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...
Main Authors: | , |
---|---|
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 |