neutron

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Selected Aspects of Neutron Decay

标签:文库时间:2024-09-13
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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

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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

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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

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arXiv:0805.1062v1 [cond-mat.supr-con] 7 May 2008

NISTCenterforNeutronResearch,NationalInstituteof

Gamma-ray bursts and density evolution of neutron star binary mergers

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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

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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

标签:文库时间:2024-09-13
【bwwdw.com - 博文网】

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