Liu Dang-bo

ORCID: 0000-0003-1538-592X
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About
Contact & Profiles
Research Areas
  • Astrophysics and Cosmic Phenomena
  • Astrophysical Phenomena and Observations
  • Gamma-ray bursts and supernovae
  • Galaxies: Formation, Evolution, Phenomena
  • Pulsars and Gravitational Waves Research
  • Advanced Chemical Physics Studies
  • Quantum, superfluid, helium dynamics
  • Astrophysics and Star Formation Studies
  • Stellar, planetary, and galactic studies
  • Nuclear physics research studies
  • Quantum Chromodynamics and Particle Interactions
  • Radiation Detection and Scintillator Technologies
  • Hydrogen Storage and Materials
  • X-ray Spectroscopy and Fluorescence Analysis
  • Calibration and Measurement Techniques
  • Laser-Plasma Interactions and Diagnostics
  • Atomic and Subatomic Physics Research
  • Particle Accelerators and Free-Electron Lasers
  • Cold Atom Physics and Bose-Einstein Condensates
  • Magnetic confinement fusion research
  • Nuclear Physics and Applications
  • High-pressure geophysics and materials
  • Quantum and electron transport phenomena
  • Ammonia Synthesis and Nitrogen Reduction
  • Particle accelerators and beam dynamics

Shanghai Jiao Tong University
2005-2022

Center for Astrophysics Harvard & Smithsonian
2014

Institute of Particle Physics
2010-2011

Institute of Theoretical Physics
2002-2003

We analyze both the early- and late-time radio X-ray data of tidal disruption event (TDE) Swift J1644+57. The at early times (≲ 5 days) necessitate separation emission regions, either spatially or in velocity space. This leads us to suggest a two-component jet model, which inner is initially relativistic with Lorentz factor Γ ≈ 15, while outer trans-relativistic, ≲ 1.2. model enables self-consistent interpretation data, terms peak frequency flux. solve dynamics, radiative cooling, expected...

10.1088/0004-637x/798/1/13 article EN The Astrophysical Journal 2014-12-12

Comptonization is a very important phenomenon in astrophysics. The Kompaneets equation describes the process up-Comptonization (h ν̄ ≪ kT e ), while it fails describing down-Comptonization ( hν ̄ ≫ which most radiative transfer hard X-ray and γ -ray astronomy. In this study we extend to new modified works more general process, including up- down-Comptonization, suitable for cases , ∼ . Numerical solutions evolution behavior of Gaussian emission lines show excellent agreement between...

10.1051/0004-6361/201936513 article EN cc-by Astronomy and Astrophysics 2020-12-21

Internal line shifts in quasars spectra have played a more prominent role our understanding of quasar structure and dynamics. The observed different redshift among broad hydrogen lines is still an amazing puzzle the study quasars. We argued that lines, as well low-ionization quasars, are significantly contributed by Cerenkov quasi-line emission fast electrons dense clouds/filaments/sheets ($N_{\rm H}\geq 10^{14}~{\rm cm^{-3}}$); whereas this line-like radiation mechanism invalid for...

10.48550/arxiv.1505.04122 preprint EN other-oa arXiv (Cornell University) 2015-01-01

We present a simplified formulae system describing the polarization properties of quantum cyclotron radiation by nonrelativistic thermal electron in very strong magnetic field. In this system, each derived quantities, including Einstein coefficients, absorption cross sections, and scattering as well coefficients plasma, is divided into perpendicularly parallelly polarized components. The results, especially sections resonant frequency photons, are potentially important x-ray γ-ray astronomy,...

10.1088/0256-307x/24/11/030 article EN Chinese Physics Letters 2007-10-17

10.1016/j.chinastron.2007.10.002 article EN Chinese Astronomy and Astrophysics 2007-10-01

Two-photon annihilation (γ–γ reaction) is an important absorption mechanism in γ-ray physics and astronomy. Using the markedly simplified direction-averaged cross section of (ω,ω') for a normal isotropic ambient radiation field around source, we obtain matching condition energies two interacting photons, which ensures attainment maximum probability. This new result that helpful to better understanding behaviour γ–γ process, this predicts some possible line-like structures emergent continuous...

10.1088/0256-307x/22/6/071 article EN Chinese Physics Letters 2005-05-25

Within the framework of Usdpf(16) interacting boson model (IBM), effects strong correlations dipole (p−-boson) and octupole (f−-boson) degree freedom on positive-parity states even-even nuclei in SU(3) limit are discussed. It is shown that configurations an even number many p- f-bosons can not only be incorporated into usual low-lying collective rotational bands, such as ground state band, β- γ-vibrational but also naturally form etc. These results similar to Usdg(15)-IBM good agreement with...

10.1088/0253-6102/39/5/587 article EN Communications in Theoretical Physics 2003-05-15

Recently we mentioned that the surface of solids often exerts Pauli repulsion on interstitial hydrogen, which markedly changes properties H, and increases its chemical activity,which is referred to as ‘Pauli activation H’ for short. The purpose this paper further confirm reality mechanism at a quantitative level. We particularly mention importance H-dipole hydrogen induced by catalysis, key understand principle catalysis mechanism. Taking simple diatomic molecule an example, first illustrate...

10.2139/ssrn.4010360 article EN SSRN Electronic Journal 2022-01-01

Recently we mentioned that the surface of solids often exerts Pauli repulsion on interstitial/substitutional hydrogen, which markedly changes properties H, and increases its chemical activity, is referred to as 'Pauli activation interstitial H' for short. The purpose this paper further confirm reality mechanism at a quantitative level. We particularly mention importance H-dipole hydrogen induced by catalysis, key understand principle catalysis mechanism. Taking simple diatomic molecule an...

10.1016/j.chphi.2022.100085 article EN cc-by-nc-nd Chemical Physics Impact 2022-06-24

The interacting boson model for anomalous rotational bands is proposed. In the SU(3) limit, an asymptotic limit discussed. Within framework of several analytic relations energies and electromagnetic transition rates are derived.

10.1088/0253-6102/38/5/591 article EN Communications in Theoretical Physics 2002-11-15

The surface of solids often exerts a Pauli repulsion on the adsorbed atoms/ions (interstitial and/or substitutional), which markedly changes their properties. And chemical activity atom/ion increases by this way. In paper, we focus activation interstitial hydrogen in hydrogenation. We simply refer it 'Pauli H' for short. first demonstrate that widely exists various solids. Then briefly introduce our past work published decades ago, is related with topics activation, including Schrodinger...

10.1016/j.chphi.2021.100058 article EN cc-by-nc-nd Chemical Physics Impact 2021-12-13
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