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Black Hole

Lensing of space time around a black hole. At Oxford we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Dr Konstantinos Tanidis

Visitor

Research theme

  • Particle astrophysics & cosmology

Sub department

  • Astrophysics

Research groups

  • Beecroft Institute for Particle Astrophysics and Cosmology
  • Euclid
konstantinos.tanidis@physics.ox.ac.uk
Denys Wilkinson Building, room 555A
  • About
  • Publications

Constraining ultra-high-energy cosmic ray composition through cross-correlations

Journal of Cosmology and Astroparticle Physics IOP Publishing 2022:12 (2022) 003-003

Authors:

Konstantinos Tanidis, Federico R Urban, Stefano Camera

Abstract:

Abstract The chemical composition of the highest end of the ultra-high-energy cosmic ray spectrum is very hard to measure experimentally, and to this day it remains mostly unknown. Since the trajectories of ultra-high-energy cosmic rays are deflected in the magnetic field of the Galaxy by an angle that depends on their atomic number Z, it could be possible to indirectly measure Z by quantifying the amount of such magnetic deflections. In this paper we show that, using the angular harmonic cross-correlation between ultra-high-energy cosmic rays and galaxies, we could effectively distinguish different atomic numbers with current data. As an example, we show how, if Z = 1, the cross-correlation can exclude a 39% fraction of Fe56 nuclei at 2σ for rays above 100 EeV.
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Constraining a late time transition of Geff using low-z galaxy survey data

Phys. Rev. D 106, 023526

Authors:

G. Alestas, L. Perivolaropoulos, K. Tanidis

Abstract:

It has recently been pointed out that a gravitational transition taking place at a recent redshift zt, reducing the effective gravitational constant Geff by about 10% for z>zt, has the potential to lead to a resolution of the Hubble tension if zt≲0.01. Since H(z)2∼Geff, such a transition would also lead to sharp change of the slope of the Hubble diagram at z=zt and a sharp decrease in the number of galaxies per redshift bin at zt. Here we attempt to impose constraints on such a transition by using two robust low-z redshift survey datasets (z<0.01), taken from the Six-degree Field Galaxy Survey (6dFGS) as well as the 2MASS Redshift Survey (2MRS). In both surveys, we bin the data in redshift bins and focus on the number of galaxies in each bin (ΔN(zi)). We observe a peak in the distribution of galaxies near a distance of approximately 20 Mpc in both datasets. This feature could be attributed to galactic density fluctuations, to coherent peculiar velocities of galaxies or to an ultra late-time gravitational transition in the same era. In the context of the later scenario we show that this feature could have been induced by a sharp change of Geff by ΔGeff/Geff≃0.6 at zt≃0.005. Thus, in a conservative approach, this method can be used to impose constraints on a possible abrupt change of the gravitational constant taking place at very low redshifts.
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Constraining ultra-high-energy cosmic ray composition through cross-correlations

ArXiv 2203.09538 (2022)

Authors:

Konstantinos Tanidis, Federico R Urban, Stefano Camera
Details from ArXiV

Constraining a late time transition of $G_{\rm eff}$ using low-z galaxy survey data

ArXiv 2201.05846 (2022)

Authors:

G Alestas, L Perivolaropoulos, K Tanidis
Details from ArXiV

EuCAPT White Paper: Opportunities and Challenges for Theoretical Astroparticle Physics in the Next Decade

ArXiv preprint. White paper of the European Consortium for Astroparticle Theory (EuCAPT). 135 authors, 400 endorsers, 133 pages, 1382 references

Authors:

R. Alves Batista, M. A. Amin, G. Barenboim, N. Bartolo, D. Baumann, A. Bauswein, E. Bellini, D. Benisty, G. Bertone, P. Blasi, C.G. Böhmer, Ž. Bošnjak, T. Bringmann, C. Burrage, M. Bustamante, J. Calderón Bustillo, C. T. Byrnes, F. Calore, R. Catena, D. G. Cerdeño, S. S. Cerri, M. Chianese, K. Clough, A. Cole, P. Coloma, A. Coogan, L. Covi, D. Cutting, A.C. Davis, C. de Rham, A. di Matteo, G. Domènech, M. Drewes, T. Dietrich, T. D. P. Edwards, I. Esteban, R. Erdem, C. Evoli, M. Fasiello, S. M. Feeney, R. Z. Ferreira, A. Fialkov, N. Fornengo, S. Gabici, T. Galatyuk, D.Gaggero, D. Grasso, C. Guépin, J. Harz, M. Herrero-Valea, T. Hinderer, N. B. Hogg, D. C. Hooper, F. Iocco, J. Isern, K. Karchev, B. J. Kavanagh, M. Korsmeier, K. Kotera, K. Koyama, B. Krishnan, J. Lesgourgues, J. Levi Said, L. Lombriser, C. S. Lorenz, S. Manconi, M. Mapelli, A. Marcowith, S. B. Markoff, D. J. E. Marsh, M. Martinelli, C.J.A.P. Martins, J. H. Matthews, A. Meli, O. Mena, J. Mifsud, M. M. Miller Bertolami, P. Millington, P. Moesta, K. Nippel, V. Niro, E. O'Connor, F. Oikonomou, C. F. Paganini, G. Pagliaroli, P. Pani, C. Pfrommer, S. Pascoli, L. Pinol, L. Pizzuti, R. A. Porto, A. Pound, F. Quevedo, G. G. Raffelt, A. Raccanelli, E. Ramirez-Ruiz, M. Raveri, S. Renaux-Petel, A. Ricciardone, A. Rida Khalifeh , A. Riotto, R. Roiban, J. Rubio, M. Sahlén, N. Sabti, L. Sagunski, N. Šarčević, K. Schmitz, P. Schwaller, T. Schwetz, A. Sedrakian, E. Sellentin, A. Serenelli, P.D. Serpico, E. I. Sfakianakis, S. Shalgar, A. Silvestri, I. Tamborra, K. Tanidis, D. Teresi, A. A. Tokareva, L. Tolos, S. Trojanowski, R. Trotta, C. Uhlemann, F. R. Urban, F. Vernizzi, A. van Vliet, F. L. Villante, A. Vincent, J. Vink, E. Vitagliano, C. Weniger, A. Wickenbrock, W. Winter, S. Zell, M. Zeng

Abstract:

Astroparticle physics is undergoing a profound transformation, due to a series of extraordinary new results, such as the discovery of high-energy cosmic neutrinos with IceCube, the direct detection of gravitational waves with LIGO and Virgo, and many others. This white paper is the result of a collaborative effort that involved hundreds of theoretical astroparticle physicists and cosmologists, under the coordination of the European Consortium for Astroparticle Theory (EuCAPT). Addressed to the whole astroparticle physics community, it explores upcoming theoretical opportunities and challenges for our field of research, with particular emphasis on the possible synergies among different subfields, and the prospects for solving the most fundamental open questions with multi-messenger observations.
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