The cosmological dark matter, can be in the range from $10^6$ GeV up to $10^$ GeV. Proper value of the mass of the LSP-type particle, allowing it to make Depending on the channel of the scalaron decay the We have shown that particle production by oscillatingР”В¬urvature (scalaron) could significantly diminish the density of Realistic example we discuss $R^2$ inflationary model, suggested by Modified gravity theories which could lead to significant deviation of theР”В®xpansion regime from that in the conventional cosmology. In this connection it is interesting to consider

(LSP), is practically excluded by the recent lower bound on its mass In the canonical theory a naturalР”В¬andidate for dark matter, the lightest supersymmetric particle The frozen density of DM particles is determined by the

In this seminar I will illustrate how we can set out to create the interfaces to solve our difficult optimization problems, with great prospects for future endeavours that allow for time and resources to carry out such studies.Р”В¬osmological energy density of dark matter (DM) particles isР”Вetermined by their interaction strength, their mass, and the universeР”В®xpansion law.

Backpropagation through a differentiable pipeline of all the elements of the problem may allow to probe the design space and realign design and goals of experiments that base their operation on the interaction of radiation with matter, besides finding entirely new ways to solve our detection problems. Our saviour may be differentiable programming, which allows to create precise models of detectors, pattern recognition and inference extraction, cost, other constraints, and detector-related systematic uncertainties, as well as, crucially, a carefully constructed objective function. The result is a huge potential loss in performance. However, the construction choices live in a hundreds-dimensional parameter space which humans cannot probe. In addition, our technology nowadays allows for non-planar geometries and solutions that may significantly boost the performance of those devices. In the past few decades particle physics has made giant leaps by studying matter at the shortest distance scales with detectors built on a few paradigms (track-first-destroy-later, redundancy, cross-verification and calibration) which worked very well, but which today look increasingly misaligned with the progress of information-extraction procedures. The conference will be hosted in the Conference Center of the Orthodox Academy of Crete (OAC), an exceptionally beautiful location only a few meters from the Mediterranean sea. The conference will bring together worldwide experts and promising young scientists working on experimental and theoretical aspects of particle, nuclear, heavy ion and astro-particle physics and cosmology, with colleagues from other disciplines, for example, solid-state physics, mathematics, mathematical physics, quantum optics and other. The International Conference on New Frontiers in Physics aims to promote scientific exchange and the development of novel ideas in science with a particular accent in interdisciplinarity.

If needed we may add an extended internet-only session of ICNFP 2021.

2 September 2021, 18:00 Closing of physical ICNFP 2021.

24 AugustР’В 2021, 8:00 Opening of the main plenary session of ICNFP2021.

10th International Conference on New Frontiers in Physics (ICNFP 2021)

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