|
|
|
题名
|
作者
|
年代
|
出处
|
被引量
|
| 1 | 西洋蓍草提取物对糖尿病大鼠的β细胞保护活性及降糖、降脂作用(英文)显示文摘AIM:To evaluate the therapeutic uses of Achillea millifolium in diabetic rats.METHODS:Diabetes was induced bysingle intraperitoneal injection of freshly prepared solution of alloxan monohydrate(150 mg·kg.1 body weight) in Wistar rats of150.200 g body weight.In this study,the aqueous and methanolic extract of Achillea millifolium was studied for its hypoglycemic andhypolipidemic properties.The rats were divided into several groups,serving as Normal group,Diabetic Control group,Diabetictreated with glibenclamide,and extract treated groups.The blood serum collected from the various groups of rats was analysed for itsvarious biochemical parameters like glucose,cholesterol,triglycerides,VLDL,SGOT,SGPT and ALP.On the 14th day of the experimentthe rats were scarified and pancreas was collected for histopathological studies.RESULTS:The extracts at dose levels of 250and 500 mg·kg.1 body weight showed significant(P ≤ 0.05) decrease in blood glucose level,TGL,VLDL,cholesterol,SGOT,SGPT,and ALP in diabetic rats.The extracts prevented the β-cells of pancreas from the cytotoxic effects of Alloxan monohydrate.CONCLUSION:The results indicate that the extracts as mentioned above are effective in hyperglycemia and can effectively protectagainst other metabolic aberrations caused by alloxan monohydrate. | Khalid G.Mustafa Bashir A.Ganai Seema Akbar Mohamad Y.Dar Akbar Masood | 2012 | 中国天然药物2012，10，3： | 3 |
| 2 | Exploring physical features of anisotropic quark stars in Brans-Dicke theory with a massive scalar field via embedding approach显示文摘The main aim of this study is to explore the existence and salient features of spherically symmetric relativistic quark stars in the background of massive Brans-Dicke gravity.The exact solutions to the modified Einstein field equations are derived for specific forms of coupling and scalar field functions using the equation of state relating to the strange quark matter that stimulates the phenomenological MIT-Bag model as a free Fermi gas of quarks.We use a well-behaved function along with the Karmarkar condition for class-one embedding as well as junction conditions to determine the unknown metric tensors.The radii of strange compact stars viz.,PSR J1416-2230,PSR J1903+327,4U 1820-30,CenX-3,and EXO1785-248,are predicted via their observed mass for different values of the massive Brans-Dicke parameters.We explore the influences of the mass of scalar field m_(ϕ),coupling parameter ωBD,and bag constant B on state determinants and perform several tests on the viability and stability of the constructed stellar model.Conclusively,we find that our stellar system is physically viable and stable as it satisfies all the energy conditions and necessary stability criteria under the influence of a gravitational scalar field. | Abdelghani Errehymy G.Mustafa Youssef Khedif Mohammed Daoud | 2022 | Chinese Physics C2022，46，4： | 0 |
| 3 | Shadows and gravitational weak lensing by the Schwarzschild black hole in the string cloud background with quintessential field显示文摘In this study,we observe that,in the presence of the string cloud parameter a and the quintessence parameterγ,with the equation of state parameter,ω_(q) = -2/3the radius of the shadow of the Schwarzschild black hole increases as compared with that in the pure Schwarzschild black hole case.The existence of both quintessential dark energy and the cloud of strings increases the shadow size;hence,the strength of the gravitational field around the Schwarzschild black hole increases.Using the data collected by the Event Horizon Telescope(EHT)collaboration for M87*and Sgr A*,we obtain upper bounds on the values of a andγ.Further,we see the effects of a andγon the rate of emission energy for the Schwarzschild black hole.We notice that the rate of emission energy is higher in the presence of clouds of strings and quintessence.Moreover,we study the weak deflection angle using the Gauss-Bonnet theorem.We show the influence of a andγon the weak deflection angle.We notice that both a andγincrease the deflection angleα. | G.Mustafa Farruh Atamurotov Ibrar Hussain Sanjar Shaymatov Ali Övgün | 2022 | Chinese Physics C2022，46，12： | 0 |
| 4 | Anisotropic stellar structures in the f(T)theory of gravity with quintessence via embedding approach显示文摘This work suggests a new model for anisotropic compact stars with quintessence in f(T)gravity by us-ing the off-diagonal tetrad and the power-law as f(T)=βT^(n),where T is the scalar torsion andβand n are real con-stants.The acquired field equations incorporating the anisotropic matter source along with the quintessence field,in f(T)gravity,are investigated by making use of the specific character of the scalar torsion T for the observed stars PSRJ1614-2230,4U1608-52.CenX-3,EXO1785-248,and SMCX-1.It is suggested that all the stellar struc-tures under examination are advantageously independent of any central singularity and are stable.Comprehensive graphical analysis shows that various physical features which are crucially important for the emergence of the stellar structures are conferred. | Allah Ditta Mushtaq Ahmad Ibrar Hussain G.Mustafa | 2021 | Chinese Physics C2021，45，4： | 0 |
| 5 | Thermal analysis and Joule-Thomson expansion of black hole exhibiting metric-affine gravity显示文摘This study examines a recently hypothesized black hole,which is a perfect solution of metric-affine gravity with a positive cosmological constant,and its thermodynamic features as well as the Joule-Thomson expansion.We develop some thermodynamical quantities,such as volume,Gibbs free energy,and heat capacity,using the entropy and Hawking temperature.We also examine the first law of thermodynamics and thermal fluctuations,which might eliminate certain black hole instabilities.In this regard,a phase transition from unstable to stable is conceivable when the first law order corrections are present.In addition,we study the efficiency of this system as a heat engine and the effect of metric-affine gravity for the physical parameters q_(e),q_(m),κ_(s),κ_(d),and κ_(sh).Further,we study the Joule-Thomson coefficient and inversion temperature,and observe the isenthalpic curves in the Ti−Pi plane.In metric-affine gravity,a comparison is made between a van der Waals fluid and a black hole to study their similarities and differences. | Muhammad Yasir 夏铁成 Faisal Javed G.Mustafa | 2024 | Chinese Physics C2024，48，1： | 0 |
您所在的机构暂未开通此部分的功能，请联系管理员