The stability of a quantum superposition of two different stationary
mass distributions is examined, where the perturbing effect of each
distribution on the space-time structure is taken into account, in
accordance with the principles of general relativity. It is argued that
the definition of the time-translation operator for the superposed
space-times involves an inherent ill-definedness, leading to an
essential uncertainty in the energy of the superposed state which, in
the Newtonian limit, is proportional to the gravitational self-energyE
<SUB>Delta</SUB> of the difference between the two mass distributions.
This is consistent with a suggested finite lifetime of the order of
h/E <SUB>Delta</SUB> for the superposed state, in agreement
with a certain proposal made by the author for a gravitationally induced
spontaneous quantum state reduction, and with closely related earlier
suggestions by Di&\#243;si and by Ghirardiet al.
%0 Journal Article
%1 Penrose1996Gravitys
%A Penrose, R.
%D 1996
%I Springer Netherlands
%J General Relativity and Gravitation
%K quantum gravity
%N 5
%P 581--600
%R 10.1007/bf02105068
%T On Gravity's role in Quantum State Reduction
%U http://dx.doi.org/10.1007/bf02105068
%V 28
%X The stability of a quantum superposition of two different stationary
mass distributions is examined, where the perturbing effect of each
distribution on the space-time structure is taken into account, in
accordance with the principles of general relativity. It is argued that
the definition of the time-translation operator for the superposed
space-times involves an inherent ill-definedness, leading to an
essential uncertainty in the energy of the superposed state which, in
the Newtonian limit, is proportional to the gravitational self-energyE
<SUB>Delta</SUB> of the difference between the two mass distributions.
This is consistent with a suggested finite lifetime of the order of
h/E <SUB>Delta</SUB> for the superposed state, in agreement
with a certain proposal made by the author for a gravitationally induced
spontaneous quantum state reduction, and with closely related earlier
suggestions by Di&\#243;si and by Ghirardiet al.
@article{Penrose1996Gravitys,
abstract = {{The stability of a quantum superposition of two different stationary
mass distributions is examined, where the perturbing effect of each
distribution on the space-time structure is taken into account, in
accordance with the principles of general relativity. It is argued that
the definition of the time-translation operator for the superposed
space-times involves an inherent ill-definedness, leading to an
essential uncertainty in the energy of the superposed state which, in
the Newtonian limit, is proportional to the gravitational self-energyE
<SUB>Delta</SUB> of the difference between the two mass distributions.
This is consistent with a suggested finite lifetime of the order of
h/E <SUB>Delta</SUB> for the superposed state, in agreement
with a certain proposal made by the author for a gravitationally induced
spontaneous quantum state reduction, and with closely related earlier
suggestions by Di\&\#243;si and by Ghirardiet al.}},
added-at = {2013-09-09T23:59:35.000+0200},
author = {{Penrose}, R.},
biburl = {https://www.bibsonomy.org/bibtex/242a139495e43e80069dd867d7d45b024/jacksankey},
citeulike-article-id = {7676318},
citeulike-linkout-0 = {http://dx.doi.org/10.1007/bf02105068},
citeulike-linkout-1 = {http://adsabs.harvard.edu/cgi-bin/nph-bib\_query?bibcode=1996GReGr..28..581P},
citeulike-linkout-2 = {http://www.springerlink.com/content/k75046wh3668l654},
day = 1,
doi = {10.1007/bf02105068},
interhash = {fa73d6216b428575290c7686db1c4647},
intrahash = {42a139495e43e80069dd867d7d45b024},
issn = {0001-7701},
journal = {General Relativity and Gravitation},
keywords = {quantum gravity},
month = may,
number = 5,
pages = {581--600},
posted-at = {2010-10-15 19:28:14},
priority = {2},
publisher = {Springer Netherlands},
timestamp = {2013-09-11T14:37:11.000+0200},
title = {{On Gravity's role in Quantum State Reduction}},
url = {http://dx.doi.org/10.1007/bf02105068},
volume = 28,
year = 1996
}