Quasi-spherical

Gravitational collapse in (n+2) dimensional quasi-spherical space-time is studied for a fluid with non vanishing radial pressure. An exact analytic solution is obtained (ignoring the arbitrary integration function) for the equation of state $p_{r}=(\gamma-

Gravitational collapse in (n+2) dimensional quasi-spherical space-time is studied for a fluid with non vanishing radial pressure. An exact analytic solution is obtained (ignoring the arbitrary integration function) for the equation of state $p_{r}=(\gamma-

Gravitational col

Quasi-Contract

准合同

1 The term ‘quasi-contract’, once used to describe the area of law now called ‘restitution’ or ‘unjust enrichment’, is now out of favour. ‘Quasi-contract’ says only that the matter is not contract. So far as it suggests that there is a sort of contract, it deceives, unintelligibly. Quasi-contractual liability should be understood not as part of unjust enrichment, but as a different basis of liability that can help us see what liability for unjust enrichment might be: liability grounded in notions of fairn

LDPC码

IEEECOMMUNICATIONSLETTERS,VOL.9,NO.9,SEPTEMBER2005823

ACombiningMethodofQuasi-CyclicLDPCCodesbytheChineseRemainderTheorem

SehoMyungandKyeongcheolYang,Member,IEEE

Abstract—Inthispaperweproposeamethodofconstructingquasi-cycliclow-densityparity-check(QC-LDPC)codesoflargelengthbycombiningQC-LDPCcodesofsmalllengthastheircomponentcodes,viatheChineseRemainderTheorem.ThegirthoftheQC-LDPCcodesobtainedbytheproposedmethodisalwayslargerthanorequaltothatofeachcomponentcode.Byapplyingthemethodtoarraycodes,wepresentafamilyofhigh-ratereg

Precise energies of rovibrational states of the exotic hydrogen-like molecule $(dt\mu)Xee$ are of importance for $dt\mu$ resonant formation, which is a key process in the muon-catalyzed fusion cycle. The effect of the internal structure and motion of the $

E ectofdtµquasi-nucleusstructureonenergylevelsofthe

(dtµ)Xeeexoticmolecule

arXiv:physics/0403116v2 [physics.atom-ph] 31 Mar 2004O.I.Kartavtsev,1A.V.Malykh,1,2andV.P.Permyakov31DzhelepovLaboratoryofNuclearProblems,JointInstituteforNuclearResearch,Dubna,141980,Russ

Using large number of Rossi X-ray Time Explorer observations of Sco X-1 we present a detailed investigation of the transition layer (TL) and the relativistic precession (RP) models. These models predict the existence of the invariant quantities: an inclina

THEASTROPHYSICALJOURNAL,571:L000,2002JUNE1

APreprinttypesetusingLTEXstyleemulateapjv.11/12/01

CANANY“INVARIANTS”BEREVEALEDINQUASI-PERIODICPHENOMENAOBSERVEDFROM

SCOX-1?

SERGEYKUZNETSOV1

Received2002February25;Accepted2002April19

AND

LEVTITARCHUK2,3

arXiv:astro-ph/0204456v1 26 Apr