Skip to main content
CenXiv.org
This website is in trial operation, support us!
We gratefully acknowledge support from all contributors.
Contribute
Donate
cenxiv logo > hep-th > arXiv:2510.01324

Help | Advanced Search

High Energy Physics - Theory

arXiv:2510.01324 (hep-th)
[Submitted on 1 Oct 2025 ]

Title: AdS vacua of non-supersymmetric strings

Title: 非超对称弦的AdS真空

Authors:Salvatore Raucci, Alessandro Tomasiello
Abstract: Few vacua are known for the three tachyon-free non-supersymmetric string theories. We find new classes of AdS backgrounds by focusing on spaces where the equations of motion reduce to purely algebraic conditions. Our first examples involve non-zero three-form fluxes supported either on direct product internal spaces or on $T_{p,q}$ geometries. For the ${\mathrm{SO}}(16)\times{\mathrm{SO}}(16)$ heterotic string, we then develop a method to engineer vacua with the addition of gauge fields. A formal Kaluza--Klein reduction yields complete solutions on a broad class of coset spaces $G/H$, automatically satisfying the three-form Bianchi identities with $H$-valued gauge fields.
Abstract: 已知三种无快子的非超对称弦理论的真空状态很少。 我们通过关注方程运动简化为纯代数条件的空间,找到了新的AdS背景类别。 我们的第一个例子涉及在直积内部空间或$T_{p,q}$几何上支持的非零三形式通量。 对于${\mathrm{SO}}(16)\times{\mathrm{SO}}(16)$杂交弦理论,我们随后开发了一种方法,通过添加规范场来构造真空。 一种形式的Kaluza--Klein约化在广义的齐次空间$G/H$上产生了完整的解,自动满足带有$H$值规范场的三形式Bianchi恒等式。
Comments: 31 pages
Subjects: High Energy Physics - Theory (hep-th)
Cite as: arXiv:2510.01324 [hep-th]
  (or arXiv:2510.01324v1 [hep-th] for this version)
  https://doi.org/10.48550/arXiv.2510.01324
arXiv-issued DOI via DataCite
Journal reference: IFT-UAM/CSIC-25-101

Submission history

From: Salvatore Raucci [view email]
[v1] Wed, 1 Oct 2025 18:00:06 UTC (41 KB)
Full-text links:

Access Paper:

    View a PDF of the paper titled
  • View Chinese PDF
  • View PDF
  • HTML (experimental)
  • TeX Source
view license
Current browse context:
hep-th
< prev   |   next >
new | recent | 2025-10

References & Citations

  • NASA ADS
  • Google Scholar
  • Semantic Scholar
a export BibTeX citation Loading...

BibTeX formatted citation

×
Data provided by:

Bookmark

BibSonomy logo Reddit logo

Bibliographic and Citation Tools

Bibliographic Explorer (What is the Explorer?)
Connected Papers (What is Connected Papers?)
Litmaps (What is Litmaps?)
scite Smart Citations (What are Smart Citations?)

Code, Data and Media Associated with this Article

alphaXiv (What is alphaXiv?)
CatalyzeX Code Finder for Papers (What is CatalyzeX?)
DagsHub (What is DagsHub?)
Gotit.pub (What is GotitPub?)
Hugging Face (What is Huggingface?)
Papers with Code (What is Papers with Code?)
ScienceCast (What is ScienceCast?)

Demos

Replicate (What is Replicate?)
Hugging Face Spaces (What is Spaces?)
TXYZ.AI (What is TXYZ.AI?)

Recommenders and Search Tools

Influence Flower (What are Influence Flowers?)
CORE Recommender (What is CORE?)
IArxiv Recommender (What is IArxiv?)
  • Author
  • Venue
  • Institution
  • Topic

arXivLabs: experimental projects with community collaborators

arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website.

Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them.

Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs.

Which authors of this paper are endorsers? | Disable MathJax (What is MathJax?)
  • About
  • Help
  • contact arXivClick here to contact arXiv Contact
  • subscribe to arXiv mailingsClick here to subscribe Subscribe
  • Copyright
  • Privacy Policy
  • Web Accessibility Assistance
  • arXiv Operational Status
    Get status notifications via email or slack

京ICP备2025123034号