On stage V recovery in VIa b.c.c. metals

B. M. Pandé; G. Goedemé; L. Stals; J. Nihoul

doi:10.1080/00337577008235016

On stage V recovery in VIa b.c.c. metals

B. M. Pandé
, G. Goedemé
, L. Stals
, J. Nihoul

Research output › peer-review

Abstract

A resistometric study at 4. 2 K of the high temperature recovery spectrum of neutron- irradiated molybdenum as a function of fast fluence and of cold- worked molybdenum as a function of the heating program, yields evidence against vacancy migration in the 0. 31 Tm stage for VIa bcc metals.

Original language	English
Pages (from-to)	153-155
Number of pages	3
Journal	Radiation Effects
Volume	5
Issue number	3-4
DOIs	https://doi.org/10.1080/00337577008235016
State	Published - 1 Jan 1970

ASJC Scopus subject areas

General Engineering

Access to Document

10.1080/00337577008235016

Cite this

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title = "On stage V recovery in VIa b.c.c. metals",

abstract = "A resistometric study at 4. 2 K of the high temperature recovery spectrum of neutron- irradiated molybdenum as a function of fast fluence and of cold- worked molybdenum as a function of the heating program, yields evidence against vacancy migration in the 0. 31 Tm stage for VIa bcc metals.",

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AU - Goedemé, G.

AU - Stals, L.

AU - Nihoul, J.

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Y1 - 1970/1/1

N2 - A resistometric study at 4. 2 K of the high temperature recovery spectrum of neutron- irradiated molybdenum as a function of fast fluence and of cold- worked molybdenum as a function of the heating program, yields evidence against vacancy migration in the 0. 31 Tm stage for VIa bcc metals.

AB - A resistometric study at 4. 2 K of the high temperature recovery spectrum of neutron- irradiated molybdenum as a function of fast fluence and of cold- worked molybdenum as a function of the heating program, yields evidence against vacancy migration in the 0. 31 Tm stage for VIa bcc metals.

UR - https://www.scopus.com/pages/publications/0014863513

U2 - 10.1080/00337577008235016

DO - 10.1080/00337577008235016

M3 - Article

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JO - Radiation Effects

JF - Radiation Effects

IS - 3-4

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