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XENON

The XENON dark matter search project

It is know from numerous astronomical and cosmological observations that the vast majority of the energy content of the Universe is dark: so far it is invisible to our detectors. About 70% is the mysterious dark energy, responsible for the accelerated expansion of the cosmos, and about 25% is made of dark matter. This yet unknown form of matter builds large scale structures in the Universe and dominates the dynamics of galaxies and galaxy clusters. Only 5% is made from ordinary matter such as protons, neutrons, and electrons which build atoms, molecules and eventually our "known" world.

We participate in the XENON dark matter project, which aims to directly detect the particle making up the dark matter and which should be present in our cosmic neighborhood in large amounts. Its interaction probability with normal matter, and hence with particle detectors, must be extremely weak, otherwise the dark matter would not be dark. However, there are plenty of models which predict that there should be a very small interaction probability. One promising candidate is the WIMP (weakly interacting massive particle), which arises naturally in many extensions of the standard model of particle physics.

LNGS: The Laboratory

The expected interaction rate in our detector is very low, but backgrounds are large since natural radioactivity is everywhere in the environment and cosmic rays also interact with detectors. Therefore, we need a detector with an ultra-low background. In order to achieve this, the XENON detectors are placed deep underground in the Italian Gran Sasso Laboratory (LNGS, in the Abbruzzian mountains) which reduces the rate of cosmic ray muons by six orders of magnitude.

Fig: The XENON installations in Hall B of LNGS.

The detection principle

The XENON instruments are dual-phase time projection chambers (TPC) filled with ultra-pure xenon, which has been liquefied by cooling it to about -95°C. When a particle interacts with the xenon, it creates scintillation light and liberates electrons by ionization. Both signals, scintillation and ionization, are detected by a large number of photosensors. They are used to determine the energy deposition, the number of interactions in the detector, their 3-dimensional interaction vertex, and whether the particle looks more signal- or more background-like.

The combination of these features, together with a careful detector design and selection of all construction materials, allows achieving very low radioactive background levels - one of the prime advantages of this detector technology.

XENON1T: the instrument

The XENON collaboration has installed the next-generation dark matter detector XENON1T in November 2015 and is currently in dark matter mode. XENON1T is about 35x larger than its predecessor XENON100 (in terms of target mass) and uses a total of 3.5t of liquid xenon. The larger mass, together with a very low background, will allow us to increase its sensitivity to dark matter interactions by a factor 100 compared to XENON100, and by more than an order of magnitude compared to the current best results.

The first results from the first science run of 34 live days were released in May 2017. No indications for dark matter interactions were found and the strongest limits for WIMP masses above 10 GeV/c² were thus placed (publication).

Fig: Assembly of the XENON1T inner detector (TPC).

The main responsibilities of the Freiburg group are:

  • Data acquisition and electronics: We are responsible for the electronics and the data acquisition system for XENON1T. We have developed an asynchronous trigger-less readout system with virtually no threshold.
  • Detector design: We have led the design of the time projection chamber (TPC) of XENON1T. This is the innermost part of the detector which contains the active dark matter target. We are also involved in the development of low-radioactive detector components.
  • Data analysis: XENON1T is the largest and most sensitive dark matter detector world-wide and we contribute to analyse its data.

Have a look at a short movie of the XENON1T construction: The XENON1T Story

XENON is an international collaboration with more than 160 members from Germany, USA, Italy, Portugal, Switzerland, France, the Netherlands, Sweden, UAE, Israel, and Japan.

Further Information

Official XENON website
Local XENON website

Dark Matter and Dual-phase Liquid Xenon Detectors

  • Dark Matter: M. Schumann, EPJ Web Conf. 96, 01027 (2015), arXiv:1501.01200.
  • Liquid Xenon Detectors: M. Schumann, JINST 9, C08004 (2014), arXiv:1405.7600.

XENON1T

  • XENON1T: Results from Science Run 1
    E. Aprile et al. (XENON1T Collaboration), arXiv:1705.06655
  • XENON1T Sensitivity:
    E. Aprile et al. (XENON1T Collaboration), JCAP 04, 027 (2016), arXiv:1512.07501

XENON100

  • XENON100 Instrument Paper:
    E. Aprile et al. (XENON100), Astropart. Phys. 35, 573 (2012), arXiv:1107.2155.
  • XENON100 WIMP result:
    E. Aprile et al. (XENON100), Phys. Rev. Lett. 109, 131801 (2012), arXiv:1207.5988.
  • Annual Modulation Analysis:
    E. Aprile et al. (XENON00), Phys. Rev. Lett. 115, 091302 (2015), arXiv:1507.07748.