Investigating the possible existence of hyper-heavy nuclei in a neutron-star environment-Reference-Cited by-同舟云学术

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Investigating the possible existence of hyper-heavy nuclei in a neutron-star environment

Published:2022-07-18 Issue:1 Volume:106 Page:
ISSN:2469-9985
Container-title:Physical Review C
language:en
Short-container-title:Phys. Rev. C

Author:

Veselský M.^ORCID,Petousis V.^ORCID,Moustakidis Ch. C.^ORCID,Souliotis G. A.^ORCID,Bonasera A.^ORCID

Funder

Grantová Agentura České Republiky

U.S. Department of Energy

National Nuclear Security Administration

České Vysoké Učení Technické v Praze

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.106.L012802/fulltext

Reference30 articles.

1. Foreword

2. Colloquium : Superheavy elements: Oganesson and beyond

3. Superheavy and hyperheavy nuclei in the form of bubbles or semi-bubbles

4. The Ground State of Matter at High Densities: Equation of State and Stellar Models

5. Neutron star inner crust: Nuclear physics input

Cited by 3 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Superheavy elements and ultradense matter;The European Physical Journal Plus;2023-09-15

2. Novel Concepts of Nuclear Physics in a Neutron Star Environment;The 2nd Electronic Conference on Universe;2023-02-17

3. Investigating the possible existence of hyper-heavy nuclei in a neutron-star environment;Physical Review C;2022-07-18

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