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Faculty of Physics University of Warsaw > Events > Seminars > Solid State Physics Seminar
2024-11-22 (Friday)
room 0.06, Pasteura 5 at 10:15  Calendar icon
prof. Michał Nikodem (Faculty of Fundamental Problems of Technology, Wrocław University of Science and Technology)

"Antiresonant hollow-core fibers – a useful tool... also in gas sensing"

Antiresonant hollow-core fibers (AR-HCFs) have proven highly valuable across various applications. They are utilized in fields ranging from high-energy pulse delivery to ultra-low-loss and low-latency light transmission. In my presentation, I will explore how AR-HCFs can be effectively applied in laser spectroscopy, with a special emphasis on practical aspects of their use. I will show our experimental approach to laser-based trace gas sensing with AR-HCFs and highlight unique sensing configurations that are not achievable with conventional laser-based sensing methods.
2024-11-15 (Friday)
room 0.06, Pasteura 5 at 10:15  Calendar icon
dr inż. Marek Maciaszek (Wydział Fizyki Politechniki Warszawskiej Faculty of Physics, Warsaw University of Technology)

Ab initio study of carbon-related defects in hexagonal boron nitride: searching for single-photon emitters

Hexagonal boron nitride (h-BN) has long been used in nanotechnology as an insulating layer in heterostructures with graphene, owing to its wide bandgap (~6 eV). Recently, however, h-BN has gained significant attention due to the discovery of various color centers in its samples that exhibit single-photon emission. These single-photon emitters in h-BN are particularly attractive due to their excellent brightness and photostability, even at room temperature. Additionally, the wide bandgap of h-BN enables the hosting of single-photon emitters across a broad spectral range, from the infrared to the ultraviolet.While experiments suggest a correlation between the intensity of emission from many of these centers and the carbon content in h-BN samples, the chemical nature of most of the observed emitters remains unclear. To further advance the field, it is crucial to identify the point defects responsible for the observed emissions. First-principles calculations could play a pivotal role in achieving this goal.In my presentation I will discuss results of first-principles calculations focused on identifying three groups of emitters in h-BN, most likely associated with carbon defects: (i) ultraviolet emitters (ZPL 4.1 eV), (ii) so called “visible emitters” (ZPL between 1.6 and 2.1 eV), and (iii) blue emitters (ZPL 2.85 eV).
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