Title of article :
Influence of Addendum Modification Factor on Root Stresses in Normal Contact Ratio Asymmetric Spur Gears
Author/Authors :
Prabhu Sekar, R Mechanical Engineering Department - Motilal Nehru National Institute of Technology - Allahabad, India , Ravivarman, R Research Scholar Department of Mechanical Engineering - Pondicherry Engineering college - Pondicherry, India
Abstract :
Tooth root crack is considered as one of the crucial causes of failure in
the gearing system and it occurs at the tooth root due to an excessive
bending stress developed in the root region. The modern power
transmission gear drives demand high bending load capacity, increased
contact load capacity, low weight, reduced noise and longer life. These
subsequent conditions are satisfied by the aid of precisely designed
asymmetric tooth profile which turns out to be a suitable alternate for
symmetric spur gears in applications like aerospace, automotive, gear
pump and wind turbine industries. In all step up and step down gear
drives (gear ratio > 1), the pinion (smaller in size) is treated as a
vulnerable one than gear (larger in size) which is primarily due to the
development of maximum root stress in the pinion tooth. This paper
presents an idea to improve the bending load capacity of asymmetric spur
gear drive system by achieving the same stresses between the asymmetric
pinion and gear fillet regions which can be accomplished by providing an
appropriate addendum modification. For this modified addendum the
pinion and gear teeth proportion equations have been derived. In
addition, the addendum modification factors required for a balanced
maximum fillet stress condition has been determined through FEM for
different parameters like drive side pressure angle, number of teeth and
gear ratio. The bending load capacity of the simulated addendum
modified asymmetric spur gear drives were observed to be prevalent
(very nearly 7%) to that of uncorrected asymmetric gear drives.
Keywords :
Asymmetric gear , Addendum modification factor , Finite element model , Fillet stress factor
Journal title :
Astroparticle Physics