nishant, Shah, Amee, Shanbhag, Sujata, Sharma, Gaurav, Skotnicki, Robert, Sobczak, Michael, Soman, Prem, Sorrell, Vincent, Srichai, Monvadi, Streeter, Jim, Strickland, Leah, Suliman, Suliman, Tebyanian, Naghmeh, Thomas, Dustin, Thompson, Randall, Uretsky, Seth, Vallurupalli, Srikanth, Vandyck-Acquah, Marian, Verma, Vikas, Villines, Todd, Weinstein, Joseph, Wolinsky, David, Zareba, Karolina, Zgaljardic, Michael, Beretta, Mario, Ferrando, Rodolfo, Kapitan, Miguel, Mut, Fernando, Djuraev, Omoa, Rozikhodjaeva, Gulnora, Vera, Luisa, Duc, Binh Duong, Nguyen, Xuan Canh, Hiep Nguyen, Phuoc Minh, Hirschfeld, Cole, Choi, Andrew D., Ansheles, Alexey A., Kudo, Takashi, Bucciarelli-Ducci, Chiara, 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2022
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