Zobrazeno 1 - 10
of 5 899
pro vyhledávání: '"P. Moiseev"'
Autor:
Moiseev, S. A., Gerasimov, K. I., Minnegaliev, M. M., Moiseev, E. S., Deev, A. D., Balega, Yu. Yu.
Based on new obtained analytical results, the main properties of photon echo quantum memory protocols are analysed and discussed together with recently achieved experimental results. The main attention is paid to studying the influence of spectral di
Externí odkaz:
http://arxiv.org/abs/2410.01664
We continue to present the results of a Byurakan Narrow Band Imaging Survey (BNBIS). In this work we present the results of the search and further detailed investigation of the objects, found in the course of the BNBIS survey in the southern part of
Externí odkaz:
http://arxiv.org/abs/2412.11268
We continue to study the structure and kinematics of HH flows. Herbig-Haro (HH) flows exhibit large variety of morphological and kinematical structures. Both proper motion (PM) and radial velocity investigations are essential to understand the physic
Externí odkaz:
http://arxiv.org/abs/2411.17171
We present a time-dependent quantum calculations of the first order and second order photon correlation functions for the scattering of a single-photon pulse on a two-level atom (qubit) embedded in a one-dimensional open waveguide. Within Markov appr
Externí odkaz:
http://arxiv.org/abs/2410.17710
Autor:
Moiseev, Kirill
Publikováno v:
Journal of the New Economic Association, 3 (64), 30-52 (2024), in Russian
In countries with a growing number of elderly and a shrinking workforce, one of which is Russia, it becomes impossible to maintain a solidary pension system and a need to switch to a more stable funded system appears. This paper analyzes various scen
Externí odkaz:
http://arxiv.org/abs/2410.14004
Publikováno v:
Astronomy Reports, 2024, Vol.68, No.7, pp.619-640
Results of a study of physical parameters of stellar population in star formation regions in galaxies with signs of peculiarity NGC 3963 and NGC 7292 are presented. The study was carried out based on the analysis of photometric (UBVRI bands), H-alpha
Externí odkaz:
http://arxiv.org/abs/2410.06098
Autor:
Smith, Lucas D., Cannady, Nicholas, Caputo, Regina, Kierans, Carolyn, Kirschner, Nicholas, Liceaga-Indart, Iker, McEnery, Julie, Metzler, Zachary, Moiseev, A. A., Parker, Lucas, Perkins, Jeremy, Sasaki, Makoto, Schoenwald, Adam J., Shy, Daniel, Valverde, Janeth, Wasti, Sambid, Woolf, Richard, Bolotnikov, Aleksey, Caligiure, Thomas J., Crosier, A. Wilder, Fried, Jack, Ghosh, Priyarshini, Griffin, Sean, Grove, J. Eric, Hays, Elizabeth, Kong, Emily, Mitchell, John, Phlips, Bernard, Sleator, Clio, Thompson, D. J., Wulf, Eric, Zajczyk, Anna
Publikováno v:
Proc. SPIE 13093, Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray, 130937Z (21 August 2024)
The ComPair balloon instrument is a prototype gamma-ray telescope that aims to further develop technology for observing the gamma-ray sky in the MeV regime. ComPair combines four detector subsystems to enable parallel Compton scattering and pair-prod
Externí odkaz:
http://arxiv.org/abs/2410.02557
We propose a quantum memory based on the pre-created long-lived macroscopic quantum coherence. It is shown that the proposed approach provides new physical properties and methods for retrieval of the signal light fields and improvement of the basic p
Externí odkaz:
http://arxiv.org/abs/2408.09991
We show that swallowtail catastrophe consisting of various-order non-Hermitian and Hermitian degeneracies naturally exists in the dynamics of two-mode driven-dissipative quadrature squeezing systems that break pseudo-Hermiciticy by judiciously engine
Externí odkaz:
http://arxiv.org/abs/2408.11268
Autor:
Xi, Hongwei, Peng, Bo, Staveley-Smith, Lister, For, Bi-Qing, Liu, Bin, Chen, Ru-Rong, Yu, Lei, Ding, Dejian, Guo, Wei-Jian, Zou, Hu, Xue, Suijian, Wang, Jing, Brink, Thomas G., Zheng, WeiKang, Filippenko, Alexei V., Yang, Yi, Wei, Jianyan, Dai, Y. Sophia, Li, Zi-Jian, He, Zizhao, Jiang, Chengzi, Moiseev, Alexei, Kotov, Sergey
Publikováno v:
ApJL, 966(2024), L36
Neutral hydrogen (HI) is the primary component of the cool interstellar medium (ISM) and is the reservoir of fuel for star formation. Owing to the sensitivity of existing radio telescopes, our understanding of the evolution of the ISM in galaxies rem
Externí odkaz:
http://arxiv.org/abs/2408.00419