• HOME
  • NEWS
  • EXPLORE
    • CAREER
      • Companies
      • Jobs
    • EVENTS
    • iGEM
      • News
      • Team
    • PHOTOS
    • VIDEO
    • WIKI
  • BLOG
  • COMMUNITY
    • FACEBOOK
    • INSTAGRAM
    • TWITTER
Tuesday, October 21, 2025
BIOENGINEER.ORG
No Result
View All Result
  • Login
  • HOME
  • NEWS
  • EXPLORE
    • CAREER
      • Companies
      • Jobs
        • Lecturer
        • PhD Studentship
        • Postdoc
        • Research Assistant
    • EVENTS
    • iGEM
      • News
      • Team
    • PHOTOS
    • VIDEO
    • WIKI
  • BLOG
  • COMMUNITY
    • FACEBOOK
    • INSTAGRAM
    • TWITTER
  • HOME
  • NEWS
  • EXPLORE
    • CAREER
      • Companies
      • Jobs
        • Lecturer
        • PhD Studentship
        • Postdoc
        • Research Assistant
    • EVENTS
    • iGEM
      • News
      • Team
    • PHOTOS
    • VIDEO
    • WIKI
  • BLOG
  • COMMUNITY
    • FACEBOOK
    • INSTAGRAM
    • TWITTER
No Result
View All Result
Bioengineer.org
No Result
View All Result
Home NEWS Science News Chemistry

How heavy elements come about in the universe

Bioengineer by Bioengineer
March 18, 2019
in Chemistry
Reading Time: 3 mins read
0
IMAGE
Share on FacebookShare on TwitterShare on LinkedinShare on RedditShare on Telegram

An experiment at GSI simulates how heavy elements capture protons

IMAGE

Credit: Mario Weigand

FRANKFURT. Heavy elements are produced during stellar explosion or on the surfaces of neutron stars through the capture of hydrogen nuclei (protons). This occurs at extremely high temperatures, but at relatively low energies. An international research team headed by Goethe University has now succeeded in investigating the capture of protons at the storage ring of the GSI Helmholtzzentrum für Schwerionenforschung.

As the scientists report in the current issue of Physical Review Letters, their goal was to determine more precisely the probability for a proton capture in astrophysical scenarios. As Dr. Jan Glorius from the GSI atomic physics research department explains, they were faced with two challenges in this endeavour: “The reactions are most probable under astrophysical circumstances in an energy range called the Gamow window. In this range, nuclei tend to be somewhat slow, making them difficult to obtain in the required intensity. In addition, the cross section – the probability of proton capture – decreases rapidly with energy. Until now, it has been almost impossible to create the right conditions in a laboratory for these kinds of reactions.”

René Reifarth, Professor for experimental astrophysics at Goethe University suggested a solution as early as ten years ago: The low energies within the Gamow window range can be reached more precisely when the heavy reaction partner circulates in an accelerator in which it interact with an stationary proton gas. He achieved first successes in September 2015 with a group of Heimholtz early career researchers. Since then, his team has gained excellent support from Professor Yuri Litvinov, who leads the EU-funded research project ASTRUm at GSI.

In the experiment, the international team first produced xenon ions. They were decelerated in the experimental storage ring ESR and caused to interact with protons. This resulted in reactions in which the xenon nuclei captured a proton and were transformed into heavier caesium – a process like that which occurs in astrophysical scenarios.

“The experiment makes a decisive contribution to advancing our understanding of nucleosynthesis in the cosmos,” says René Reifarth. “Thanks to the high-performance accelerator facility at GSI, we were able to improve the experimental technique for decelerating the heavy reaction partner. We now have more exact knowledge of the area in which the reaction rates occur, which until now had only been theoretically predicted. This allows us to more precisely model the production of elements in the universe.”

###

The experiment took place as part of the research collaboration SPARC (Stored Particles Atomic Physics Research Collaboration), which is part of the FAIR research programme. Equipment funded by the Verbundforschung (collaborative research) of the Federal Ministry for Education and Research was used in this experiment.

A picture can be downloaded here: http://www.uni-frankfurt.de/76756294

Caption: For the first time, the fusion of hydrogen and xenon was able to be investigated at the same temperatures as occur in stellar explosions using an ion storage ring.

Credit: Mario Weigand, Goethe-Universität

Publication:

J. Glorius et al: Approaching the Gamow window with stored ions: Direct measurement of 124Xe(p,γ) in the ESR storage ring, in PRL, DOI:10.1103/PhysRevLett.122.092701

Further information: Professor René Reifarth, Institute for Applied Physics at Goethe University, Riedberg Campus, Tel.: +49 69 798-47442, [email protected].

Current news about science, teaching, and society can be found on GOETHE-UNI online

Goethe University is a research-oriented university in the European financial centre Frankfurt am Main. The university was founded in 1914 through private funding, primarily from Jewish sponsors, and has since produced pioneering achievements in the areas of social sciences, sociology and economics, medicine, quantum physics, brain research, and labour law. It gained a unique level of autonomy on 1 January 2008 by returning to its historic roots as a “foundation university”. Today, it is one of the three largest universities in Germany. Together with the Technical University of Darmstadt and the University of Mainz, it is a partner in the inter-state strategic Rhine-Main University Alliance. Internet: http://www.uni-frankfurt.de

Publisher: The President of Goethe University Editor: Dr. Anne Hardy, Science Editor, PR & Communication Department, Theodor-W.-Adorno-Platz 1, 60323 Frankfurt am Main, Tel: +49 69 798-13035, Fax: +49 69 798-763 12531, , [email protected].

Media Contact
René Reifarth
[email protected]

Original Source

https://aktuelles.uni-frankfurt.de/englisch/physics-how-heavy-elements-come-about-in-the-universe/

Related Journal Article

http://dx.doi.org/10.1103/PhysRevLett.122.092701

Tags: AstrophysicsAtomic/Molecular/Particle PhysicsChemistry/Physics/Materials SciencesMolecular Physics
Share20Tweet8Share2ShareShareShare2

Related Posts

blank

Innovative Protective Coating for Spacecraft in Development by Engineers

October 20, 2025
blank

Scientists Uncover Life’s Building Blocks in Ice Surrounding a Forming Star in Nearby Galaxy

October 20, 2025

Copper-Catalyzed Asymmetric Cross-Coupling with Reactive Radicals

October 20, 2025

The Quantum Doorway Puzzle: Electrons Struggling to Find Their Exit

October 20, 2025
Please login to join discussion

POPULAR NEWS

  • Sperm MicroRNAs: Crucial Mediators of Paternal Exercise Capacity Transmission

    1268 shares
    Share 506 Tweet 317
  • Stinkbug Leg Organ Hosts Symbiotic Fungi That Protect Eggs from Parasitic Wasps

    301 shares
    Share 120 Tweet 75
  • New Study Suggests ALS and MS May Stem from Common Environmental Factor

    129 shares
    Share 52 Tweet 32
  • ESMO 2025: mRNA COVID Vaccines Enhance Efficacy of Cancer Immunotherapy

    118 shares
    Share 47 Tweet 30

About

We bring you the latest biotechnology news from best research centers and universities around the world. Check our website.

Follow us

Recent News

Modeling Wound Healing Through Strain-Induced MSC Differentiation

Ammonium Molybdate Hydrogel Boosts Photoenergy Harvesting

Unlocking Your Microbiome: The Key to Lifelong Health

Subscribe to Blog via Email

Enter your email address to subscribe to this blog and receive notifications of new posts by email.

Join 66 other subscribers
  • Contact Us

Bioengineer.org © Copyright 2023 All Rights Reserved.

Welcome Back!

Login to your account below

Forgotten Password?

Retrieve your password

Please enter your username or email address to reset your password.

Log In
No Result
View All Result
  • Homepages
    • Home Page 1
    • Home Page 2
  • News
  • National
  • Business
  • Health
  • Lifestyle
  • Science

Bioengineer.org © Copyright 2023 All Rights Reserved.