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Featured researches published by P. O. Hess.


Nuclear Physics | 1995

Neutrinoless double beta decay in heavy deformed nuclei

Jorge G. Hirsch; O. Castaños; P. O. Hess

Abstract The zero-neutrino mode of the double beta decay in heavy deformed nuclei is investigated in the framework of the pseudo-SU(3) model, which has provided an accurate description of collective nuclear structure and predicted half-lives for the two-neutrino mode in good agreement with experiments. In the case of 238U the calculated zero-neutrino half-life is at least three orders of magnitude greater than the two-neutrino one, giving strong support of the identification of the radiochemically determined half-life as being the two-neutrino double beta decay. For 150Nd the zero-neutrino matrix elements are of the order of magnitude of, but lesser than, those evaluated using the QRPA. This result confirms that different nuclear models produce similar zero-neutrino matrix elements, contrary to the two-neutrino case. Using these pseudo-SU(3) results and the upper limit for the neutrino mass we estimate the ββ0ν half-lives for six nuclei. An upper limit for majoron coupling constant is extracted from the experimental data.


Physical Review C | 1995

Double-beta decay of 100Mo: The deformed limit.

Jorge G. Hirsch; O. Castaños; P. O. Hess; Osvaldo Civitarese

The double beta decay of


Journal of Mathematical Physics | 1982

Complete set of states for microscopic nuclear collective models

O. Castaños; A. Frank; E. Chacón; P. O. Hess; Marcos Moshinsky

^{100}Mo


International Journal of Modern Physics E-nuclear Physics | 2012

PSEUDO-COMPLEX GENERAL RELATIVITY: SCHWARZSCHILD, REISSNER–NORDSTRÖM AND KERR SOLUTIONS

Gunther Caspar; Thomas Schönenbach; P. O. Hess; Mirko Schäfer; W. Greiner

to the ground state and excited states of


Nuclear Physics | 1991

Pseudo-symplectic model for strongly deformed heavy nuclei

O. Castaños; P. O. Hess; J. P. Draayer; P. Rochford

^{100}Ru


European Physical Journal A | 1991

Shape transitions and shape coexistence in the Ru and Hg chains

D. Troltenier; J. A. Maruhn; W. Greiner; V. Velazquez Aguilar; P. O. Hess; J. H. Hamilton

is analysed in the context of the pseudo SU(3) scheme. The results of this deformed limit are compared with the vibrational one based on the QRPA formalism. Consistency between the deformed limit and the experimental information is found for various


Journal of Mathematical Physics | 1984

Collectivity and geometry. II. The two‐dimensional case

E. Chacón; P. O. Hess; Marcos Moshinsky

\beta\beta


Nuclear Physics | 1995

Double-beta decay to excited states in 150Nd

Jorge G. Hirsch; O. Castaños; P. O. Hess; Osvaldo Civitarese

transitions, although, in this approximation some energies and B(E2) intensities cannot reproduced.


Monthly Notices of the Royal Astronomical Society | 2013

Experimental Tests of Pseudo-Complex General Relativity

Thomas Schönenbach; Gunther Caspar; P. O. Hess; Thomas Boller; Andreas Müller; Mirko Schäfer; W. Greiner

For several years the authors have been interested in determining complete sets of states for macroscopic nuclear collective models, such as the Bohr–Mottelson one (BM) and the interacting boson approximation (IBA), as well as in their use in nuclear structure calculations. In the present paper we obtain a complete set of states for microscopic nuclear collective models such as those of Vanagas and of Filippov and Smirnov. For calculations in these models, one requires a set of states for the A nucleon system, in appropriate coordinates which include the ones related with collective degrees of freedom. As is customary in nuclear physics, the complete set of states is derived more conveniently if one assumes an oscillator interaction between the nucleons. We obtain explicitly this set of states when A≫1, showing that it can be expressed in terms of wavefunctions whose dependence on the collective coordinates is similar to those appearing in the BM model and in the IBA. We briefly indicate how this set of s...


Physical Review C | 1997

Single- and double-beta decay Fermi transitions in an exactly solvable model

Jorge G. Hirsch; P. O. Hess; Osvaldo Civitarese

The pseudo-complex General Relativity (pc-GR) is further considered. A new projection method is proposed. It is shown that the pc-GR introduces automatically terms into the system which can be interpreted as dark energy. The modified pseudo-complex Schwarzschild solution is investigated. The dark energy part is treated as a liquid and possible solutions are discussed. As a consequence, the collapse of a large stellar mass into a singularity at r = 0 is avoided and no event-horizon is formed. Thus, black holes do not exist. The resulting object can be viewed as a gray star. It contains no singularity which emphasizes, again, that it is not a black hole. The corrections implied by a charged large mass object (Reissner–Nordstrom) and a rotating gray star (Kerr) are presented. For the latter, a special solution is presented. Finally, we will consider the orbital speed of a mass in a circular orbit and suggest a possible experimental verification.

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Osvaldo Civitarese

National Autonomous University of Mexico

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W. Greiner

Frankfurt Institute for Advanced Studies

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Jorge G. Hirsch

National Autonomous University of Mexico

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J. Cseh

Hungarian Academy of Sciences

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O. Castaños

National Autonomous University of Mexico

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A. Algora

Hungarian Academy of Sciences

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Judit Darai

University of Debrecen

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H. Yépez-Martínez

Universidad Autónoma de la Ciudad de México

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Mirko Schäfer

Goethe University Frankfurt

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W. Scheid

University of Giessen

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