Celebrating 40 years of Milgromian dynamics and charting the road ahead:

opportunities and challenges in galaxies and cosmology

Hosted in St Andrews, Monday 5th June - Friday 9th June 2023



The source of the gravitational field in objects ranging from individual galaxies to the largest scales in the universe is one of the biggest unanswered questions of modern physics. It is generally assumed that the gravitational field in extragalactic systems is dominated by dark matter particles occupying a dark sector that represents new physics beyond the stubbornly successful Standard Model of particle physics. So far, candidates for these particles have evaded detection in remarkably sensitive laboratory experiments: the evidence for missing mass remains entirely astrophysical in nature.

Forty years ago, Weizmann-Institute professor Mordehai Milgrom published a series of three articles in The Astrophysical Journal in which he proposed that the dark matter phenomenon is not due to unknown particles, but to a departure from the known laws of dynamics when the acceleration is about eleven orders of magnitude smaller than that on Earth's surface (Milgrom 1983). Only one year later, in 1984, Jacob Bekenstein and Mordehai Milgrom developed this Modified Newtonian Dynamics (or Milgromian Dynamics, MOND) into a non-relativistic Lagrangian theory (Bekenstein & Milgrom 1984). During the ensuing decades, MOND has developed into a multifaceted paradigm that includes several non-relativistic and relativistic theory proposals, as well as possible connections with quantum gravity theories. Most remarkably, MOND has successfully made many striking and unique a priori predictions.

This conference will commemorate the last 40 years of this modern gravitational paradigm, of its predictive successes as well as its outstanding challenges, and will look to the road ahead.

Topics of the conference will include:

  • Observational tests of MOND in galaxies of all types, including our own Milky Way
  • Observational tests of MOND in galaxy clusters and galaxy groups, including our own Local Group
  • Numerical simulations of galaxy formation and evolution in MOND
  • Relativistic extensions of MOND, cosmology, and the Cosmic Microwave Background
  • Foundations of MOND and links with quantum physics
  • Philosophical and sociological aspects of MOND

Keynote speakers:

This conference will be held in St Andrews and follows similar previous conferences in Edinburgh (2006), Strasbourg (2010 and 2015), Cleveland (2017) and Bonn (2019).

The conference is supported by the School of Physics and Astronomy at the University of St Andrews and the SPODYR group at the University of Bonn.

Registration and Abstract Submission

Registration and abstract submission for this event have now closed. Please only use the abstract form to update previously submitted details here.


The programme for this event is available here. An informal meeting has been arranged at The Rule pub on South Street at 6-9 p.m. on Sunday 4th June 2023, please walk straight through to the back if you would like to come. There will be a wine reception and conference dinner on Wednesday 7th June 2023 in Lower College Hall. Invited talks will take up to 45 minutes and contributed talks will take up to 20 minutes, which in both cases does not include questions.

Posters are permitted up to a maximum size of A0 portrait. Poster presenters will receive separate instructions about how to request an announcement of their poster to the other conference delegates in a maximum 2 minute talk without slides.

Delegates who do not wish to attend the conference dinner should contact organiser Dr. Banik (ib45@st-andrews.ac.uk) at least two weeks before the conference starts so that a cash refund can be arranged.


Accommodation arranged by the University will be available to all guests from June 1st to June 13th and can be booked here. This will cost about £50 per night using the discount code MOND40 and should be booked by the end of April 2023. Guests who wish to arrange their own accommodation should be warned that hotel prices in St Andrews can be inflated during the golfing season in Summer.

Note: International visitors should bring an electrical adaptor so they can use the three-pin British sockets.

Location and Travel


The conference will take place in Lecture Theatre B at the School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, KY16 9SS. A map of University buildings can be found here. St Andrews itself is a small town and can be crossed on foot in about 25 minutes.

Travel connections

St Andrews is well connected to the rest of Scotland through bus routes. Most bus services terminate at the Bus Station, which is a 5 minute walk from the School of Physics and Astronomy.
The nearest train station is Leuchars, which is 5 miles away. There is a regular bus service (route 99) to the town from this station, along with a taxi rank (at St Andrews the taxi ranks are on Bell Street and in front of Holy Trinity Church on South Street). Leuchars is easily accesible from several major train stations, including direct train links from London King's Cross and Edinburgh Waverley. There is also a direct train service from Edinburgh Gateway for those who fly in to Edinburgh airport.
Further travel details can be found on the University's website.

Conference Poster


The conference poster can be downloaded here.



Francoise Combes (Chair, Paris Observatory), Indranil Banik (St Andrews), James Binney (Oxford), Benoit Famaey (Strasbourg), Lavinia Heisenberg (ETH Zurich), Federico Lelli (Florence), Stacy McGaugh (CWRU), Xufen Wu (Hefei), Hongsheng Zhao (St Andrews)


Elena Asencio, Indranil Banik (head), Alfie Russell