• CORDIS Link / ESSnuSB+
  • CORDIS Link / ESSnuSB
  • Neutrino Conferences

ESSnuSB / ESSnuSB+

Funded by the European Union

  • ESSνSB proton accelerator Power (5MW):
    Image by Pete Linforth on Pixabay
    5.5 times the power of the most powerful road-going car Bugatti Veyron Super.
  • It will take the ESSνSB Super Beam proton pulse 1.8 ms=0.0018 seconds to reach the far detector if located at 540 km distance from ESS (Garpenberg mine) or 1.2ms=0.0012 seconds if located at 360km (Zinkgruvan mine).
    Image by Pete Linforth on Pixabay
  • ESSνSB Far Detector will be built 1km underground which is at a depth of about 3 times the height of the Eiffel Tower.
    Picture by Gerd Altmann on Pixabay
  • The ESS Linear Accelerator (Linac) is 490m long which represents around 4.7 times the length of a soccer field.
    Picture by Garik Barseghyan on Pixabay
  • ESSνSB Far Detector will contain 1 000 000 000 litres of water which represents a volume equal to that of a cube 100 m high and with a 100 m x 100 m bottom surface and is twice the volume that can be carried by the world largest super-tanker (TI Europe)
    Picture by Kai Kalhh on Pixabay
  • ESSνSB is the world's most intense neutrino beam project.
    Picture by Media Design and Media Publishing on Pixabay
  • What are neutrinos?
    Picture by Gerd Altmann on Pixabay
    The lightest fundamental particle.
  • Neutrinos are elusive and difficult to detect.
    Picture by Gerd Altmann on Pixabay
  • Neutrinos are plentiful: they come from everywhere, from the sun, from the earth, from supernovae and from the Big Bang.
    Image by Barbara A. Lane on Pixabay
  • Neutrinos travel as fast as light (almost!)
    Picture by Public Domain Pictures on Pixabay
  • Neutrinos have three different flavours: Electron, Muon, Tau.
    Picture by Gerd Altmann on Pixabay
  • Without the asymmetry between Matter and Antimatter we would not exist. How this symmetry was broken is an outstanding question?
    Picture by Gerd Altmann of Pixabay
    ESSνSB will study this question.
  • The years of major neutrino discoveries and years when those discoveries were awarded the Nobel Prizes:
    Picture by Gerd Altmann on Pixabay
    Pauli 1930/1945 : Prediction of neutrino
    Cowan & Reines 1956/1995: Discovery of neutrino.
    Davis & Koshiba 1987/2002: Solar & cosmic neutrinos.
    Kajita & McDonald 1998/2001/2015: Neutrino oscillations.
  • ESSνSB Timeline and funding obtained (till 2017) or required (as of 2022):
    Picture by Gerd Altmann on Pixabay
    2015: Concept (2M€)
    2019: Initial Design (5M€)
    2022: Final Design (10M€)
    2025: Construction of Detector (550M€)
    2028: Construction of Neutrino Source (650M€)
    2035-2085: Operational phase
    2012: First ideas
  • There were equal quantities of Matter and Antimatter created in the Big Bang.
    Image by Douglas James on Pixabay
    But there is no antimatter in the Universe now. Why?
  • Advantages of ESSνSB Project:
    Image by Douglas James on Pixabay
    - Hightest production intensity (5MW proton driver);
    - Largest detector (1 million tonnes of water);
    - Greatest sensitivity (measures at the 2nd neutrino oscillation maximum).
  • Picture by Wikilmages on Pixabay
    In ESSνSB project, a single beam pulse has the same energy as a 7.2kg bullet traveling at 1100 km/hour or, differently expressed, has the same kinetic energy as a 1000 kg car traveling at nearly 100 km/hour or the same heat energy it takes to melt 1000 kg of ice.
  • Picture by Wikilmages on Pixabay
    In the ESSνSB project, the duration of a super beam pulse will be 3 ms which means that there will be a distance of 900km (distance between Roma in Italy and Geneva in Switzerland) between the first and the last proton of the beam pulse.
  • Latest news
  • About us
  • ESSnuSB+ partnership
  • ESSnuSB+ Organisation
  • ESSnuSB+ at international events
  • Upcoming meetings
  • Twitter
  • ESSnuSB+ in media
  • Job offers
  • Glossary
  • Documents
  • ESSnuSB 2018-2022
    • ESSnuSB Organisation
      • Governing Board
      • Management Team
      • Executive Committee
      • ESSnuSB Dissemination & Exploitation Board
      • International Advisory Panel
      • Co-coordinators
    • ESSnuSB Work Packages
      • Definition
      • WP1 – Management Team
      • WP2 – Linac upgrade
      • WP3 – Accumulator
      • WP4 – Target Station
      • WP5 – Detector performance
      • WP6 – Physics Reach
    • ESSnuSB participants
      • On the map
      • People
      • Institutes and Organisations
    • Publications, Talks & Posters
      • Publications
      • Talks
      • Posters
    • The ESSnuSB Gazette
    • Past events
  • EuroNuNet
  • Neutrino Conferences
  • Outreach events
  • Recent publications
  • Contact Page

Latest news

ESSnuSB Input to the European Strategy for Particle Physics (ESPP) - 2026 update

ESSnuSB+ submitted its input to ESPP. It is available here.

-------------------------------------

Summer School on Neutrino Physics Beyond the Standard Model

Registration is open (deadline: 1 June 2025)

It is organised by Collaboration members and will be held on 29 June- 11 July 2025 at the Faculty of Physics and Engineering of the University of Strasbourg, France.

-------------------------------------

The 2025 ESSnuSB+ Annual Meeting will take place
on 22-26 September
at the George Eliopoulos Conference Centre,
Adamas, Greek island of Milos.

ESSnuSB+ at
international events

On 16 October 2024, the ESSnuSB+ Executive Committee was invited by Zinkgruvan Mining AB to visit the Zinkgruvan Mine, Sweden.

11 October 2024: ESSnuSB+ is founding a ground for future partnership cooperation with Hamamatsu Photonics

The ESSnuSB+ second Annual Meeting took place at the University of Hamburg, Germany, on 23-27 September 2024


ESSnuSB+ Flyer


The ESSnuSB+ first Annual Meeting was held
at CERN, Geneva, on 16-20 October 2023

The ESSnuSB Conceptual Design Report is now published by 

The European Physical Journal Special Topics

The new proposal, ESSnuSB+, submitted to the EU in April 2022, was approved in July 2022.

 Objectives and Ambitions of the new project :

The key objective of the H2020 ESSνSB Design Study was to demonstrate the feasibility of using the European Spallation Source proton linac to produce the world’s most intense neutrino beam concurrently with the 5 MW proton beam that will be used for the production of spallation neutrons.
After the production of all deliverables and the publication of the ESSνSB CDR, this is now accomplished. The present Design Study is proposed to pave the way of ESSνSB by introducing complementary studies and enlarging its scope by introducing investigations of synergetic projects.
The ESSνSB+ strategic objectives are:
1) Make all necessary civil engineering and geotechnical studies needed for the facility implementation of the ESSνSB/ESSνSB+ technical facilities at the ESS site and at the far detector side.
2) Study the implementation of a special target station for pion production and extraction for injection to a Low Energy nuSTORM decay ring and Low Energy Monitored Neutrino Beam decay tunnel.
3) Study the Low Energy nuSTORM decay ring and the injection of pions and muons coming from the special target station.
4) Study the Low Energy Monitored Neutrino Beam instrumented decay tunnel and the injection of pions coming from the special target station.
5) Study the design of a common detector for the Low Energy nuSTORM and for the Low Energy Monitored Neutrino Beam sub-projects for measurement of the neutrino cross-sections of interest.
6) Investigate the possibility of the utilisation of the Low Energy nuSTORM with its near detector and the ESSνSB near detector, already designed, for sterile neutrino searches.
7) Carry out studies of the geotechnical characteristics of the currently preferred site at Zinkgruvan for the underground ESSνSB far detector and study its potential for astroparticle physics programme.
8) Promote the ESSνSB/ESSνSB+ projects to their stakeholders, including scientists, politicians, funders, industrialists and the general public in order to have it included in the ESFRI list, which will allow to carry out extensive R&D work leading to a Technical Design Report for the whole facility.


The ESSnuSB+ Kick-off meeting took place at ESS (European Spallation Source), Lund, Sweden, on 17-18 January 2023


2018-2022 ESSnuSB Events

ESSnuSB looking for the answer.

https://youtu.be/qAnvft0nAlg

ESSnuSB Design Study Project

https://youtu.be/PwzNzLQh-Dw
  • Cukurova University
  • DEMOKRITOS NCSR
  • ESS Bilbao
  • CERN
  • Universität Hamburg UHH
  • Lulea University of Technology
  • ESS Lund
  • Lunds Universitet
  • Università di Milano Bicocca
  • Nagoya University
  • Università di Padova
  • INFN - Italy
  • Università di Roma Tre
  • Sofia University
  • KTH Stockholm
  • IPHC Strasbourg
  • CNRS - Strasbourg
  • Université de Strasbourg
  • AUTH - Thessaloniki
  • Uppsala Universitet
  • RBI - Ruder Boskovic Institute

ESSnuSB+ Work Packages 2023-2026

  • WP1 Management Team
  • WP2 Engineering & Infrastructure
  • WP3 Target Station & pion extraction
  • WP4 Low Energy nuSTORM
  • WP5 Detectors and physics reach
  • WP6 Low Energy Monitored Neutrino Beam

ESSnuSB Work Packages 2018-

  • WP1 – Management
  • WP2 – Linac upgrade
  • WP3 – Accumulator
  • WP4 – Target Station
  • WP5 – Detector performance
  • WP6 – Physics Reach

ESSNUSB+ CALENDAR

May 2025
MTWTFSS
    1 2 3 4
5 6 7 8 9 10 11
12 13 14 15 16 17 18
19 20 21 22 23 24 25
26 27 28 29 30 31  
« Apr   Jun »

Planned meetings

Links

  • CORDIS Link / ESSnuSB+
  • CORDIS Link / ESSnuSB
  • Neutrino Conferences
Copyright © 2025. ESSnuSB / ESSnuSB+
Powered By WordPress and Meritorious