Results 1 to 10 of about 2,752,786 (196)
Progress in Jinping Underground Nuclear Astrophysics Experiment
Nuclear astrophysics is an interdisciplinary subject of nuclear physics and astrophysics. As the forefront of fundamental research, it has played an important role in the process of deepening understanding of the universe and stellar evolution.
LIAN Gang;GUO Bing;SHEN Yangping;SU Jun;LI Zhihong;HE Jianjun;TANG Xiaodong;CUI Baoqun;SUN Liangting;AN Zhu;LIU Weiping
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Formation of CO2 Driven by Photochemistry of Water Ice Mixed with Carbon Grains
We present results on photochemistry of carbon-grains/water-ice mixtures at temperatures from 10 to 150 K. Such a temperature range corresponds to the physical conditions found in molecular clouds, hot cores and corinos, protostellar envelopes, and ...
Alexey Potapov +3 more
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In this paper we discuss the magnetic field self generation, via the so-called Biermann battery effect, and its diffusion for a blast wave (BW) expanding in a perturbed background medium.
A Marocchino, S Atzeni, A Schiavi
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The recent astronomical detection of ethynylbutatrienylidene (HCCCHCCC)—a high-energy isomer of triacetylene (HCCCCCCH) and hexapentaenylidene (H _2 CCCCCC)—in TMC-1 puzzled the laboratory astrophysics community since proposed reaction pathways could not
Alexander M. Mebel +3 more
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Double to Tenfold M-shell Photoionization of Singly Charged Lanthanum Ions
Using the photon-ion merged-beams technique at the PETRA III synchrotron light source, we have measured cross sections for double and up to tenfold photoionization of La ^+ ions by a single photon in the energy range 820–1400 eV, where resonances and ...
Mirko Looshorn +11 more
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Detectors and Shieldings: Past and Future at LUNA
Nuclear reactions are responsible for the chemical evolution of stars, galaxies and the Universe. Unfortunately, at temperatures of interest for nuclear astrophysics, the cross-sections of the thermonuclear reactions are in the pico- femto-barn range and
Chemseddine Ananna +13 more
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Nuclear astrophysics at Gran Sasso Laboratory: the LUNA experiment
LUNA is an experimental approach for the study of nuclear fusion reactions based on an underground accelerator laboratory. Aim of the experiment is the direct measurement of the cross section of nuclear reactions relevant for stellar and primordial ...
Cavanna Francesca
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ISO and Laboratory Astrophysics [PDF]
ISO, the Infrared Space Observatory is capable of measuring spectra across most of the mid-infrared, the region from 4000 to 500 cm−1 (2.5-20 μm). Of these 3500 cm−1, about 670 have been inaccessible to astronomers due to strong atmospheric absorptions and about 750 cm−1 require an airborne platform, making access limited. ISO will provide high quality
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Advances in instrumentation for nuclear astrophysics
The study of the nuclear physics properties which govern energy generation and nucleosynthesis in the astrophysical phenomena we observe in the universe is crucial to understanding how these objects behave and how the chemical history of the universe ...
S. D. Pain
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Laboratory Astrophysics in Europe
Europe has a broad activity in Laboratory Astrophysics, covering theory and experiment, as well initiatives promoting open science, including databases and tools aiding connection to astrophysical modelling and interpretation of observations. The talk will present some examples of Laboratory Astrophysics in Europe, as well as examples of organisation ...
Barklem, Paul, Dubernet, Marie-Lise
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