In recent months, we have been hearing a lot of news on a topic that has been characterized by a long silence for decades, Lars Jaeger writes in an essay on finews.first.


This article is published on finews.first, a forum for authors specialized in economic and financial topics.


On one and the same day (January 26, 2022), almost all press organs carried headlines such as:

  • ‹Burning› hydrogen plasma in the world’s largest laser sets fusion records
  • Nuclear fusion milestone creates ‹burning plasma› for the first time
  • Physicists create self-burning plasma – but is it a step toward sustainable nuclear fusion energy?
  • Scientists reach a major milestone in harnessing fusion energy

Progress in nuclear fusion (as opposed to nuclear fission, on which today’s controversial nuclear power generation is based) is of great importance because nuclear fusion offers the possibility of safe and (almost) climate-neutral energy generation.

Yet the history of nuclear fusion research is already more than 80 years old. Since the 1930s, physicists have known that hydrogen nuclei fuse to form helium atomic nuclei under very high pressure and temperature – and that it is this mechanism (as well as the fusion of larger atomic nuclei) that enables the sun to generate its enormous amounts of energy.

«In fact, this corresponds to the reactions in the interior of the sun»

Recent headlines have specifically focused on the achievement of scientists at the National Ignition Facility (NIF) at Lawrence Livermore National Laboratory in Northern California. Here, a high-power laser was used to create for the first time a «burning plasma», demonstrating for a (very) brief moment how the «fuel», i.e. the combination of deuterium and tritium, can be made to undergo nuclear fusion and thus produce energy.

The energy achieved here was much of the energy required to sustain the nuclear reaction. This corresponds to the reactions in the interior of the sun, whereby here on earth the problem is that for the production of these reactions enormously high energy quantities or densities are necessary at first, in order to set the process in motion, which then maintains itself (on suns of a certain size this is caused automatically by the enormously high gravitational force).

«Here, it is more of a traditional fusion approach»

Just a few months earlier, incidentally, there had been a similar wave of newspaper articles on nuclear fusion. The trigger here was the Boston-based company Commonwealth Fusion Systems (CFS), a spin-off of MIT, which received more than a billion dollars from investors such as Bill Gates and George Soros, as it communicated. The way these nuclear fusion works is quite different from NIF’s.

Here, it is more of a traditional fusion approach, building a donut-shaped «tokamak» reactor, a «big magnetic bottle», according to CFS’s CEO Bob Mumgaard, in which powerful magnetic fields control spheres in plasma that’s about 100 million degrees hot, which should produce the same fusion of hydrogen isotope nuclei as in the laser-driven reactor.

Mumgaard said they will have a working reactor in six years basing his optimism on CFS’s successful 2021 summer test of new electromagnets made with barium-copper-oxide superconductors.

«Jeff Bezos backs General Fusion»

However, there will almost certainly be room for more than one fusion winner. Other companies include Canada-based General Fusion, backed by Jeff Bezos, which received $130 million from investors in 2021.

And then there is TAE Energy in California, which is arguably the furthest along with commercially successful nuclear fusion, having already experimented with it at a cost of $1 billion over the past twenty years and now, with having successfully raised more money, plans to build the first permanently operational nuclear fusion reactor within the next three years, which they are already calling «Copernicus».

«Otherwise, investors would hardly put so much money into it»

The fact that investors are now willing to put up several billion dollars of private capital for the next round of funding for the development of nuclear fusion energy machines (with a correspondingly high expected return) shows that they expect to see commercially viable nuclear fusion in five or only a little more years. Otherwise, they would hardly put so much money into it. Commercially available fusion technology, if it were actually available to us one day – and perhaps soon – would mean a paradigm shift in society.

If we were actually able to produce energy like the sun and thus gain access to the most efficient, safest and environmentally-friendly form of energy that nature has to offer, this would certainly not only be another major technological advance, but rather a leap forward in a civilization that would be on a par with the invention of the steam engine, which 250 years ago gave us the energy to completely turn our society upside down.


Lars Jaeger is a Swiss-German author and investment manager. He writes on the history and philosophy of science and technology and has in the past been an author on hedge funds, quantitative investing, and risk management. He just recently published his latest book: «Wege aus der Klimakatastrophe».


Previous contributions: Rudi Bogni, Peter Kurer, Rolf Banz, Dieter Ruloff, Werner Vogt, Walter Wittmann, Alfred Mettler, Robert Holzach, Craig Murray, David Zollinger, Arthur Bolliger, Beat Kappeler, Chris Rowe, Stefan Gerlach, Marc Lussy, Nuno Fernandes, Richard Egger, Maurice Pedergnana, Marco Bargel, Steve Hanke, Urs Schoettli, Ursula Finsterwald, Stefan Kreuzkamp, Oliver Bussmann, Michael Benz, Albert Steck, Martin Dahinden, Thomas Fedier, Alfred MettlerBrigitte Strebel, Mirjam Staub-Bisang, Nicolas Roth, Thorsten Polleit, Kim Iskyan, Stephen Dover, Denise Kenyon-Rouvinez, Christian Dreyer, Kinan Khadam-Al-Jame, Robert HemmiAnton AffentrangerYves Mirabaud, Katharina Bart, Frédéric Papp, Hans-Martin Kraus, Gerard Guerdat, Mario Bassi, Stephen Thariyan, Dan Steinbock, Rino BoriniBert Flossbach, Michael Hasenstab, Guido Schilling, Werner E. RutschDorte Bech Vizard, Adriano B. Lucatelli, Katharina Bart, Maya Bhandari, Jean Tirole, Hans Jakob RothMarco Martinelli, Thomas SutterTom KingWerner Peyer, Thomas Kupfer, Peter KurerArturo BrisFrederic PappJames Syme, Dennis Larsen, Bernd Kramer, Armin JansNicolas Roth, Hans Ulrich Jost, Patrick Hunger, Fabrizio QuirighettiClaire Shaw, Peter FanconiAlex Wolf, Dan Steinbock, Patrick Scheurle, Sandro Occhilupo, Will Ballard, Nicholas Yeo, Claude-Alain Margelisch, Jean-François Hirschel, Jens Pongratz, Samuel Gerber, Philipp Weckherlin, Anne Richards, Antoni Trenchev, Benoit Barbereau, Pascal R. Bersier, Shaul Lifshitz, Klaus Breiner, Ana Botín, Martin Gilbert, Jesper Koll, Ingo Rauser, Carlo Capaul, Claude Baumann, Markus Winkler, Konrad Hummler, Thomas Steinemann, Christina Boeck, Guillaume Compeyron, Miro Zivkovic, Alexander F. Wagner, Eric Heymann, Christoph Sax, Felix Brem, Jochen Moebert, Jacques-Aurélien Marcireau, Ursula Finsterwald, Claudia Kraaz, Michel Longhini, Stefan Blum, Zsolt Kohalmi, Karin M. Klossek, Nicolas Ramelet, Søren Bjønness, Andreas Britt, Gilles Prince, Salman Ahmed, Stephane Monier, and Peter van der Welle, Ken Orchard, Christian Gast, Jeffrey Bohn, Juergen Braunstein, Jeff Voegeli, Fiona Frick, Stefan Schneider, Matthias Hunn, Andreas Vetsch, Fabiana Fedeli, Marionna WegensteinKim Fournais, Carole Millet, Swetha Ramachandran, Brigitte Kaps, Thomas Stucki, Neil Shearing, Claude Baumann, Tom Naratil, Oliver Berger, Robert Sharps, Tobias Mueller, Florian Wicki, Jean Keller, Niels Lan Doky, Karin M. Klossek, Johnny El Hachem, Judith Basad, Katharina Bart, Thorsten Polleit, Bernardo Brunschwiler, Peter Schmid, Karam Hinduja, Zsolt Kohalmi, Raphaël Surber, Santosh Brivio, Mark Urquhart, Olivier Kessler, Bruno Capone, Peter Hody, Andrew Isbester, Florin Baeriswyl, and Michael Bornhaeusser, Agnieszka Walorska, Thomas Mueller, Ebrahim Attarzadeh, Marcel HostettlerHui Zhang, Michael Bornhaeusser, Reto Jauch, Angela Agostini, Guy de Blonay, Tatjana Greil Castro, Jean-Baptiste Berthon, Marc Saint John Webb, Dietrich Goenemeyer, Mobeen Tahir, Didier Saint-Georges, Serge Tabachnik, Rolando Grandi, Vega Ibanez, David Folkerts-Landau, Andreas Ita, Teodoro Cocca, Michael Welti, Mihkel Vitsur, Fabrizio Pagani, Roman Balzan, Todd Saligman, Christian Kaelin, Stuart Dunbar, Fernando Fernández, Carina Schaurte, Birte Orth-Freese, Gun Woo, Lamara von Albertini, Philip Adler, Ramon Vogt, Gérard Piasko, Andrea Hoffmann, Niccolò Garzelli, Darren Williams, Benjamin Böhner, Mike Judith, Gregoire Bordier, Jared Cook, Henk Grootveld, Roman Gaus, Nicolas Faller, Anna Stünzi, Philipp Kaupke, Thomas Höhne-Sparborth, Fabrizio Pagani, Taimur Hyat, Ralph Ebert, Guy de Blonay, Lars Jaeger, Jan Boudewijns, Beat Wittmann, Sean Hagerty, Alina Donets, and Sébastien Galy.