On Index System Of Space Science Strength And Its Enlightenment,
2022
National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China
On Index System Of Space Science Strength And Its Enlightenment, Quanlin Fan, Tingting Song, Peng Shi, Haiyan Wei, Xiaoli Chen, Xuezhao Wang, Shijie Guo
Bulletin of Chinese Academy of Sciences (Chinese Version)
Major achievements of space science and technology are important symbols of a country's scientific and technological level and ability. The basic consensus of the aerospace community is that China's space technology has been well-developed, space applications need to be strengthened, and space science is relatively the less-developed. Thus, it is extremely urgent for China to build a strong country in space science and tackle the "bottleneck". Here we elaborate the internal logic among the strength of S&T, aerospace, and space science, expound the connotation of space science strength, investigate the index system, and suggest the three-tier system scientifically for the …
Thoughts On Space Science Development,
2022
Technology and Engineering Center for Space Utilization, Chinese Academy of Sciences, Beijing 100094, China
Thoughts On Space Science Development, Yidong Gu
Bulletin of Chinese Academy of Sciences (Chinese Version)
Space science is a large-scale activity by using space vehicles to explore the universe and natural laws and carry out special experiments, which has made great contributions to the development of contemporary science. This paper outlines the major breakthroughs in international space science, analyzes the context and new trends of space science and manned exploration activities, reviews the development achievements of space science in China in the past 20 years, puts forward existing problems and gaps, and emphasizes the strategic position of space science and its importance to China's science and technology, aerospace and the national long-term development. It is …
Prospects Of Global Space Science Breakthroughs And China’S Contributions,
2022
National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China
Prospects Of Global Space Science Breakthroughs And China’S Contributions, Chi Wang
Bulletin of Chinese Academy of Sciences (Chinese Version)
Space science is a frontier interdisciplinary subject that probes the macroscopic and microscopic worlds with spacecraft as a platform. Since the 1960s, many Nobel Prize-level discoveries and original achievements have been spawned in related basic science, breaking through the boundaries of human cognition of the nature, and expanding the human knowledge graph continuously. In the 21st century, with a new round of scientific and technological revolution brewing, space science has also entered a new era of revolutionary advancements. Here we review the major progress in global space science in the past ten years, as well as the trend of space …
Connecting The Last Mile To Speed Up Space Science Development Of China—Review And Prospect Of The Funding Practices For Space Science By Nsfc,
2022
National Natural Science Foundation of China, Beijing 100085, China
Connecting The Last Mile To Speed Up Space Science Development Of China—Review And Prospect Of The Funding Practices For Space Science By Nsfc, Zengqian Hou, Yupeng Yao, Guoxuan Dong, Sheng Yu
Bulletin of Chinese Academy of Sciences (Chinese Version)
Strengthening the basic scientific research in an all-round way and achieving more breakthroughs from zero to one as soon as possible are the major strategic needs of building a world leading power in science and technology in the new era. As the main channel funding basic research in China, the National Natural Science Foundation of China (NSFC) has always focused on the basic frontiers and major scientific issues in space science, carried out strategic research on the planning of relevant disciplines, sorted out key scientific questions, defined the priority development direction, and provided continuous and stable funding through major, key, …
Reverberation Mapping Of Markarian 421 Using V,R, I, And Ha Filters,
2022
Bridgewater State University
Reverberation Mapping Of Markarian 421 Using V,R, I, And Ha Filters, Alex Whitman
Honors Program Theses and Projects
Active Galactic Nuclei (AGN) at their most basic level are supermassive blackholes that emit light. While that sounds paradoxical, it speaks volumes to how little we know about these extraordinary objects. One technique that can be used, and was used here to better understand these objects is reverberation mapping. We employed this method on the AGN Markarian 421 (Mrk 421) at Bridgewater State University (BSU). Mrk 421 was chosen because it is the brightest known AGN, averaging 12.7 magnitudes, and the observational abilities of BSU are best suited for objects brighter than 18 magnitudes in optical wavelengths. We observed Mrk …
Dissipation In Global Simulations Of Accretion Disks,
2022
University of San Diego
Dissipation In Global Simulations Of Accretion Disks, Catherine Gibson, Theodore Dezen Phd
Creative Collaborations: Annual Showcase of Undergraduate Research
Abstract: We perform general relativistic magneto-hydrodynamic simulations to study the dynamics of and radiation from accretion onto stellar mass black holes. Recent theoretical work suggested magnetic torques exerted at the innermost stable circular orbit can drive significant bulk vertical energy transport in regions close to the black hole, and hence dissipate a larger fraction of accretion power near the photosphere compared to standard models. This additional heating in turn may lead to the non-thermal high-energy (into several hundred keVs) radiation observed in some systems. We analyze time-dependent global simulations to further assess the feasibility of such models and illuminate the …
X-Ray Properties Of Early-Type Stars In The Tarantula Nebula From T-Rex,
2022
University of Sheffield
X-Ray Properties Of Early-Type Stars In The Tarantula Nebula From T-Rex, Paul A. Crowther, Patrick S. Broos, Leisa K. Townsley, Andy M. T. Pollock, Katie A. Tehrani, Marc Gagné
Earth & Space Sciences Faculty Publications
We reassess the historical L-X/L-Bol relation for early-type stars from a comparison between T-ReX, the Chandra ACIS X-ray survey of the Tarantula Nebula in the Large Magellanic Cloud (LMC), and contemporary spectroscopic analysis of massive stars obtained primarily from VLT/FLAMES, VLT/MUSE, and HST/STIS surveys. For 107 sources in common (some host to multiple stars), the majority of which are bolometrically luminous (40 per cent exceed 10(6)L(circle dot)), we find an average log L-X/L-Bol = -6.90 +/- 0.65. Excluding extreme systems Mk 34 (WN5h+WN5h), R140a (WC4+WN6+), and VFTS 399 (O9 IIIn+?), plus four WR sources with anomalously hard X-ray components (R130, …
Continuum Damping Effects In Nuclear Collisions,
2022
Department of Physics, Faculty of Science, University of Arak, Arak 8349-8-38156, Iran
Continuum Damping Effects In Nuclear Collisions, Hossein Sadeghi, Mahdieh Ghafouri
Karbala International Journal of Modern Science
The Time-Dependent Skyrme Hartree-Fock (TDSHF) calculations have been conducted to study 100Sn+16O, 116Sn+16O, and 122Sn+16O collisions on a 3-Dimensional (3D) mesh with SV-bas SF. For the 100Sn+16O collision, the continuum damping width of the rotational amplitudes in Ecm = 100, 150, 200, and 250 MeV has been achieved around 108, 185, 277, and 318, with the time evolution width for z2 around 15/5, 13/5, 13/9, or 14/3 fm2. The quadrupole deformation, kinetic energy, and rotational amplitude are studied. It is seen that the compound nucleus becomes uniform and spherical as time grows. The results of the time evolution show the …
Search For Continuous Gravitational Wave Emission From The Milky Way Center In O3 Ligo-Virgo Data,
2022
The University of Texas Rio Grande Valley
Search For Continuous Gravitational Wave Emission From The Milky Way Center In O3 Ligo-Virgo Data, R. Abbott, H. Abe, F. Acernese, M. G. Benjamin, Teviet Creighton, Mario C. Diaz, F. Llamas, Soma Mukherjee, Gaukhar Nurbek, Volker Quetschke, Wenhui Wang
Physics & Astronomy Faculty Publications
We present a directed search for continuous gravitational wave (CW) signals emitted by spinning neutron stars located in the inner parsecs of the Galactic Center (GC). Compelling evidence for the presence of a numerous population of neutron stars has been reported in the literature, turning this region into a very interesting place to look for CWs. In this search, data from the full O3 LIGO-Virgo run in the detector frequency band [10,2000] Hz have been used. No significant detection was found and 95% confidence level upper limits on the signal strain amplitude were computed, over the full search band, with …
Galaxy And Mass Assembly: Galaxy Zoo Spiral Arms And Star Formation Rates,
2022
University of Louisville
Galaxy And Mass Assembly: Galaxy Zoo Spiral Arms And Star Formation Rates, R Porter-Temple, Benne Holwerda, A M. Hopkins, L E. Porter, C Henry, T Geron, B Simmons, K Masters, S Kruk
Faculty and Staff Scholarship
Understanding the effect spiral structure has on star formation properties of galaxies is important to complete our picture of spiral structure evolution. Previous studies have investigated connections between spiral arm properties and star formation, but the effect that the number of spiral arms has on this process is unclear. Here, we use the Galaxy And Mass Assembly (GAMA) survey paired with the citizen science visual classifications from the Galaxy Zoo project to explore galaxies’ spiral arm number and how it connects to the star formation process. We use the votes from the GAMA-Kilo Degree Survey Galaxy Zoo classification to investigate …
Renormalization Scheme Dependence Of Β-Functions In Lorentz-Violating Quantum Field Theory,
2022
University of South Carolina - Columbia
Renormalization Scheme Dependence Of Β-Functions In Lorentz-Violating Quantum Field Theory, Sapan Karki, Brett David Altschul
Faculty Publications
Effective quantum field theories that allow for the possibility of Lorentz symmetry violation can sometimes also include redundancies of description in their Lagrangians. Explicit calculations in a Lorentz-violating generalization of Yukawa theory show that when this kind of redundancy exists, different renormalization schemes may lead to different expressions for the renormalization group β-functions, even at only one-loop order. However, the renormalization group scaling of physically observable quantities appears not to share this kind of scheme dependence.
Search For Subsolar-Mass Binaries In The First Half Of Advanced Ligo’S And Advanced Virgo’S Third Observing Run,
2022
The University of Texas Rio Grande Valley
Search For Subsolar-Mass Binaries In The First Half Of Advanced Ligo’S And Advanced Virgo’S Third Observing Run, R. Abbott, T. D. Abbott, F. Acernese, K. Ackley, Teviet Creighton, Mario C. Diaz, Francisco Llamas, Soma Mukherjee, Volker Quetschke, Wenhui Wang
Physics & Astronomy Faculty Publications
We report on a search for compact binary coalescences where at least one binary component has a mass between 0.2 M⊙ and 1.0 M⊙ in Advanced LIGO and Advanced Virgo data collected between 1 April 2019 1500 UTC and 1 October 2019 1500 UTC. We extend our previous analyses in two main ways: we include data from the Virgo detector and we allow for more unequal mass systems, with mass ratio q≥0.1. We do not report any gravitational-wave candidates. The most significant trigger has a false alarm rate of 0.14 yr−1. This implies an upper limit on the merger rate …
Improved Measurement Of Neutrino Oscillation Parameters By The Nova Experiment,
2022
University of South Carolina
Improved Measurement Of Neutrino Oscillation Parameters By The Nova Experiment, M. A. Acero, P. Adamson, L. Aliaga, N. Anfimov, A. Antoshkin, E. Arrieta-Diaz, L. Asquith, A. Aurisano, A. Back, C. Backhouse, M. Baird, N. Balashov, P. Baldi, B. A. Bambah, S. Bashar, K. Bays, R. Bernstein, V. Bhatnagar, D. Bhattarai, B. Bhuyan, Roberto Petti, Et. Al.
Faculty Publications
We present new νμ → νe, νμ → νμ, ⊽ μ →⊽ e, and ⊽ μ → ⊽ μ oscillation measurements by the NOvA experiment, with a 50% increase in neutrino-mode beam exposure over the previously reported results. The additional data, combined with previously published neutrino and antineutrino data, are all analyzed using improved techniques and simulations. A joint fit to the νe, νμ, ⊽ e, and ⊽ μ candidate samples within the 3-flavor neutrino oscillation framework continues to yield a best-fit point in the normal mass …
Galactic Mass-To-Light Ratios With Superfluid Dark Matter,
2022
Case Western Reserve University
Galactic Mass-To-Light Ratios With Superfluid Dark Matter, Tobias Mistele, Stacy S. Mcgaugh
Faculty Scholarship
Context. We make rotation curve fits to test the superfluid dark matter model. Aims. In addition to verifying that the resulting fits match the rotation curve data reasonably well, we aim to evaluate how satisfactory they are with respect to two criteria, namely, how reasonable the resulting stellar mass-to-light ratios are and whether the fits end up in the regime of superfluid dark matter where the model resembles modified Newtonian dynamics (MOND). Methods. We fitted the superfluid dark matter model to the rotation curves of 169 galaxies in the SPARC sample. Results. We found that the mass-to-light ratios obtained with …
Unlocking The Mystery Of Tev J2032+4130 Through Veritas Data,
2022
Bridgewater State University
Unlocking The Mystery Of Tev J2032+4130 Through Veritas Data, Devon J. Barros
Honors Program Theses and Projects
TeVJ2032+4130 is a high energy celestial object that emits Very High Energy (VHE) gamma rays and is located in the star forming region of the Cygnus constellation. It was first detected by the High Energy Gamma Ray Astronomy (HEGRA) experiment. Later observations from the Very Energetic Radiation Imaging Telescope Array System (VERITAS2014) were used to determine that the gamma-ray emission from the source could be coming from a Pulsar Wind Nebula (PWN) powered by a binary pulsar named PSR J2032+4127. For the PWN scenario, VERITAS predicted a cutoff in the gamma-ray spectrum above 10 TeV. Using ~33 hours of VERITAS …
Measurement Of The Branching Fractions Of The B+ →Ηâ "+Νâ " And B+ →Η′Â "+Νâ " Decays With Signal-Side Only Reconstruction In The Full Q2 Range,
2022
Georg-August-Universität Göttingen
Measurement Of The Branching Fractions Of The B+ →Ηâ "+Νâ " And B+ →Η′Â "+Νâ " Decays With Signal-Side Only Reconstruction In The Full Q2 Range, U. Gebauer, C. Beleño, A. Frey, I. Adachi, K. Adamczyk, H. Aihara, S. Al Said, D. M. Asner, H. Atmacan, T. Aushev, R. Ayad, V. Babu, S. Bahinipati, P. Behera, K. Belous, J. Bennett, M. Bessner, V. Bhardwaj, B. Bhuyan
Faculty and Student Publications
The branching fractions of the decays B+→ηâ "+νâ "and B+→η′â "+νâ "are measured, where â "is either an electron or a muon, using a data sample of 711 fb-1 containing 772×106BB¯ pairs collected at the I (4S) resonance with the Belle detector at the KEKB asymmetric-energy e+e-collider. To reduce the dependence of the result on the form factor model, the measurement is performed over the entire q2 range. The resulting branching fractions are B(B+→ηâ "+νâ ")=(2.83±0.55(stat.)±0.34(syst.))×10-5 and B(B+→η′â "+νâ ")=(2.79±1.29(stat.)±0.30(syst.))×10-5.
Improved Measurement Of Neutrino Oscillation Parameters By The Nova Experiment,
2022
Universidad del Atlántico, Colombia
Improved Measurement Of Neutrino Oscillation Parameters By The Nova Experiment, M. A. Acero, P. Adamson, L. Aliaga, N. Anfimov, A. Antoshkin, E. Arrieta-Diaz, L. Asquith, A. Aurisano, A. Back, C. Backhouse, M. Baird, N. Balashov, P. Baldi, B. A. Bambah, S. Bashar, K. Bays, R. Bernstein, V. Bhatnagar, D. Bhattarai
Faculty and Student Publications
We present new νμ→νe, νμ→νμ, ν¯μ→ν¯e, and ν¯μ→ν¯μ oscillation measurements by the NOvA experiment, with a 50% increase in neutrino-mode beam exposure over the previously reported results. The additional data, combined with previously published neutrino and antineutrino data, are all analyzed using improved techniques and simulations. A joint fit to the νe, νμ, ν¯e, and ν¯μ candidate samples within the 3-flavor neutrino oscillation framework continues to yield a best-fit point in the normal mass ordering and the upper octant of the θ23 mixing angle, with Δm322=(2.41±0.07)×10-3 eV2 and sin2θ23=0.57-0.04+0.03. The data disfavor combinations of oscillation parameters that give rise to …
Tess Discovery Of A Sub-Neptune Orbiting A Mid-M Dwarf Toi-2136,
2022
Swarthmore College
Tess Discovery Of A Sub-Neptune Orbiting A Mid-M Dwarf Toi-2136, T. Gan, A. Soubkiou, S. X. Wang, Z. Benkhaldoun, S. Mao, É. Artigau, P. Fouqué, L. Arnold, S. Giacalone, C. A. Theissen, C. Aganze, A. Burgasser, K. A. Collins, A. Shporer, K. Barkaoui, M. Ghachoui, S. B. Howell, C. Lamman, O. D. S. Demangeon, A. Burdanov, C. Cadieux, J. Chouqar, K. I. Collins, N. J. Cook, L. Delrez, B.-O. Demory, R. Doyon, G. Dransfield, C. D. Dressing, E. Ducrot, J. Fan, L. Garcia, H. Gill, M. Gillon, C. L. Gnilka, Y. Gómez Maqueo Chew, M. N. Günther, C. E. Henze, C. X. Huang, E. Jehin, Eric L.N. Jensen, Z. Lin, N. Manset, J. Mccormac, C. A. Murray, P. Niraula, P. P. Pedersen, F. J. Pozuelos, D. Queloz, B. V. Rackham, A. B. Savel, N. Schanche, R. P. Schwarz, D. Sebastian, S. Thompson, M. Timmermans, A. H. M. J. Triaud, M. Vezie, R. D. Wells, J. De Wit, G. R. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. N. Winn, J. M. Jenkins
Physics & Astronomy Faculty Works
We present the discovery of TOI-2136 b, a sub-Neptune planet transiting a nearby M4.5V-type star every 7.85 d, identified through photometric measurements from the Transiting Exoplanet Survey Satellite (TESS) mission. The host star is located 33 pc away with a radius of R* = 0.34 ± 0.02 R⊙, a mass of 0.34 ± 0.02 M⊙, and an effective temperature of 3342 ± 100 K. We estimate its stellar rotation period to be 75 ± 5 d based on archival long-term photometry. We confirm and characterize the planet based on a series of ground-based multiwavelength …
Near-Infrared Accretion Signatures From The Circumbinary Planetary-Mass Companion Delorme 1 (Ab)B,
2022
University of Massachusetts Amherst
Near-Infrared Accretion Signatures From The Circumbinary Planetary-Mass Companion Delorme 1 (Ab)B, S. K. Betti, K. B. Follette, K. Ward-Duong, Y. Aoyama, G. D. Marleau, J. Bary, C. Robinson, M. Janson, W. Balmer, G. Chauvin, P. Palma-Bifani
Astronomy: Faculty Publications
Accretion signatures from bound brown dwarf and protoplanetary companions provide evidence for ongoing planet formation, and accreting substellar objects have enabled new avenues to study the astrophysical mechanisms controlling the formation and accretion processes. Delorme 1 (AB)b, a ?1/430-45 Myr circumbinary planetary-mass companion, was recently discovered to exhibit strong Hα emission. This suggests ongoing accretion from a circumplanetary disk, somewhat surprising given canonical gas disk dispersal timescales of 5-10 Myr. Here, we present the first NIR detection of accretion from the companion in Paβ, Pa?3, and Br?3 emission lines from SOAR/TripleSpec 4.1, confirming and further informing its accreting nature. The …
The Tess Grand Unified Hot Jupiter Survey. I. Ten Tess Planets,
2022
Swarthmore College
The Tess Grand Unified Hot Jupiter Survey. I. Ten Tess Planets, S. W. Yee, J. N. Winn, J. D. Hartman, J. E. Rodriguez, G. Zhou, S. N. Quinn, D. W. Latham, A. Bieryla, K. A. Collins, B. C. Addison, I. Angelo, K. Barkaoui, P. Benni, A. W. Boyle, R. Brahm, R. P. Butler, D. R. Ciardi, K. I. Collins, D. M. Conti, J. D. Crane, F. Dai, C. D. Dressing, J. D. Eastman, Z. Essack, R. Forés-Toribio, E. Furlan, T. Gan, S. Giacalone, H. Gill, E. Girardin, T. Henning, C. E. Henze, M. J. Hobson, J. Horner, A. W. Howard, S. B. Howell, C. X. Huang, H. Isaacson, J. M. Jenkins, Eric L.N. Jensen, A. Jordán, S. R. Kane, J. F. Kielkopf, S. Lasota, A. M. Levine, J. Lubin, A. W. Mann, B. Massey, K. K. Mcleod, M. W. Mengel, J. A. Muñoz, F. Murgas, E. Palle, P. Plavchan, A. Popowicz, D. J. Radford, G. R. Ricker, P. Rowden, B. S. Safonov, A. B. Savel, R. P. Schwarz, S. Seager, R. Sefako, A. Shporer, G. Srdoc, I. S. Strakhov, J. K. Teske, C. G. Tinney, D. Tyler, R. A. Wittenmyer, H. Zhang, C. Ziegler
Physics & Astronomy Faculty Works
Hot Jupiters—short-period giant planets—were the first extrasolar planets to be discovered, but many questions about their origin remain. NASA's Transiting Exoplanet Survey Satellite (TESS), an all-sky search for transiting planets, presents an opportunity to address these questions by constructing a uniform sample of hot Jupiters for demographic study through new detections and unifying the work of previous ground-based transit surveys. As the first results of an effort to build this large sample of planets, we report here the discovery of 10 new hot Jupiters (TOI-2193A b, TOI-2207b, TOI-2236b, TOI-2421b, TOI-2567b, TOI-2570b, TOI-3331b, TOI-3540A b, TOI-3693b, TOI-4137b). All of the planets …
