Difference between revisions of "My List of Research Articles on Photon Detection"
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| − | [http://optoelectronics.perkinelmer.com/content/ApplicationNotes/APP_APDUsersGuide.pdf Introduction on Avalanche Photodiodes] | + | *[http://optoelectronics.perkinelmer.com/content/ApplicationNotes/APP_APDUsersGuide.pdf Introduction on Avalanche Photodiodes] |
| − | * What is dark noise? | + | ** What is dark noise? |
| − | [http:// | + | *[http://zeus.phys.uconn.edu/halld/siliconPM/NPB-150-144.pdf Using the SiPM for Particle Physics] |
| + | ** Ultra-relativistic Universe? -detected to find out more about | ||
| + | ** Geiger mode? -SiPMs will be running in or "limited Geiger Mode | ||
| + | ** The SiPMs tested are ineffective at detecting Ultraviolet because it has no n-on-p structure. | ||
| + | ** Dynamic Range? of what? (wavelength of detected light?) | ||
| + | *[http://zeus.phys.uconn.edu/halld/siliconPM/ICRC-2005-101.pdf Another Article about using the SiPM for the Magic/Euso detector] | ||
| + | ** Quantum Efficiency vs. Regular Efficiency | ||
| + | ** What is threshold energy? ph.e.? | ||
| + | ** to Prevent Crosstalk, one could Optically decouples cells from each other. | ||
| + | ** Passive Quenching - why would you want to quench breakdown if that signifies a successful detection? | ||
| + | ** "In this new concept the readout node of a silicon drift detector (SDD) is replaced by a Geiger APD." (?) | ||
| + | *[http://zeus.phys.uconn.edu/halld/siliconPM/courier-2-2007.htm Cern's take on the SiPM] | ||
| + | ** Very good temperature stability? What we are testing? | ||
| + | *[http://zeus.phys.uconn.edu/halld/siliconPM/NIMA-504-48.pdf Technical applications of the SiPM] | ||
| + | *[http://zeus.phys.uconn.edu/halld/siliconPM/ICFA-9-2001.pdf Advanced study of Silicon Photomultiplier] | ||
| + | ** Graph end of Page 3, explanation - pg 4 | ||
| + | ** Where does electronic noise come from? | ||
| + | ** ENF Factor? | ||
| + | ** Figure 6 | ||
| + | ** If a SiPM is just an array of APDs, then shouldn't the SiPM have at least the same complexity, if not be more complex than the APD? | ||
| + | |||
| + | |||
| + | * If the goal is to detect individual photons, then can any dark rate be acceptable at all, especially to the magnitude of 10^6 events/mm^2 sec or even 10^4 events/mm^2 sec" | ||
| + | * What are virtual Photons? | ||
| + | ---- | ||
| + | [http://en.wikipedia.org/wiki/Silicon_photomultiplier Wiki article?] | ||
Latest revision as of 22:48, 17 January 2008
- Introduction on Avalanche Photodiodes
- What is dark noise?
- Using the SiPM for Particle Physics
- Ultra-relativistic Universe? -detected to find out more about
- Geiger mode? -SiPMs will be running in or "limited Geiger Mode
- The SiPMs tested are ineffective at detecting Ultraviolet because it has no n-on-p structure.
- Dynamic Range? of what? (wavelength of detected light?)
- Another Article about using the SiPM for the Magic/Euso detector
- Quantum Efficiency vs. Regular Efficiency
- What is threshold energy? ph.e.?
- to Prevent Crosstalk, one could Optically decouples cells from each other.
- Passive Quenching - why would you want to quench breakdown if that signifies a successful detection?
- "In this new concept the readout node of a silicon drift detector (SDD) is replaced by a Geiger APD." (?)
- Cern's take on the SiPM
- Very good temperature stability? What we are testing?
- Technical applications of the SiPM
- Advanced study of Silicon Photomultiplier
- Graph end of Page 3, explanation - pg 4
- Where does electronic noise come from?
- ENF Factor?
- Figure 6
- If a SiPM is just an array of APDs, then shouldn't the SiPM have at least the same complexity, if not be more complex than the APD?
- If the goal is to detect individual photons, then can any dark rate be acceptable at all, especially to the magnitude of 10^6 events/mm^2 sec or even 10^4 events/mm^2 sec"
- What are virtual Photons?