Theo J. Mertzimekis

Prof. Dr. Theo J. Mertzimekis

Department of Physics, University of Athens, GR-15784 Athens, Greece
orcid

Research Focus & Metrics

Academic Career Length

31Years (1996-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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13 August 2013 in Scientific Reports
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SKStephanos Kilias
Stephanos Kilias
PNParaskevi Nomikou
Paraskevi Nomikou
DPDimitrios Papanikolaou
Dimitrios Papanikolaou
PPParaskevi Polymenakou
Paraskevi Polymenakou
Athanasios GodelitsasAthanasios Godelitsas
Athanasios Godelitsas
MSMichael Scoullos
Michael Scoullos
We report on integrated geomorphological, mineralogical, geochemical and biological investigations of the hydrothermal vent field located on the floor of the density-stratified acidic (pH ~ 5) crater of the Kolumbo shallow-submarine arc-volcano, near Santorini. Kolumbo features rare geodynamic setting at convergent boundaries, where arc-volcanism and seafloor hydrothermal activity are occurring in thinned continental crust. Special focus is given to unique enrichments of polymetallic spires in Sb and Tl (±Hg, As, Au, Ag, Zn) indicating a new hybrid seafloor analogue of epithermal-to-volcanic-hosted-massive-sulphide deposits. Iron microbial-mat analyses reveal dominating ferrihydrite-type phases, and high-proportion of microbial sequences akin to "Nitrosopumilus maritimus", a mesophilic Thaumarchaeota strain capable of chemoautotrophic growth on hydrothermal ammonia and CO2. Our findings highlight that acidic shallow-submarine hydrothermal vents nourish marine ecosystems in which nitrifying Archaea are important and suggest ferrihydrite-type Fe3+-(hydrated)-oxyhydroxides in associated low-temperature iron mats are formed by anaerobic Fe2+-oxidation, dependent on microbially produced nitrate.

22 January 2002 in Physical Review C
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GJG. Jakob
G. Jakob
NBN. Benczer-Koller
N. Benczer-Koller
GKG. Kumbartzki
G. Kumbartzki
JHJ. Holden
J. Holden
Theo J. MertzimekisTheo J. Mertzimekis
Theo J. Mertzimekis
ILI. Y. Lee
I. Y. Lee
The g factors of 21+, 41+, and 22+ states in the stable 130,132,134,136Xe isotopes have been measured via projectile Coulomb excitation in inverse kinematics in combination with the transient field technique. The results show a steady decrease in g(21+) as the number of neutron holes increases in the lighter nuclei below the closed N=82 neutron shell. The g factors of the 41+ states in 132,134Xe are consistently larger than the g factors of the 21+ states, a characteristic of proton excitation. The g factors of the 21+, 41+, and 22+ states in 130Xe are approximately equal as would be expected for vibrational excitations.

2 March 2021 in The European Physical Journal A
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AMAndriana Martinou
Andriana Martinou
DBDennis Bonatsos
Dennis Bonatsos
Theo J. MertzimekisTheo J. Mertzimekis
Theo J. Mertzimekis
KKK. E. Karakatsanis
K. E. Karakatsanis
IAI. E. Assimakis
I. E. Assimakis
NMN. Minkov
N. Minkov

17 July 2001 in Physical Review C
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Theo J. MertzimekisTheo J. Mertzimekis
Theo J. Mertzimekis
NBN. Benczer-Koller
N. Benczer-Koller
JHJ. Holden
J. Holden
GJG. Jakob
G. Jakob
GKG. Kumbartzki
G. Kumbartzki
WKW. Korten
W. Korten
The g factors of the 21+ and 41+ states in 78,80,82,84,86Kr have been measured for the first time, using Coulomb excitation of isotopic Kr beams and the transient field technique. The measured g factors of 21+ states in 78,80,82Kr are well described, in both magnitude and progression with neutron number, by the IBA-II model. Whereas the lighter isotopes show a dominant collective structure with g factor values close to Z/A, the large g(21+)=1.12(14) value of 86Kr, with its closed N=50 shell, is unequivocally dominated by specific proton configurations. The g factor of the 21+ state in 84Kr, with two holes in the 1g9/2 neutron orbit, reflects both proton and neutron components in the wave function. In addition, the lifetimes of several 21+ and 41+ states were remeasured by the Doppler shift attenuation method, yielding values which, in some cases, differ from those in the literature.

30 August 2023 in Atoms
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Dennis BonatsosDennis Bonatsos
Dennis Bonatsos
AMAndriana Martinou
Andriana Martinou
SPSpyridon K. Peroulis
Spyridon K. Peroulis
Theo J. MertzimekisTheo J. Mertzimekis
Theo J. Mertzimekis
NMNikolay Minkov
Nikolay Minkov
The last decade has seen a rapid growth in our understanding of the microscopic origins of shape coexistence, assisted by the new data provided by the modern radioactive ion beam facilities built worldwide. Islands of the nuclear chart in which shape coexistence can occur have been identified, and the different microscopic particle–hole excitation mechanisms leading to neutron-induced or proton-induced shape coexistence have been clarified. The relation of shape coexistence to the islands of inversion, appearing in light nuclei, to the new spin-aligned phase appearing in N=Z nuclei, as well as to shape/phase transitions occurring in medium mass and heavy nuclei, has been understood. In the present review, these developments are considered within the shell-model and mean-field approaches, as well as by symmetry methods. In addition, based on systematics of data, as well as on symmetry considerations, quantitative rules are developed, predicting regions in which shape coexistence can appear, as a possible guide for further experimental efforts that can help in improving our understanding of the details of the nucleon–nucleon interaction, as well as of its modifications occurring far from stability.

1 February 2006 in Physics Letters B
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Journal Article
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APA. Pakou
A. Pakou
NAN. Alamanos
N. Alamanos
NCN.M. Clarke
N.M. Clarke
NDN.J. Davis
N.J. Davis
GDG. Doukelis
G. Doukelis
CZCh. Zarkadas
Ch. Zarkadas