Dense γ-ray emission in two consecutive pulses irradiating near critical density plasma
نویسندگان
چکیده
Abstract We report the overdense electron acceleration and dense gamma ray emission via use of two continuous laser pulses irradiating near critical density plasma. Thanks to ion channel formed behind first pulse, leading beam is well focused a higher intensity. As result, noticeable re-injection focusing when one incident significantly suppressed in two-consecutive- lasers scheme, efficiently improved process. Moreover, owing stronger field energy, probability rate accelerated emitting γ -rays considerably enhanced. In this regime, intensity reduced from 1 × 10 23 $4\times 10^{22}$?> 4 22 W cm −2 with competitive generated rays.
منابع مشابه
Microquasars: hard X-ray/γ-ray emission
I review some of the basic observational details of jets from X-ray binaries, or ‘microquasars’. It is shown that in both (Z and Atoll) NS and BHC systems radio emission, and therefore jet formation, is correlated with the presence of hard (30–500 keV) X-ray emission. At γ-ray (> 500 keV) energies, the relation is not so clear. Possible physical connections between the presence of a jet, with a...
متن کاملNon-photonic emission from γ-ray bursts
γ−ray bursts (GRBs) are likely sources of ultra-high energy, > 1019 eV, protons and high energy, > 1 TeV, neutrinos. Large volume detectors of ultra high energy cosmic rays (UHECRs) and high energy neutrinos, which are already operating and are being expanded, may allow to test in the coming few years the predictions of the GRB model for high energy proton and neutrino production. Detection of ...
متن کاملDiffuse γ-ray emission: lessons and perspectives
The Galactic diffuse emission is potentially able to reveal much about the sources and propagation of cosmic rays (CR), their spectra and intensities in distant locations. It can possibly unveil WIMP dark matter (DM) through its annihilation signatures. The extragalactic background may provide vital information about the early stages of the universe, neutralino annihilation, and unresolved sour...
متن کاملX-ray emission from dense plasma in CTTSs: Hydrodynamic modeling of the accretion shock
Context. High spectral resolution X-ray observations of classical T Tauri stars (CTTSs) demonstrate the presence of plasma at T ∼ 2−3×106 K and ne ∼ 1011−1013 cm−3, unobserved in non-accreting stars. Stationary models suggest that this emission is due to shockheated accreting material, but they do not allow to analyze the stability of such material and its position in the stellar atmosphere. Ai...
متن کاملHigh-energy γ-ray emission from gamma-ray bursts
GRBs are nowadays a rather well understood phenomenon in the soft (KeV-MeV) γ-ray energy band, while only a few GRBs have been observed at high photon energies (Eγ ∼ 1 GeV). It is also widely recognized that GRBs accelerate protons to relativistic energies and that dense media are often present nearby the sources. Within this framework and by further adopting Totani’s suggestion that GRB events...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Plasma Physics and Controlled Fusion
سال: 2022
ISSN: ['1361-6587', '0741-3335']
DOI: https://doi.org/10.1088/1361-6587/ac77b5