neutron
“neutron”相关的资料有哪些?“neutron”相关的范文有哪些?怎么写?下面是小编为您精心整理的“neutron”相关范文大全或资料大全,欢迎大家分享。
Selected Aspects of Neutron Decay
Precision measurements of neutron decay offer complementary access to particle physics at small distance scales or high energies. In particular they allow tests of the V-A structure of the weak interaction. Among many experimental activities which are ongo
a r
X
i
v
:h e
p
-
e x /
5
4
3
4
v
1
1
8
A
p
r
2
5
Selected Aspects of Neutron Decay Stephan Paul Physik Department E18Technische Universit¨a t M¨u nchen James Frank Strasse,D-85748Garching Precision measurements of neutron decay o?er complementary access to par-ticle physics at smal
Neutron scattering study of the oxypnictide superconductor La(O,F)FeAs
The newly discovered superconductor La(O,F)FeAs (Tc = 26 K) was investigated using the neutron scattering technique. No spin-density-wave (SDW) order was observed in the normal state nor in the superconducting state, both with and without an applied magnet
NeutronscatteringstudyoftheoxypnictidesuperconductorLaO0.87F0.13FeAs
Y.Qiu,1,2M.Kofu,3WeiBao,4, S.-H.Lee,3Q.Huang,1T.Yildirim,1J.R.D.Copley,1J.W.Lynn,1T.Wu,5G.Wu,5andX.H.Chen5
1
arXiv:0805.1062v1 [cond-mat.supr-con] 7 May 2008
NISTCenterforNeutronResearch,NationalInstituteof
Gamma-ray bursts and density evolution of neutron star binary mergers
The evolution of the comoving cosmic merger-rate density of neutron star binaries n_c(z) is calculated using a distribution of their merging times provided by population-synthesis computations of binary stars. We adopt an exponential law for the star forma
A&Amanuscriptno.
(willbeinsertedbyhandlater)
8
991 ebF 9 1v4902089/hp-ortsa:viXra1.Introduction
Therecentdiscoveriesofopticalcounterpartsoftheγ-rayburstsGRB970228(Grootetal.1997)andGRB970508(Bond1997)andthemeasuredemission-lineredshiftofz=0.853(Metzgeretal.1997)forthelatt
Gamma-ray bursts and density evolution of neutron star binary mergers
The evolution of the comoving cosmic merger-rate density of neutron star binaries n_c(z) is calculated using a distribution of their merging times provided by population-synthesis computations of binary stars. We adopt an exponential law for the star forma
A&Amanuscriptno.
(willbeinsertedbyhandlater)
8
991 ebF 9 1v4902089/hp-ortsa:viXra1.Introduction
Therecentdiscoveriesofopticalcounterpartsoftheγ-rayburstsGRB970228(Grootetal.1997)andGRB970508(Bond1997)andthemeasuredemission-lineredshiftofz=0.853(Metzgeretal.1997)forthelatt