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Relation between Mass and Radius of Exoplanets Distinguished by their Density
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作者 Alberto S.Betzler JoséG.V.Miranda 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2023年第6期47-55,共9页
The formation of the solar system has been studied since the 18th century and received a boost in 1995 with the discovery of the first exoplanet,51 Pegasi b.The investigations increased the number of confirmed planets... The formation of the solar system has been studied since the 18th century and received a boost in 1995 with the discovery of the first exoplanet,51 Pegasi b.The investigations increased the number of confirmed planets to about5400 to date.The possible internal structure and composition of these planets can be inferred from the relationship between planet mass and radius,M-R.We have analyzed the M-R relation of a selected sample of iron-rock and ice-gas planets using a fractal approach to their densities.The application of fractal theory is particularly useful to define the physical meaning of the proportionality constant and the exponent in an empirical M-R power law in exoplanets,but this does not necessarily mean that they have an internal fractal structure.The M-R relations based on this sample are M=(1.46±0.08)R^(2.6±0.2)for the rocky population(3.6≤ρ≤14.3 g cm^(-3)),with 1.5≤M≤39M_(⊕),and M=(0.27±0.04)R^(2.7±0.2)for ice-gas planets(0.3≤ρ≤2.1 g cm^(-3))with 5.1≤M≤639 M_(⊕)(or■2 M_(J))and orbital periods greater than 10 days.Both M-R relations have in their density range a great predictive power for the determination of the mass of exoplanets and even for the largest icy moons of the solar system.The average fractal dimension of these planets is D=2.6±0.1,indicating that these objects likely have a similar degree of heterogeneity in their densities and a nearly similar composition in each sample.The M-R diagram shows a"gap"between ice-gas and iron-rock planets.This gap is a direct consequence of the density range of these two samples.We empirically propose an upper mass limit of about 100 M_(⊕),so that an M-R relation for ice-gas planets in a narrow density range is defined by M∝R^(3). 展开更多
关键词 planets and satellites:formation planets and satellites:terrestrial planets planets and satellites:gaseous planets
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棒与星系整体恒星形成性质关系的统计研究
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作者 穆子豪 沈世银 +1 位作者 Rafael S.de Souza Ana L.Chies-Santos 《天文学进展》 CSCD 北大核心 2024年第1期115-127,共13页
盘状星系中的棒结构特征与星系自身所处环境及整体恒星形成特征之间存在复杂的相互关系。利用细致的星系形态特征测量计划Galaxy Zoo DECaLS中的数据构建了一组目前最大的具有同样恒星质量分布的强棒、弱棒和无棒星系样本。通过引入星... 盘状星系中的棒结构特征与星系自身所处环境及整体恒星形成特征之间存在复杂的相互关系。利用细致的星系形态特征测量计划Galaxy Zoo DECaLS中的数据构建了一组目前最大的具有同样恒星质量分布的强棒、弱棒和无棒星系样本。通过引入星系所处暗晕质量及相空间特征来控制星系所处的环境效应之后,进一步对比研究强棒、弱棒和无棒星系的恒星形成特征。研究表明,有棒星系中的恒星形成熄灭的比例系统地高于无棒星系,且强棒的效应更为明显。但是,对于仍处于恒星形成主序上的星系来说,强棒、弱棒和无棒星系的恒星形成特征并没有显著差别。以上结果表明,星系中的棒特征在其存在的时标中可能使部分星系迅速地从恒星形成转入熄灭状态。 展开更多
关键词 棒旋星系 恒星形成 环境
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Possible Connections between X-Solar Flares and Worldwide Variation in Seismicity Enhancement 被引量:6
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作者 Marilia Hagen Anibal Azevedo 《Natural Science》 2017年第12期457-476,共20页
We developed a?statistical study analyzing global seismicity enhancement and its variation?overtwenty years.?X-flares sometimes occur in conjunction with Coronal Mass Ejections (CME),which make their connection with t... We developed a?statistical study analyzing global seismicity enhancement and its variation?overtwenty years.?X-flares sometimes occur in conjunction with Coronal Mass Ejections (CME),which make their connection with the Earth’s magnetosphere stronger.?The preliminary study divided the Earth into seven regions determined by longitude and latitude, and nine levels of depth valid for most locations?in the?Pacific area.?The results showed that X beams influenced seismicity in terrestrial localities, mainly high magnitude earthquakes occurring below the crust at 70 km.?These internal enhancements happen without the presence of any external forces such as studied in Solar Speed Winds.?Nevertheless, those variations are perceptible in the presence of intense X flares and CME and less observed in the periods during which flares were absent. Two cases of high magnitude earthquakes in recent?years are analyzed, and the extreme external conditions of those events fit?with this theory. 展开更多
关键词 Sun Solar Wind CORONAL Mass Ejections X-Flares EARTHQUAKES
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Condensed Extended Hyper-Wiener Index 被引量:2
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作者 李新华 Abraham F.Jalbout 吉智 《Chinese Journal of Structural Chemistry》 SCIE CAS CSCD 北大核心 2008年第9期1134-1140,共7页
According to the definitions of molecular connectivity and hyper-Wiener index, a novel set of hyper-Wiener indexes (Dn, ^mDn) were defined and named as condensed extended hyper-Wiener index, the potential usefulness... According to the definitions of molecular connectivity and hyper-Wiener index, a novel set of hyper-Wiener indexes (Dn, ^mDn) were defined and named as condensed extended hyper-Wiener index, the potential usefulness of which in QSAR/QSPR is evaluated by its correlation with a number of C3-C8 alkanes as well as by a favorable comparison with models based on molecular connectivity index and overall Wiener index. 展开更多
关键词 hyper-Wiener index (R) condensed extended hyper-Wiener index molecular connectivity index
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Deep and Ultra-Deep Earthquakes Worldwide, Possible Anomalies in South America 被引量:3
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作者 M. Hagen A. Azevedo 《Natural Science》 2018年第6期199-213,共15页
The aim of this paper is to evaluate the worldwide variation of deep and ultra-deep earthquakes (DQ and UDQ) during the period 1996-2017. This project found only three locations around the globe presenting this kind o... The aim of this paper is to evaluate the worldwide variation of deep and ultra-deep earthquakes (DQ and UDQ) during the period 1996-2017. This project found only three locations around the globe presenting this kind of seismicity. Although there are other global settings showing deep seismicity, they are not periodical and cannot be considered by a statistical view. The three areas with intense activity for DQ and UDQ events are located mostly in subduction areas. The largest variations of DQ and UDQ border the Pacific Ocean and include the North Pacific, South Pacific, and South America. The major difference in this set is that the first two sites are subduction zones and the South American occurrences happened in the interior of the continent. Another anomaly is an internal layer between 300 - 500 km in South America that shows no tremors in the period studied. However, below 500 km activity reappears, even at extreme depths of up to 650 km. We suggested that the reason for those occurrences would be due to an anomaly in the asthenosphere in this region. This anomaly would probably be presenting a breakable material that was pushed by the Nazca platform against the South America plate. Other depths below 100 km in all the regions are discussed as well. We suggested that the reason for those occurrences was an anomaly created in the asthenosphere as part of the process of the South America collision with the Nazca plate. Part of the Nazca plate has subducted below South America, creating a slab as deep as 500 km. The convergent slab is still moving against South America and sinking due to the gravity and rotation of the Earth. The discrepancies in the occurrences we tracked at different locations indicated that this slab had different thicknesses around South America. We found similar results for Vanuatu and Fiji;in these regions UDQ events occur at the subduction zones under the ocean with depths greater than 700 km. Here, a possible explanation is that part of the lithosphere is subducted at these depths and is causing tremors. 展开更多
关键词 DEEP EARTHQUAKES (DQ) Ultra-Deep EARTHQUAKES (UDQ) South AMERICA
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Possible Connections between Seasons and Ultra-Deep Earthquakes Worldwide 被引量:2
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作者 Marilia Hagen A. Azevedo 《Natural Science》 2018年第7期288-302,共15页
The aim of this investigation is to find possible changes in ultra-deep earthquakes (UDQ) during different seasons of the year. In the acquisition of data for our previous work we observed an inexplicable pattern of g... The aim of this investigation is to find possible changes in ultra-deep earthquakes (UDQ) during different seasons of the year. In the acquisition of data for our previous work we observed an inexplicable pattern of growth of ultra-deep tremors (UDQ) during the studied period. Apparently, there is no viable explanation for growth occurring at such a level, presumably in the asthenosphere. Current research and theories developed for the inner layers of the Earth do not explain such variations. Therefore, a possible explanation would be in external factors such as the seasons of the year, which are determined by changes in the Earth’s axial tilt, and therefore the portion of the earth that is angled toward the sun. This paper focuses exclusively on UDQ events. To simplify the calculations, we consider four main locations;this includes one more region than our previous paper but includes only UDQ data. The results showed that during spring and autumn UDQ events grew slightly in both Northern and Southern Hemispheres. It is also suggested that a contributor to UDQ events is friction from the subducting lithosphere against the continental plates. 展开更多
关键词 Sun MOON Earth Ultra-Deep Quakes SEASONS
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How much has the Sun influenced Northern Hemisphere temperature trends?An ongoing debate 被引量:2
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作者 Ronan Connolly Willie Soon +20 位作者 Michael Connolly Sallie Baliunas Johan Berglund C.John Butler Rodolfo Gustavo Cionco Ana G.Elias Valery M.Fedorov Hermann Harde Gregory W.Henry Douglas V.Hoyt Ole Humlum David R.Legates Sebastian Liming Nicola Scafetta Jan-Erik Solheim Laszlo Szarka Harry van Loon Victor M.Velasco Herrera Richard C.Willson Hong Yan Weijia Zhang 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2021年第6期131-198,共68页
In order to evaluate how much Total Solar Irradiance(TSI)has influenced Northern Hemisphere surface air temperature trends,it is important to have reliable estimates of both quantities.Sixteen different estimates of t... In order to evaluate how much Total Solar Irradiance(TSI)has influenced Northern Hemisphere surface air temperature trends,it is important to have reliable estimates of both quantities.Sixteen different estimates of the changes in TSI since at least the 19th century were compiled from the literature.Half of these estimates are"low variability"and half are"high variability".Meanwhile,five largely-independent methods for estimating Northern Hemisphere temperature trends were evaluated using:1)only rural weather stations;2)all available stations whether urban or rural(the standard approach);3)only sea surface temperatures;4)tree-ring widths as temperature proxies;5)glacier length records as temperature proxies.The standard estimates which use urban as well as rural stations were somewhat anomalous as they implied a much greater warming in recent decades than the other estimates,suggesting that urbanization bias might still be a problem in current global temperature datasets-despite the conclusions of some earlier studies.Nonetheless,all five estimates confirm that it is currently warmer than the late 19th century,i.e.,there has been some"global warming"since the 19th century.For each of the five estimates of Northern Hemisphere temperatures,the contribution from direct solar forcing for all sixteen estimates of TSI was evaluated using simple linear least-squares fitting.The role of human activity on recent warming was then calculated by fitting the residuals to the UN IPCC’s recommended"anthropogenic forcings"time series.For all five Northern Hemisphere temperature series,different TSI estimates suggest everything from no role for the Sun in recent decades(implying that recent global warming is mostly human-caused)to most of the recent global warming being due to changes in solar activity(that is,that recent global warming is mostly natural).It appears that previous studies(including the most recent IPCC reports)which had prematurely concluded the former,had done so because they failed to adequately consider all the relevant estimates of TSI and/or to satisfactorily address the uncertainties still associated with Northern Hemisphere temperature trend estimates.Therefore,several recommendations on how the scientific community can more satisfactorily resolve these issues are provided. 展开更多
关键词 Sun:activity (Sun:)solar terrestrial relations (Sun:)sunspots Sun:faculae plages
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Thermoluminescence Response and Its Deconvolution on Crystalline Higher Order Mixtures of Alkali Halides Exposed to Gamma-Rays for Dosimetric Use 被引量:1
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作者 Ricardo Rodriguez Mijangosl G. Vazquez-Polo +1 位作者 R. Perez-Salas1 P. Gonzalez-Martinez 《Journal of Chemistry and Chemical Engineering》 2012年第12期1093-1098,共6页
Alkali halides crystals have been the subject of intense research. High order crystalline one phase mixtures (high order: more that binary) studied by TL (thermoluminiscence technique) proved having persistent pe... Alkali halides crystals have been the subject of intense research. High order crystalline one phase mixtures (high order: more that binary) studied by TL (thermoluminiscence technique) proved having persistent peaks along the time after the radiation to which they are exposed. In general in alkali halide crystals the traps associated with highest recorded temperature peaks in the TL due to radiation damage have greater permanence in time too. These features are useful for dosimetric applications. In this work, temperature thermoluminescence glow peaks of ternary and quaternary mixed alkali halide crystals have been studied. The study has been focused on their high temperature glow peaks after being subjected to thermal treatments at 373, 573, and 673 K. The glow peaks of high temperature were isolated and studied 24 h and 48 h after irradiation. The parameters of the recombination processes associated to these peaks were obtained using a glow peak shape method. Orders of kinetics were higher than 1.0 and the activation energy greater than 1.2 eV. The results suggest that such materials have a high potential as dosimeter and energy storage materials. 展开更多
关键词 Thermoluminiscence alkali halide mixed crystals gamma radiation dosimetry.
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Extraction of Nuclear Matter Properties from Nuclear Masses by a Model of Equation of State
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作者 K.C.Chung C.S.Wang A.J.Santiago 《Communications in Theoretical Physics》 SCIE CAS CSCD 2001年第11期583-588,共6页
The extraction of nuclear matter properties from measured nuclear masses is investigated in the energy density functional formalism of nuclei.It is shown that the volume energy a1 and the nuclear incompressibility Ko ... The extraction of nuclear matter properties from measured nuclear masses is investigated in the energy density functional formalism of nuclei.It is shown that the volume energy a1 and the nuclear incompressibility Ko depend essentially on μnN -+- pZ - 2EN,whereas the symmetry energy J and the density symmetry coefficient L as well as symmetry incompressibility Ks depend essentially on μn - μp,where μp =μp - Ec/ Z,μn and μp are the neutron and proton chemical potentials respectively,EN the nuclear energy,and Ec the Coulomb energy.The obtained symmetry energy is J = 28.5 MeV,while other coefficients are uncertain within ranges depending on the model of nuclear equation of state. 展开更多
关键词 NUCLEAR MATTER properties nuclear MATTER EQUATION of state
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Light Front Boson Model Propagation
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作者 Jorge Henrique Sales Alfredo Takashi Suzuki 《Communications in Theoretical Physics》 SCIE CAS CSCD 2011年第6期1029-1040,共12页
The scope and aim of this work is to describe the two-body interaction mediated by a particle (either the scalar or the gauge boson) within the light-front formulation. To do this, first of all we point out the impo... The scope and aim of this work is to describe the two-body interaction mediated by a particle (either the scalar or the gauge boson) within the light-front formulation. To do this, first of all we point out the importance of propagators and Green functions in Quantum Mechanics. Then we project the covariant quantum propagator onto the light front time to get the propagator for scalar particles in these coordinates. This operator propagates the wave function from x+ = 0 to x+ 〉 0. It corresponds to the definition of the time ordering operation in the light front time x+. We calculate the light-front Green's function for 2 interacting bosons propagating forward in x+. We also show how to write down the light front Green's function from the Feynman propagator and finally make a generalization to N bosons. 展开更多
关键词 insert light-front BOSONS PROPAGATION
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Raman spectroscopy for detection of imatinib in plasma: A proof of concept
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作者 Sanhita Rath Aditi Sahu +3 位作者 Vikram Gota P.G.Martínez-Torres J.L.Pichardo-Molina C.Murali Krishna 《Journal of Innovative Optical Health Sciences》 SCIE EI CAS 2015年第5期56-66,共11页
Imatinib is the standard first line treatment for chronic myeloid leukemia(CML).Owing to doserelated toxicities of Imatinib such as neutropenia,there is scope for treatment optimization through therapeutic drug monito... Imatinib is the standard first line treatment for chronic myeloid leukemia(CML).Owing to doserelated toxicities of Imatinib such as neutropenia,there is scope for treatment optimization through therapeutic drug monitoring(TDM).Trough concentration of 1g/mL is considered the therapeutic threshhold.Existing methods for the detection of Imatinib in plasma are limited by long read out time and expensive instrumentation.Hence,Raman spectroscopy was explored as a rapid and objective tool for monitoring Imatinib concentration.Three approaches:conventional Raman spectroscopy(CRS),Drop coating deposition Raman(DCDR)spectroscopy and surface-enhanced Raman spectroscopy(SERS)were employed to detect the required trough concentration of 1g/mL and above.Detection of therapeutically relevant concentrations(1g/mL)using SERS and suitable nanoparticle substrates has been demonstrated.Prospectively,rigorous validation using clinical samples is necessary to confirm the utility of this approach in routine clinical usage. 展开更多
关键词 Therapeutic drug monitoring Raman spectroscopy IMATINIB SERS DCDR chronic myeloid leukemia
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Magnetism of Cr Impurities Embedded in Cu fcc Matrix: Density Functional Calculations
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作者 Juan Ulisses Gallardo Zazueta Raul Enrique Felix Medina +2 位作者 Manuel Andres Leyva Lucero Ricardo Alberto Guirado Lopez Salvador Meza Aguilar 《材料科学与工程(中英文B版)》 2014年第8期262-267,共6页
关键词 密度泛函理论 磁性杂质 嵌入式 FCC 反铁磁耦合 等腰直角三角形 矩阵
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Seasonality Variability and Periodicities for Ultra-Deep Earthquakes Worldwide
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作者 Marilia Hagen Anibal Azevedo 《Open Journal of Earthquake Research》 2019年第1期1-18,共18页
Our last study found that deepest-depth earthquakes with larger magnitudes (M6 or above) showed seasonality, which is dependent on the area searched. The main results indicated strong evidence that the causes for the ... Our last study found that deepest-depth earthquakes with larger magnitudes (M6 or above) showed seasonality, which is dependent on the area searched. The main results indicated strong evidence that the causes for the delays in enhancements along the period investigated were due to the tectonics also, not only the season. Therefore, if the inquiry was about an area in Northern Hemisphere, the season in which the increases occurred is different than the season in the Southern Hemisphere. Also, higher latitudes in the Northern Hemisphere or around the Equator, displayed seasonality similarly where the tremors appear to increase during the Spring and Summer. This did not happen to the Southern Hemisphere where disturbances and anomalies occurred without showing much connection to the seasons in the analyzed period. However, some of the regions presented periodicities independent from the seasons. 展开更多
关键词 SEASONS SUBDUCTION Zones Earthquakes PERIODICITY South HEMISPHERE
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The AdS_(5)×S^(5) Fermionic Model
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作者 Elcio Abdalla Antonio Lima-Santos 《Journal of Modern Physics》 2014年第6期483-487,共5页
We consider the AdS5 × S5 integrable model. As it turns out, relying on well known arguments, we claim that the conformally invariant fermionic model is solvable, the resulting solution given in terms of two curr... We consider the AdS5 × S5 integrable model. As it turns out, relying on well known arguments, we claim that the conformally invariant fermionic model is solvable, the resulting solution given in terms of two current algebras realizations. 展开更多
关键词 COMPONENT Formatting STYLE STYLING INSERT
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Photoacoustic Studies of Colloidal Silica Particles after MeV Ion-Induced Shape Deformation
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作者 Ulises Morales Rosalba Castaneda-Guzman +1 位作者 Santiago Jesus Perez-Ruiz Juan Carlos Cheang Wong 《New Journal of Glass and Ceramics》 2011年第2期63-68,共6页
Ordered arrays of colloidal submicrometer-sized silica particles deposited onto silicon wafers were irradiated with MeV Si ions. The spherical silica particles turned into oblate particles as a result of the increase ... Ordered arrays of colloidal submicrometer-sized silica particles deposited onto silicon wafers were irradiated with MeV Si ions. The spherical silica particles turned into oblate particles as a result of the increase of the particle dimension perpendicular to the ion beam direction and the decrease in the parallel direction. Pulsed laser photoacoustic spectroscopy was used to study the structural changes of the silica particles after the ion-induced shape deformation. Our purpose is to correlate the mechanical vibrations generated by the pulsed laser as a function of the Si irradiation parameters: ion energy and fluence. Fast Fourier transform analysis of the photoacoustic signal was carried out in order to obtain the normal vibration modes of the system. The size, size distribution and shape of the silica particles were determined by scanning electron microscopy. Our results revealed significant structural differences between the spherical and the deformed silica particles. 展开更多
关键词 Pulsed Laser Photoacoustic Spectroscopy Silica Particles Ion Irradiation
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Cosmology of the Nambu-Jona-Lasinio Model
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作者 Leonardo Quintanar G. A. de la Macorra 《Journal of Modern Physics》 2016年第13期1777-1800,共25页
We review the Nambu and Jona-Lasinio model (NJL), proposed long time ago, in the sixties, as a fermion interaction theory with chiral symmetry. The theory is not renormalizable and presents a symmetry breaking due to ... We review the Nambu and Jona-Lasinio model (NJL), proposed long time ago, in the sixties, as a fermion interaction theory with chiral symmetry. The theory is not renormalizable and presents a symmetry breaking due to quantum effects which depends on the strength of the coupling constant. We may associate a phase transition with this symmetry breaking, leading from fermion states to a fermion condensate which can be described effectively by a scalar field. Our purpose in this paper is to exploit the interesting properties of NJL in a different context other than particle physics by studying its cosmological dynamics. We are interested in finding whether possibly the NJL model could be used to describe the still unknown dark energy and/or dark matter, from up to 95% of the energy content of the universe at present time. 展开更多
关键词 COSMOLOGY Nambu Jona Lasinio
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CEPC Technical Design Report 被引量:1
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作者 Waleed Abdallah Tiago Carlos Adorno de Freitas +1111 位作者 Konstantin Afanaciev Shakeel Ahmad Ijaz Ahmed Xiaocong Ai Abid Aleem Wolfgang Altmannshofer Fabio Alves Weiming An Rui An Daniele Paolo Anderle Stefan Antusch Yasuo Arai Andrej Arbuzov Abdesslam Arhrib Mustafa Ashry Sha Bai Yu Bai Yang Bai Vipul Bairathi Csaba Balazs Philip Bambade Yong Ban Tripamo Bandyopadhyay Shou-Shan Bao Desmond P.Barber Ayse Bat Varvara Batozskaya Subash Chandra Behera Alexander Belyaev Michele Bertucci Xiao-Jun Bi Yuanjie Bi Tianjian Bian Fabrizio Bianchi Thomas Biekotter Michela Biglietti Shalva Bilanishvili Deng Binglin Denis Bodrov Anton Bogomyagkov Serge Bondarenko Stewart Boogert Maarten Boonekamp Marcello Borri Angelo Bosotti Vincent Boudry Mohammed Boukidi Igor Boyko Ivanka Bozovic Giuseppe Bozzi Jean-Claude Brient Anastasiia Budzinskaya Masroor Bukhari Vladimir Bytev Giacomo Cacciapaglia Hua Cai Wenyong Cai Wujun Cai Yijian Cai Yizhou Cai Yuchen Cai Haiying Cai Huacheng Cai Lorenzo Calibbi Junsong Cang Guofu Cao Jianshe Cao Antoine Chance Xuejun Chang Yue Chang Zhe Chang Xinyuan Chang Wei Chao Auttakit Chatrabhuti Yimin Che Yuzhi Che Bin Chen Danping Chen Fuqing Chen Fusan Chen Gang Chen Guoming Chen Hua-Xing Chen Huirun Chen Jinhui Chen Ji-Yuan Chen Kai Chen Mali Chen Mingjun Chen Mingshui Chen Ning Chen Shanhong Chen Shanzhen Chen Shao-Long Chen Shaomin Chen Shiqiang Chen Tianlu Chen Wei Chen Xiang Chen Xiaoyu Chen Xin Chen Xun Chen Xurong Chen Ye Chen Ying Chen Yukai Chen Zelin Chen Zilin Chen Gang Chen Boping Chen Chunhui Chen Hok Chuen Cheng Huajie Cheng Shan Cheng Tongguang Cheng Yunlong Chi Pietro Chimenti Wen Han Chiu Guk Cho Ming-Chung Chu Xiaotong Chu Ziliang Chu Guglielmo Coloretti Andreas Crivellin Hanhua Cui Xiaohao Cui Zhaoyuan Cui Brunella D'Anzi Ling-Yun Dai Xinchen Dai Xuwen Dai Antonio De Maria Nicola De Filippis Christophe De La Taille Francesca De Mori Chiara De Sio Elisa Del Core Shuangxue Deng Wei-Tian Deng Zhi Deng Ziyan Deng Bhupal Dev Tang Dewen Biagio Di Micco Ran Ding Siqin Dingl Yadong Ding Haiyi Dong Jianing Dong Jing Dong Lan Dong Mingyi Dong Xu Dong Yipei Dong Yubing Dong Milos Dordevic Marco Drewes Mingxuan Du Mingxuan Du Qianqian Du Xiaokang Du Yanyan Du Yong Du Yunfei Du Chun-Gui Duan Zhe Duan Yahor Dydyshka Ulrik Egede Walaa Elmetenawee Yun Eo Ka Yan Fan Kuanjun Fan Yunyun Fan Bo Fang Shuangshi Fang Yuquan Fang Ada Farilla Riccardo Farinelli Muhammad Farooq Angeles Faus Golfe Almaz Fazliakhmetov Rujun Fei Bo Feng Chong Feng Junhua Feng Xu Feng Zhuoran Feng Zhuoran Feng Luis Roberto Flores Castillo Etienne Forest Andrew Fowlie Harald Fox Hai-Bing Fu Jinyu Fu Benjamin Fuks Yoshihiro Funakoshi Emidio Gabrielli Nan Gan Li Gang Jie Gao Meisen Gao Wenbin Gao Wenchun Gao Yu Gao Yuanning Gao Zhanxiang Gao Yanyan Gao Kun Ge Shao-Feng Ge Zhenwu Ge Li-Sheng Geng Qinglin Geng Chao-Qiang Geng Swagata Ghosh Antonio Gioiosa Leonid Gladilin Ti Gong Stefania Gori Quanbu Gou Sebastian Grinstein Chenxi Gu Gerardo Guillermo Joao Guimaraes da Costa Dizhou Guo Fangyi Guo Jiacheng Guo Jun Guo Lei Guo Lei Guo Xia Guo Xin-Heng Guo Xinyang Guo Yun Guo Yunqiang Guo Yuping Guo Zhi-Hui Guo Alejandro Gutierrez-Rodriguez Seungkyu Ha Noman Habib Jan Hajer Francois Hammer Chengcheng Han Huayong Han Jifeng Han Liang Han Liangliang Han Ruixiong Han Yang Han Yezi Han Yuanying Han Tao Han Jiankui Hao Xiqing Hao Xiqing Hao Chuanqi He Dayong He Dongbing He Guangyuan He Hong-Jian He Jibo He Jun He Longyan He Xiang He Xiao-Gang He Zhenqiang He Klaus Heinemann Sven Heinemeyer Yuekun Heng Maria A.Hernandez-Ruiz Jiamin Hong Yuenkeung Hor George W.S.Hou Xiantao Hou Xiaonan Hou Zhilong Hou Suen Hou Caishi Hu Chen Hu Dake Hu Haiming Hu Jiagen Hu Jun Hu Kun Hu Shouyang Hu Yongcai Hu Yu Hu Zhen Hu Zhehao Hua Jianfei Hua Chao-Shang Huang Fa Peng Huang Guangshun Huang Jinshu Huang Ke Huang Liangsheng Huang Shuhui Huang Xingtao Huang Xu-Guang Huang Yanping Huang Yonggang Huang Yongsheng Huang Zimiao Huang Chen Huanyuan Changgi Hua Jiaqi Hui Lihua Huo Talab Hussain Kyuyeong Hwang Ara loannisian Munawar Iqbal Paul Jackson Shahriyar Jafarzade Haeun Jang Seoyun Jang Daheng Ji Qingping Ji Quan Ji Xiaolu Ji Jingguang Jia Jinsheng Jia Xuewei Jia Zihang Ja Cailian Jiang Han Ren Jiang Houbing Jiang Jun Jiang Xiaowei Jiang Xin Jiang Xuhui Jiang Yongcheng Jiang Zhongjian Jiang Cheng Jiang Ruiqi Jiao Dapeng Jin Shan Jin Song Jin Yi Jin Junji Jis Sunghoon Jung Goran Kacarevic Eric Kajfasz Lidia Kalinovskaya Aleksei Kampf Wen Kang Xian-Wei Kang Xiaolin Kang Biswajit Karmakar Zhiyong Ke Rijeesh Keloth Alamgir Khan Hamzeh Khanpour Khanchai Khosonthongkee KhanchaiKhosonthongkee Bobae Kim Dongwoon Kim Mi Ran Kim Minsuk Kim Sungwon Kim On Kim Michael Klasen Sanghyun Ko Ivan Koop Vitaliy Kornienko Bryan Kortman Gennady Kozlov Shiqing Kuang Mukesh Kumar Chia Ming Kuo Tsz Hong Kwok Fran cois Sylvain Ren Lagarde Pei-Zhu Lai Imad Laktineh Xiaofei Lan Zuxiu Lan Lia Lavezzi Justin Lee Junghyun Lee Sehwook Lee Ge Lei Roy Lemmon longxiang Leng Sze 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Hao Zeng Ming Zeng Jian Zhai Jiyuan Zhai Xin Zhe Zhai Xi-Jie Zhan Ben-Wei Zhang Bolun Zhang Di Zhang Guangyi Zhang Hao Zhang Hong-Hao Zhang Huaqiao Zhang Hui Zhang Jialiang Zhang Jianyu Zhang Jianzhong Zhang Jiehao Zhang Jielei Zhang Jingru Zhang Jinxian Zhang Junsong Zhang Junxing Zhang Lei Zhang Lei Zhang Liang Zhang Licheng Zhang Liming Zhang Linhao Zhang Luyan Zhang Mengchao Zhang Rao Zhang Shulei Zhang Wan Zhang Wenchao Zhang Xiangzhen Zhang Xiaomei Zhang Xiaoming Zhang Xiaoxu Zhang Xiaoyu Zhang Xuantong Zhang Xueyao Zhang Yang Zhang Yang Zhang Yanxi Zhang Yao Zhang Ying Zhang Yixiang Zhang Yizhou Zhang Yongchao Zhang Yu Zhang Yuan Zhang Yujie Zhang Yulei Zhang Yumei Zhang Yunlong Zhang Zhandong Zhang Zhaoru Zhang Zhen-Hua Zhang Zhenyu Zhang Zhichao Zhang Zhi-Qing Zhang Zhuo Zhang Zhiqing Zhang Cong Zhang Tianliang Zhang Luyan Zhang Guang Zhao Hongyun Zhao Jie Zhao Jingxia Zhao Jingyi Zhao Ling Zhao Luyang Zhao Mei Zhao Minggang Zhao Mingrui Zhao Qiang Zhao Ruiguang Zhao Tongxian Zhao Yaliang Zhao Ying Zhao Yue Zhao Zhiyu Zhao Zhuo Zhao Alexey Zhemchugov Hongjuan Zheng Jinchao Zheng Liang Zheng Ran Zheng shanxi zheng Xu-Chang Zheng Wang Zhile Weicai Zhong Yi-Ming Zhong Chen Zhou Daicui Zhou Jianxin Zhou Jing Zhou Jing Zhou Ning Zhou Qi-Dong Zhou Shiyu Zhou Shun Zhou Sihong Zhou Xiang Zhou Xingyu Zhou Yang Zhou Yong Zhou Yu-Feng Zhou Zusheng Zhou Demin Zhou Dechong Zhu Hongbo Zhu Huaxing Zhu Jingya Zhu Kai Zhu Pengxuan Zhu Ruilin Zhu Xianglei Zhu Yingshun Zhu Yongfeng Zhu Xiao Zhuang Xuai Zhuang Mikhail Zobov Zhanguo Zong Cong Zou Hongying Zou 《Radiation Detection Technology and Methods》 CSCD 2024年第1期I0003-I0016,1-1091,共1105页
The Circular Electron Positron Collider(CEPC)is a large scientific project initiated and hosted by China,fostered through extensive collaboration with international partners.The complex comprises four accelerators:a 3... The Circular Electron Positron Collider(CEPC)is a large scientific project initiated and hosted by China,fostered through extensive collaboration with international partners.The complex comprises four accelerators:a 30 GeV Linac,a 1.1 GeV Damping Ring,a Booster capable of achieving energies up to 180 GeV,and a Collider operating at varying energy modes(Z,W,H,and tt).The Linac and Damping Ring are situated on the surface,while the subterranean Booster and Collider are housed in a 100 km circumference underground tunnel,strategically accommodating future expansion with provisions for a potential Super Proton Proton Collider(SPPC).The CEPC primarily serves as a Higgs factory.In its baseline design with synchrotron radiation(SR)power of 30 MW per beam,it can achieve a luminosity of 5×10^(34)cm^(-2)s^(-1)per interaction point(IP),resulting in an integrated luminosity of 13 ab^(-1)for two IPs over a decade,producing 2.6 million Higgs bosons.Increasing the SR power to 50 MW per beam expands the CEPC's capability to generate 4.3 million Higgs bosons,facilitating precise measurements of Higgs coupling at sub-percent levels,exceeding the precision expected from the HL-LHC by an order of magnitude.This Technical Design Report(TDR)follows the Preliminary Conceptual Design Report(Pre-CDR,2015)and the Conceptual Design Report(CDR,2018),comprehensively detailing the machine's layout,performance metrics,physical design and analysis,technical systems design,R&D and prototyping efforts,and associated civil engineering aspects.Additionally,it includes a cost estimate and a preliminary construction timeline,establishing a framework for forthcoming engineering design phase and site selection procedures.Construction is anticipated to begin around 2027-2028,pending government approval,with an estimated duration of 8 years.The commencement of experiments and data collection could potentially be initiated in the mid-2030s. 展开更多
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The Use of Rank Histograms and MVL Diagrams to Characterize Ensemble Evolution in Weather Forecasting 被引量:2
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作者 Jorge A.REVELLI Miguel A.RODRIGUEZ Horacio S.WIO 《Advances in Atmospheric Sciences》 SCIE CAS CSCD 2010年第6期1425-1437,共13页
Rank Histograms are suitable tools to assess the quality of ensembles within an ensemble prediction system or framework. By counting the rank of a given variable in the ensemble, we are basically making a sample analy... Rank Histograms are suitable tools to assess the quality of ensembles within an ensemble prediction system or framework. By counting the rank of a given variable in the ensemble, we are basically making a sample analysis, which does not allow us to distinguish if the origin of its variability is external noise or comes from chaotic sources. The recently introduced Mean to Variance Logarithmic (MVL) Diagram accounts for the spatial variability, being very sensitive to the spatial localization produced by infinitesimal perturbations of spatiotemporal chaotic systems. By using as a benchmark a simple model subject to noise, we show the distinct information given by Rank Histograms and MVL Diagrams. Hence, the main effects of the external noise can be visualized in a graphic. From the MVL diagram we clearly observe a reduction of the amplitude growth rate and of the spatial localization (chaos suppression), while from the Rank Histogram we observe changes in the reliability of the ensemble. We conclude that in a complex framework including spatiotemporal chaos and noise, both provide a more complete forecasting picture. 展开更多
关键词 rank histogram MVL diagram ensemble evolution noise space-time chaos forecasting
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Sun-Moon-Earth Interactions, External Factors for Earthquakes 被引量:4
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作者 M. Hagen A. Azevedo 《Natural Science》 2017年第6期162-180,共19页
The aim of this paper is to continue analyzing the interactions in the three-body system made up of the Sun, the Moon, and the Earth. First, we review new details about Moon-Earth connections, with a special focus on ... The aim of this paper is to continue analyzing the interactions in the three-body system made up of the Sun, the Moon, and the Earth. First, we review new details about Moon-Earth connections, with a special focus on mechanical forces. Following, we expand the study to consider the pair Sun-Earth, with calculations for electromagnetic forces. The objective in both cases is to know how mechanical and electromagnetic forces affect seismological events on Earth. Our calculations found that Solar Cycles have no direct interaction with earthquake variations. Instead, we established that there is an internal discrepancy for quakes below 35 km detected in some of the regions analyzed. The results indicate that geomagnetic variations must be studied next to understand their connections to earthquakes. 展开更多
关键词 Sun MOON EARTH SOLAR Wind CORONAL Mass Ejections SOLAR Cycles EARTHQUAKES
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Nucleon Finite Volume Effect and Nuclear Matter Properties in a Relativistic Mean-Field Theory 被引量:1
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作者 R. Costa A.J. Santiago +1 位作者 H. Rodrigues J. Sa Borges 《Communications in Theoretical Physics》 SCIE CAS CSCD 2006年第6X期1052-1058,共7页
Effects of excluded volume of nucleons on nuclear matter are studied, and the nuclear properties that follow from different relativistic mean-field model parametrizations are compared. We show that, for all tested par... Effects of excluded volume of nucleons on nuclear matter are studied, and the nuclear properties that follow from different relativistic mean-field model parametrizations are compared. We show that, for all tested parametrizations, the resulting volume energy al and the symmetry energy J are around the acceptable values of 16 MeV and 30 MeV, and the density symmetry L is around 100 MeV. On the other hand, models that consider only linear terms lead to incompressibility Ko much higher than expected. For most parameter sets there exists a critical point (pc, δc), where the minimum and the maximum of the equation of state are coincident and the incompressibility equals zero. This critical point depends on the excluded volume parameter r. If this parameter is larger than 0.5 fm, there is no critical point and the pure neutron matter is predicted to be bound. The maximum value for neutron star mass is 1.85M⊙, which is in agreement with the mass of the heaviest observed neutron star 4U0900-40 and corresponds to r = 0.72 fm. We also show that the light neutron star mass (1.2M⊙) is obtained for r ≌ 0.9 fro. 展开更多
关键词 nuclear matter relativistic models nuclear matter aspects of neutron stars
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