diff options
| author | John MacFarlane <jgm@berkeley.edu> | 2020-10-07 23:03:14 -0700 |
|---|---|---|
| committer | John MacFarlane <jgm@berkeley.edu> | 2020-10-07 23:05:51 -0700 |
| commit | 1be0f0fba8d860b960e79442a891fce6b1aca192 (patch) | |
| tree | 8a8be459bd7d03e5509382029ba65f2433969240 /test/command/biblatex-itzhaki.md | |
| parent | a520181cdbfa69b4c9a0432e12847cd7d666d41f (diff) | |
| download | pandoc-1be0f0fba8d860b960e79442a891fce6b1aca192.tar.gz | |
Use double quotes for YAML metadata.
Closes #6727.
Diffstat (limited to 'test/command/biblatex-itzhaki.md')
| -rw-r--r-- | test/command/biblatex-itzhaki.md | 16 |
1 files changed, 8 insertions, 8 deletions
diff --git a/test/command/biblatex-itzhaki.md b/test/command/biblatex-itzhaki.md index 29921404c..e440418dc 100644 --- a/test/command/biblatex-itzhaki.md +++ b/test/command/biblatex-itzhaki.md @@ -55,14 +55,14 @@ NOTES: ^D --- -nocite: '[@*]' +nocite: "[@*]" references: -- abstract: 'We discuss the limitations of ''t Hooft''s proposal for the +- abstract: "We discuss the limitations of 't Hooft's proposal for the black hole S-matrix. We find that the validity of the S-matrix implies violation of the semi-classical approximation at scales large compared to the Planck scale. We also show that the effect of the centrifugal barrier on the S-matrix is crucial even for large - transverse distances.' + transverse distances." annote: An online reference from arXiv. Note the eprint and eprinttype fields. Also note that the arXiv reference is transformed into a clickable link if hyperref support has been enabled @@ -70,12 +70,12 @@ references: - family: Itzhaki given: Nissan id: itzhaki - issued: '1996-03-11' - language: 'en-US' - title: 'Some remarks on ''[t Hooft''s]{.nocase} S-matrix for black - holes' + issued: "1996-03-11" + language: "en-US" + title: "Some remarks on '[t Hooft's]{.nocase} S-matrix for black + holes" type: webpage - url: 'http://arxiv.org/abs/hep-th/9603067' + url: "http://arxiv.org/abs/hep-th/9603067" version: 1 --- |