arXiv (All)
open access
Parameter Estimation from Amplitude Collapse in Correlated Matter-Wave Interference
Operating matter-wave interferometers as quantum detectors for fundamental physics or inertial sensors with unprecedented accuracies relies on noise rejection, often implemented by correlating multiple sensors. They can be spatially separated (gradiometry or gravitational-wave detection) or consist
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Time domain non-linear quantum interferometry#1083253
- Direct characterization of classical dephasing noise for a qubit#1052146
- EPR-based quantum noise reduction in future gravitational-wave detectors: control and optomechanical integration of the SIPS interferometer#433529
- Path-Degenerate Quantum Interferometry for Decoherence Mitigation in Gravitational-Wave Detectors#1000168
- Wide-Mass-Scanning-Range Setup and Phase-Resolved Protocol for Axion Dark Matter Detection#1116885
Record · ID 984986
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive