Simple perturbatively traversable wormholes from bulk fermions

Abstract A new class of traversable wormholes was recently constructed which relies only on local bulk dynamics rather than an explicit coupling between distinct boundaries. Here we begin with a four-dimensional Weyl fermion field of any mass m propagating on a classical background defined by a Z2 q...

Full description

Bibliographic Details
Main Authors: Donald Marolf, Sean McBride
Format: Article
Language:English
Published: SpringerOpen 2019-11-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP11(2019)037
id doaj-bbb123deab904d1dba2a0eae0f1c60c9
record_format Article
spelling doaj-bbb123deab904d1dba2a0eae0f1c60c92020-11-25T04:08:37ZengSpringerOpenJournal of High Energy Physics1029-84792019-11-0120191113110.1007/JHEP11(2019)037Simple perturbatively traversable wormholes from bulk fermionsDonald Marolf0Sean McBride1Department of Physics, University of CaliforniaDepartment of Physics, University of CaliforniaAbstract A new class of traversable wormholes was recently constructed which relies only on local bulk dynamics rather than an explicit coupling between distinct boundaries. Here we begin with a four-dimensional Weyl fermion field of any mass m propagating on a classical background defined by a Z2 quotient of (rotating) BTZ × S 1. This setup allows one to compute the fermion stress-energy tensor exactly. For appropriate boundary conditions around a non-contractible curve, perturbative back-reaction at any m renders the associated wormhole traversable and suggests it can become eternally traversable at the limit where the background becomes extremal. A key technical step is the proper formulation of the method of images for fermions in curved spacetime. We find the stress- energy of spinor fields to have important kinematic differences from that of scalar fields, typically causing the sign of the integrated null stress-energy (and thus in many cases the sign of the time delay/advance) to vary around the throat of the wormhole. Similar effects may arise for higher-spin fields.http://link.springer.com/article/10.1007/JHEP11(2019)037Black HolesGauge-gravity correspondence
collection DOAJ
language English
format Article
sources DOAJ
author Donald Marolf
Sean McBride
spellingShingle Donald Marolf
Sean McBride
Simple perturbatively traversable wormholes from bulk fermions
Journal of High Energy Physics
Black Holes
Gauge-gravity correspondence
author_facet Donald Marolf
Sean McBride
author_sort Donald Marolf
title Simple perturbatively traversable wormholes from bulk fermions
title_short Simple perturbatively traversable wormholes from bulk fermions
title_full Simple perturbatively traversable wormholes from bulk fermions
title_fullStr Simple perturbatively traversable wormholes from bulk fermions
title_full_unstemmed Simple perturbatively traversable wormholes from bulk fermions
title_sort simple perturbatively traversable wormholes from bulk fermions
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2019-11-01
description Abstract A new class of traversable wormholes was recently constructed which relies only on local bulk dynamics rather than an explicit coupling between distinct boundaries. Here we begin with a four-dimensional Weyl fermion field of any mass m propagating on a classical background defined by a Z2 quotient of (rotating) BTZ × S 1. This setup allows one to compute the fermion stress-energy tensor exactly. For appropriate boundary conditions around a non-contractible curve, perturbative back-reaction at any m renders the associated wormhole traversable and suggests it can become eternally traversable at the limit where the background becomes extremal. A key technical step is the proper formulation of the method of images for fermions in curved spacetime. We find the stress- energy of spinor fields to have important kinematic differences from that of scalar fields, typically causing the sign of the integrated null stress-energy (and thus in many cases the sign of the time delay/advance) to vary around the throat of the wormhole. Similar effects may arise for higher-spin fields.
topic Black Holes
Gauge-gravity correspondence
url http://link.springer.com/article/10.1007/JHEP11(2019)037
work_keys_str_mv AT donaldmarolf simpleperturbativelytraversablewormholesfrombulkfermions
AT seanmcbride simpleperturbativelytraversablewormholesfrombulkfermions
_version_ 1724424872394752000