Published May 4, 2011 | Version v1
Journal article

Modelling Of Residual Stresses Induced By High Speed Milling Process

  • 1. Mines ParisTech, CEMEF, Centre of Material Forming, CNRS UMR 7635, BP 207, 1 rue Claude Daunesse, 06904 Sophia Antipolis Cedex (France)
  • 2. Industrial Risks Management Dept.-EDF R and D, Chatou-78400 (France)

Description

Maintenance processes used in heavy industries often include high speed milling operations. The reliability of the post-process material state has to be studied. Numerical simulation appears to be a very interesting way to supply an efficient residual stresses (RS) distribution prediction.Because the adiabatic shear band and the serrated chip shaping are features of the austenitic stainless steel high speed machining, a 2D high speed orthogonal cutting model is briefly presented. This finite element model, developed on Forge registered software, is based on data taken from Outeiro and al.'s paper [1]. A new behaviour law fully coupling Johnson-Cook's constitutive law and Latham and Cockcroft's damage model is detailed in this paper. It ensures results that fit those found in literature.Then, the numerical tools used on the 2D model are integrated to a 3D high speed milling model. Residual stresses distribution is analysed, on the surface and into the depth of the material. Various revolutions and passes of the two teeth hemispheric mill on the workpiece are simulated. Thus the sensitivity of the residual stresses generation to the cutting conditions can be discussed. In order to validate the 3D model, a comparison of the cutting forces measured by EDF R and D to those given by numerical simulations is achieved.

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1353
Journal Issue
1
Journal Page Range
p. 597-602
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
14. international ESAFORM conference on material forming
Acronym
ESAFORM 2011
Dates
27-29 Apr 2011
Place
Belfast, Northern Ireland (United Kingdom)

Optional Information

Notes
(c) 2011 American Institute of Physics