We study the stability of extra dimensions in string gas cosmology at late times. Vacuum energy and, interestingly, baryons lead to decompactification after they become dynamically important. The string gas can stabilise the effect of baryons, but not that of vacuum energy. However, we find that the interplay of baryons and strings can lead to acceleration in the visible dimensions, without the need for vacuum energy.Peer reviewe
We study the production of dark matter and dark radiation after reheating in string inflation models...
Recent astrophysical observations, pertaining to either high-redshift supernovae or cosmic microwave...
AbstractWe present a new model of dark energy which could explain the observed accelerated expansion...
We study the stability of extra dimensions in string gas cosmology at late times. Vacuum energy and,...
We present a critical review and summary of String Gas Cosmology. We include a pedagogical derivatio...
We present a critical review and summary of String Gas Cosmology. We include a pedagogical derivatio...
We study string gas dynamics in the early universe and seek to realize the Brandenberger - Vafa mech...
A long-standing problem of theoretical physics is the exceptionally small value of the cosmological ...
We study string gas dynamics in the early universe and seek to realize the Brandenberger - Vafa mech...
We study string gas dynamics in the early universe and seek to realize the Brandenberger - Vafa mech...
We argue that, for string compactifications broadly consistent with swampland constraints, dark ener...
We argue that, for string compactifications broadly consistent with swampland constraints, dark ener...
The problem of dark energy arises due to its self-gravitating properties. Therefore explaining vacuu...
We give an overview of the status of string cosmology. We explain the motivation for the subject, ou...
We review the origins, motivations, and implications for cosmology and black holes, of our proposal ...
We study the production of dark matter and dark radiation after reheating in string inflation models...
Recent astrophysical observations, pertaining to either high-redshift supernovae or cosmic microwave...
AbstractWe present a new model of dark energy which could explain the observed accelerated expansion...
We study the stability of extra dimensions in string gas cosmology at late times. Vacuum energy and,...
We present a critical review and summary of String Gas Cosmology. We include a pedagogical derivatio...
We present a critical review and summary of String Gas Cosmology. We include a pedagogical derivatio...
We study string gas dynamics in the early universe and seek to realize the Brandenberger - Vafa mech...
A long-standing problem of theoretical physics is the exceptionally small value of the cosmological ...
We study string gas dynamics in the early universe and seek to realize the Brandenberger - Vafa mech...
We study string gas dynamics in the early universe and seek to realize the Brandenberger - Vafa mech...
We argue that, for string compactifications broadly consistent with swampland constraints, dark ener...
We argue that, for string compactifications broadly consistent with swampland constraints, dark ener...
The problem of dark energy arises due to its self-gravitating properties. Therefore explaining vacuu...
We give an overview of the status of string cosmology. We explain the motivation for the subject, ou...
We review the origins, motivations, and implications for cosmology and black holes, of our proposal ...
We study the production of dark matter and dark radiation after reheating in string inflation models...
Recent astrophysical observations, pertaining to either high-redshift supernovae or cosmic microwave...
AbstractWe present a new model of dark energy which could explain the observed accelerated expansion...