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241
Estandarización de un modelo para inducir obesidad en ratas
Published 2013-10-01Subjects: “…ratas wistar…”
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242
¿Ser o estar “queer” en Latinoamérica? El devenir emancipador en: Lemebel, Perlongher y Arenas
Published 2011-01-01“…Sus creaciones contestan los modelos importados tanto de análisis teórico como de formas de ser disidente y reivindican la importancia social del amor. Ser/estar queer en América Latina sugiere entonces una suerte de des-identidad, un devenir-incesante, siempretransgresor, siempre-auto-emancipador. …”
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243
Pengembangan media pembelajaran video untuk meningkatkan hasil belajar materi geometri bangun datar kelas IV
Published 2022-06-01Subjects: Get full text
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244
Ser Pai, Estar Preso: Vivências e Sentidos da Paternidade em Presídios no Rio de Janeiro
Published 2024-12-01Get full text
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245
Hankel Determinants for the Logarithmic Coefficients of a Subclass of Close-to-Star Functions
Published 2024-01-01“…Suppose that ST1 is a class of close-to-star functions. In this paper, we investigated the estimate of Zalcman functional on the logarithmic coefficients and the third Hankel determinant for the class ST1 with the determinant entry of logarithmic coefficients. …”
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246
Hierarchical Classification of Variable Stars Using Deep Convolutional Neural Networks
Published 2022-04-01Subjects: “…variable stars…”
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247
Multicolor Ramsey numbers and star-critical Ramsey numbers involving fans
Published 2025-01-01Get full text
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248
Research on Load Characteristic of Star Gear Transmission System of Turbofan Engine
Published 2021-06-01“…A gear rotor bearing coupling dynamics model is established for the star gear transmission system of geared turbofan engine(GTF). …”
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249
Effect of Generalized Uncertainty Principle on Main-Sequence Stars and White Dwarfs
Published 2015-01-01“…Astrophysical objects such as main-sequence stars and white dwarfs are examined and discussed as an application. …”
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250
The Main Ionization Sources of Gas in Several Nearby Star Forming Galaxies
Published 2021-03-01“…In intermediate cases, when the contributions of radiation from OB stars and from shock waves mix, the identification becomes uncertain. …”
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251
Analysis of the Conformally Flat Approximation for Binary Neutron Star Initial Conditions
Published 2017-01-01“…The spatially conformally flat approximation (CFA) is a viable method to deduce initial conditions for the subsequent evolution of binary neutron stars employing the full Einstein equations. Here we analyze the viability of the CFA for the general relativistic hydrodynamic initial conditions of binary neutron stars. …”
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252
The Fault in our Stars – Starry-coloured Halos in Occipital Lobe Infarct
Published 2024-12-01“…She also complained of seeing multi-coloured rings in a star pattern, each episode lasting for 10 to 15 min. …”
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253
Can Effects of a Generalized Uncertainty Principle Appear in Compact Stars?
Published 2024-12-01“…The corresponding results for the equation of state and the mass-radius relation for neutron stars are in tune with recent observations with a maximum mass around 2.5 M<sub>⊙</sub> and radius close to 12 km. …”
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254
Thermal and Mechanical Properties of Biodegradable Star-Shaped/Linear Polylactide Stereocomplexes
Published 2015-01-01“…The 6-arm star-shaped poly(L-lactide) (6PLL)/linear poly(D-lactide) (1PDL) stereocomplex films were prepared by the solvent casting method. …”
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255
Identifying Hierarchically Triple Star Systems with Gaia DR3 and LAMOST
Published 2025-01-01Subjects: Get full text
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256
Ultraviolet Photometry and Habitable Zones of over 2700 Planet-hosting Stars
Published 2025-01-01“…The Sun’s low FUV emission and moderate NUV emission highlight its uniqueness among (solar-like) stars.…”
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257
The S4G-WISE View of Global Star Formation in the Nearby Universe
Published 2025-01-01Subjects: “…Star formation…”
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258
Magnetized Protoplanetary Disks around Young Stars in the Presence of Realistic Cooling
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259
Joint beamforming optimization algorithm for secure cognitive radio based on STARS
Published 2024-03-01“…Secure cognitive radio (SCR) system based on reconfigurable intelligent surface (RIS) assumes that secondary user (SU) and primary user (PU) locate on the same side of the base station (BS), which can only cover part of the communication area and limits the deployment flexibility and effectiveness of the RIS.In order to solve the above problem, a new SCR system based on simultaneously transmitting and reflecting surface (STARS) was proposed.In the system, STARS could achieve full coverage of communication area, improve the received signal strength of the SU with the transmission beamforming vector and reduce the interference of the SU to the PU with the reflection beamforming vector, which provided new optimization degree of freedom (DoF) for the design of the SCR system.Considering secrecy rate constraint of the SU, interference power constraint (IPC) of the PU and transmission/reflection parameters constraint of the STARS, BS active beamforming vector and STARS transmission/reflection beamforming vectors were jointly optimized to minimize the BS’s transmit power from the perspective of reducing the total power consumption of the system.The minimization problem is a variable coupling non-convex problem, which is difficult to tackle directly.An alternating optimization (AO) algorithm based on difference-of-convex relaxation (DCR) method and sequential rank-one constraint relaxation (SROCR) method was proposed to jointly design the BS active beamforming vector and STARS transmission/reflection beamforming vectors.Simulation results show that the proposed algorithm has good convergence performance and effectively reduces the interference of SU on PU.Compared with the traditional RIS, random phase, maximum-ratio transmission (MRT) and equal energy splitting (Equal ES) schemes, the BS transmitting power is reduced by 8.3%, 15.4%, 5.9% and 5.3%, respectively.…”
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260
GR-Athena++: General-relativistic Magnetohydrodynamics Simulations of Neutron Star Spacetimes
Published 2025-01-01Subjects: “…Compact binary stars…”
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