The compact spinning with pneumatic groove utilizes transverse air force and mechanical force of the pneumatic groove to condense fiber bundles to eliminate the spinning triangle.Range analysis and variance analysis o...The compact spinning with pneumatic groove utilizes transverse air force and mechanical force of the pneumatic groove to condense fiber bundles to eliminate the spinning triangle.Range analysis and variance analysis of orthogonal experiment were used to discover both important and general factors that influence the condensing effect of the compact yarn including negative pressure,traveler,roving moisture regain,and spinning tension.Results from this research have confirmed that the spinning tension is the most important factor affecting the condensing effect and the yarn quality;the negative pressure,traveler,and roving moisture regain are general factors.The optimal combination for producing least yarn hairiness,A3B2C1D1,is acquired,where the value of negative pressure A is -3.0 kPa,roving moisture regain B is 7.64%,traveler C is 20 #(yarn tex 20.8),and spinning tension D is 25 cN.展开更多
Sufficient conditions are given to assert that two differentiable mappings between Banach spaces have common values. The proof is essentially based upon continuation methods.
In this work we present a theoretical framework within Einstein’s classical general relativity which models stellar compact objects such as PSR J1614-2230 and SAX J1808.4-3658.The Einstein field equations are solved ...In this work we present a theoretical framework within Einstein’s classical general relativity which models stellar compact objects such as PSR J1614-2230 and SAX J1808.4-3658.The Einstein field equations are solved by assuming that the interior of the compact object is described by a class I spacetime.The so-called Karmarkar condition arising from this requirement is integrated to reduce the gravitational behaviour to a single generating function.By appealing to physics we adopt a form for the gravitational potential which is sufficiently robust to accurately describe compact objects.Our model satisfies all the requirements for physically realistic stellar structures.展开更多
Let ∑be a C^3 compact symmetric convex hypersurface in R^8.We prove that when ∑ carries exactly four geometrically distinct closed characteristics,then all of them must be symmetric.Due to the example of weakly non-...Let ∑be a C^3 compact symmetric convex hypersurface in R^8.We prove that when ∑ carries exactly four geometrically distinct closed characteristics,then all of them must be symmetric.Due to the example of weakly non-resonant ellipsoids,our result is sharp.展开更多
基金National Key Technologies R&D Program of China during the 11th Five-Year Plan Period(No.2007BAE41B04)
文摘The compact spinning with pneumatic groove utilizes transverse air force and mechanical force of the pneumatic groove to condense fiber bundles to eliminate the spinning triangle.Range analysis and variance analysis of orthogonal experiment were used to discover both important and general factors that influence the condensing effect of the compact yarn including negative pressure,traveler,roving moisture regain,and spinning tension.Results from this research have confirmed that the spinning tension is the most important factor affecting the condensing effect and the yarn quality;the negative pressure,traveler,and roving moisture regain are general factors.The optimal combination for producing least yarn hairiness,A3B2C1D1,is acquired,where the value of negative pressure A is -3.0 kPa,roving moisture regain B is 7.64%,traveler C is 20 #(yarn tex 20.8),and spinning tension D is 25 cN.
文摘Sufficient conditions are given to assert that two differentiable mappings between Banach spaces have common values. The proof is essentially based upon continuation methods.
文摘In this work we present a theoretical framework within Einstein’s classical general relativity which models stellar compact objects such as PSR J1614-2230 and SAX J1808.4-3658.The Einstein field equations are solved by assuming that the interior of the compact object is described by a class I spacetime.The so-called Karmarkar condition arising from this requirement is integrated to reduce the gravitational behaviour to a single generating function.By appealing to physics we adopt a form for the gravitational potential which is sufficiently robust to accurately describe compact objects.Our model satisfies all the requirements for physically realistic stellar structures.
基金Hui Liu Partially supported by NSFC(No.11401555)China Postdoctoral Science Foundation No.2014T70589,CUSF(No.WK0010000037)Yiming Long Partially supported by NSFC。
文摘Let ∑be a C^3 compact symmetric convex hypersurface in R^8.We prove that when ∑ carries exactly four geometrically distinct closed characteristics,then all of them must be symmetric.Due to the example of weakly non-resonant ellipsoids,our result is sharp.
