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 > physics > arXiv:2509.01449v1

Help | Advanced Search

Physics > Optics

arXiv:2509.01449v1 (physics)
[Submitted on 1 Sep 2025 ]

Title: A matter of perspective: how nanoscale optical defects limit cosmic-scale gravitational wave observations

Title: 视角的问题:纳米尺度的光学缺陷如何限制宇宙尺度的引力波观测

Authors:Anna C. Green, Antonella Bianchi, Daniel D. Brown, Felice Feldmann, Jeremie Gobeil, Miron van der Kolk, Riccardo Maggiore, Jonathan W. Perry, Emma Prins, Mischa Salle, Alina Soflau, Enzo Tapia, Andreas Freise
Abstract: Ground-based gravitational-wave (GW) detectors, such as LIGO, Virgo, and KAGRA, have revolutionised as- tronomy. Now, future detectors like the Einstein Telescope and Cosmic Explorer aim to achieve even greater sensitivity. Advanced optical simulations are crucial to overcoming the challenges faced by these complex in- terferometers. Finesse, the leading interferometer simulation tool in the GW community, supports the design and commissioning of these detectors by modeling optical, quantum, and mechanical effects. A key focus is understanding optical defects that distort the shape of the laser light and limit detector performance. This work explores how nanoscale defects affect GW observations and presents recent advancements in modeling their effects to guide the development of next-generation detector optics.
Abstract: 地面引力波(GW)探测器,如LIGO、Virgo和KAGRA,已经革新了天文学。 现在,未来的探测器如爱因斯坦望远镜和宇宙探索者旨在实现更高的灵敏度。 先进的光学模拟对于克服这些复杂干涉仪面临的挑战至关重要。 Finesse是GW社区中领先的干涉仪模拟工具,通过建模光学、量子和机械效应来支持这些探测器的设计和调试。 一个关键的研究重点是理解会扭曲激光光束形状并限制探测器性能的光学缺陷。 这项工作探讨了纳米级缺陷如何影响引力波观测,并介绍了最近在模拟其影响方面的进展,以指导下一代探测器光学的发展。
Comments: Proceedings, SPIE Optical Metrology X, 2025
Subjects: Optics (physics.optics) ; General Relativity and Quantum Cosmology (gr-qc); Instrumentation and Detectors (physics.ins-det)
Cite as: arXiv:2509.01449 [physics.optics]
  (or arXiv:2509.01449v1 [physics.optics] for this version)
  https://doi.org/10.48550/arXiv.2509.01449
arXiv-issued DOI via DataCite
Journal reference: Proceedings Volume 13568, Modeling Aspects in Optical Metrology X; 135680R (2025)
Related DOI: https://doi.org/10.1117/12.3062573
DOI(s) linking to related resources

Submission history

From: Anna C. Green [view email]
[v1] Mon, 1 Sep 2025 13:07:41 UTC (2,548 KB)
Full-text links:

Access Paper:

    View a PDF of the paper titled
  • View Chinese PDF
  • View PDF
  • HTML (experimental)
  • TeX Source
  • Other Formats
license icon view license
Current browse context:
physics.optics
< prev   |   next >
new | recent | 2025-09
Change to browse by:
gr-qc
physics
physics.ins-det

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