Bounds on Spontaneous Collapse model of Quantum Mechanics from formation
  of CMBR and Standard Cosmology
  Continuous Spontaneous Localization (CSL) model of Quantum Mechanics modifies
Schr\"{o}dinger equation by adding non-linear stochastic terms due to which the
total energy of a system increases with a constant rate which is proportional
to the collapse rate $\lambda$. Thus applying CSL model to cosmological
scenarios can change the thermal behaviour of the particles during evolution
and we will put constraints on $\lambda$ by considering several cosmological
scenarios.
