Nanostrukturalno oblikovanje jakom plastičnom deformacijom

The influence of severe plastic deformations on structural, mechanical and plastic properties of ARMCO-Fe in equal-channel angular pressing procedure was investigated. Mathematical simulations of stress and temperature fields were applied, too.Istraživao se utjecaj snažnih plastičnih deformacija na strukturalna, mehanička i plastična svojstva ARMCO-željeza u postupku prešanja s istiskivanjem kroz jednake kanale (ECAP) postavljene pod nekim kutom. Primjenjivale su se također i matematičke simulacije područja naprezanja i temperaturnih područja

Limovi za karoserije auta nove generacije

This paper deals with the development of hot - and cold - rolled sheets designed for automotive industry. The achieved properties of some grade sheets after simulation of technological processes in the laboratory conditions are compared to the common properties of individual sheet groups. The attention is paid to the processes of hot rolling with the accent to the ferittic rolling.Rad se bavi razvojem toplo i hladno valjanih limova, namijenjenih industriji auta. Dobivena svojstva nekih kvalitetnih čelika nakon simulacije tehničkih procesa u laboratorijskim uvjetima uspoređuju se s zajedničkim svojstvima pojedinih grupa limova. Govori se također o procesima toplog valjanja s naglaskom na feritno valjanje

Enrichment of the HR 8799 planets by minor bodies and dust

Context. In the Solar System, minor bodies and dust deliver various materials to planetary surfaces. Several exoplanetary systems are known to host inner and outer belts, analogues of the main asteroid belt and the Kuiper belt, respectively. Aims: We study the possibility that exominor bodies and exodust deliver volatiles and refractories to the exoplanets in the well-characterised system HR 8799. Methods: We performed N-body simulations to study the impact rates of minor bodies in the system HR 8799. The model consists of the host star, four giant planets (HR 8799 e, d, c, and b), 650 000 test particles representing the inner belt, and 1 450 000 test particles representing the outer belt. Moreover we modelled dust populations that originate from both belts. Results: Within a million years, the two belts evolve towards the expected dynamical structure (also derived in other works), where mean-motion resonances with the planets carve the analogues of Kirkwood gaps. We find that, after this point, the planets suffer impacts by objects from the inner and outer belt at rates that are essentially constant with time, while dust populations do not contribute significantly to the delivery process. We convert the impact rates to volatile and refractory delivery rates using our best estimates of the total mass contained in the belts and their volatile and refractory content. Over their lifetime, the four giant planets receive between 10-4 and 10-3 M⊕ of material from both belts. Conclusions: The total amount of delivered volatiles and refractories, 5 × 10-3 M⊕, is small compared to the total mass of the planets, 11 × 103 M⊕. However, if the planets were formed to be volatile-rich, their exogenous enrichment in refractory material may well be significant and observable, for example with JWST-MIRI. If terrestrial planets exist within the snow line of the system, volatile delivery would be an important astrobiological mechanism and may be observable as atmospheric trace gases

Enrichment of the HR 8799 planets by minor bodies and dust

In the Solar System, minor bodies and dust deliver various materials to planetary surfaces. Several exoplanetary systems are known to host inner and outer belts, analogues of the main asteroid belt and the Kuiper belt. We study the possibility that exominor bodies and exodust deliver volatiles and refractories to the exoplanets in the system HR8799 by performing N-body simulations. The model consists of the host star, four giant planets (HR8799 e, d, c, and b), 650000 test particles representing the inner belt, and 1450000 test particles representing the outer belt. Moreover we modelled dust populations that originate from both belts. Within a million years, the two belts evolve towards the expected dynamical structure (also derived in other works), where mean-motion resonances with the planets carve the analogues of Kirkwood gaps. We find that, after this point, the planets suffer impacts by objects from the inner and outer belt at rates that are essentially constant with time, while dust populations do not contribute significantly to the delivery process. We convert the impact rates to volatile and refractory delivery rates using our best estimates of the total mass contained in the belts and their volatile and refractory content. Over their lifetime, the four giant planets receive between $10^{-4}$ and 10^{-3}M_\bigoplus of material from both belts. The total amount of delivered volatiles and refractories, {5\times10^{-3}\textrm{M}_\bigoplus}, is small compared to the total mass of the planets, 11\times10^{3}\textrm{M}_\bigoplus. However, if the planets were formed to be volatile-rich, their exogenous enrichment in refractory material may well be significant and observable, for example with JWST-MIRI. If terrestrial planets exist within the snow line of the system, volatile delivery would be an important astrobiological mechanism and may be observable as atmospheric trace gases.Comment: 11 pages, 8 figures, accepted for publication in Astronomy&Astrophysic

Global regularity criterion for the 3D Navier-Stokes equations involving one entry of the velocity gradient tensor

In this paper we provide a sufficient condition, in terms of only one of the nine entries of the gradient tensor, i.e., the Jacobian matrix of the velocity vector field, for the global regularity of strong solutions to the three-dimensional Navier-Stokes equations in the whole space, as well as for the case of periodic boundary conditions

LiBC by polarized Raman spectroscopy: Evidence for lower crystal symmetry ?

The paper presents polarized Raman scattering study on a few-micron-size crystallite of LiBC with natural faces. The experiment on as grown sample has revealed a four lattice modes with frequencies at 1276 cm^-1, 830 cm^-1, 546 cm^-1 and 170 cm^-1, respectively. The number of observed Raman lines and their selection rules are incompatible with the assumed D6h symmetry. The modes at 1276 cm^-1 and 170 cm^-1 correspond to the expected Raman active modes. In contrast with the superconducting compound MgB2, the B-C bond stretching mode (at 1276 cm^-1) has rather small damping. The two "forbidden" modes (at 830 cm^-1 and 546 cm^-1) disappeared after subsequent thermal treatment.Comment: 4 pages, LaTeX, complementary experimental resul

Utjecaj uvjeta zagrijavanja i hlađenja na strukturu i mehanička svojstva C-Mn-Si čelika

The paper deals with structure and properties development of AHSS (advance high-strength steel) and UHSS (ultra high-strength steel) steel grades for various groups of automotive parts. C-Mn-Si type steel properties are evaluated based on the results of laboratory controlled rolling and cooling. The important influence on mechanical and plastic properties, amount of residual austenite (RA) and final structural type has, except for cooling rate, also starting temperature of intensive cooling (TIC) which follows after hot plastic deformations. If TIC is from interval of 620-760°C the final structure predominantly consists of ferrite with RA. Mostly acicular ferrite with RA, as well as bainite with RA was obtained when TIC was kept in the range of 760-850°C.Utjecaj uvjeta zagrijavanja i hlađenja na strukturu i mehanička svojstva C-Mn-Si čelika. Članak daje razvitak strukture i svojstava NVČČ (napredno visoko čvrstih čelika) i UVČČ (ultra visoko čvrsti čelici) za raznolike skupine dijelova automobila. Svojstva čelika C-Mn-Si su utvrđena na temelju laboratorijskog kontroliranog valjanja i hlađenja. Najveći utjecaj na mehanička i plastična svojstva uz zaostali austenit (ZA) i završni tip strukture, ima osim brzine hlađenja i početna temperatura intenzivnog hlađenja (Tpo) koja je nastavak vruće plastične deformacije. Ako je Tpo u intervalu 620-760°C, završna struktura se sastoji od ferita sa ZA. Pretežito acikularni ferit sa ZA, također bainit sa ZA je uočen kad je Tpo bila u intervalu 760-850°C

Ne-termalni biopokazatelji izloženosti radiofrekvencijskom/mikrovalnom zračenju

This article gives a review or several hypotheses on the biological effects of non-thermal radiofrequency/microwave (RF/MW) radiation and discusses our own findings from animal and in vitro studies performed over the last decade. We have found that RF/MW radiation disturbs cell proliferation and leads to cell differentiation in the bone marrow, which is reflected in the peripheral blood of rats. Repeated RF/MW radiation can also temporarily disrupt melatonin turnover. The observed changes seem to be a sign of adaptation to stress caused by irradiation rather than of malfunction. The article looks further into the basic mechanisms of RF/MW biological action, including cell growth parameters, colony-forming ability, viability, and the polar and apolar protein cytoskeleton structures. The observed reversible cell changes significantly obstructed cell growth. In contrast to the apolar intermediate proteins, the intracellular polar microtubule and actin fibres were damaged by radiation in a time-dependent manner. These signifi cantly altered parameters can be considered as the biomarkers of exposure. Future research should combine dosimetry, experimental studies, and epidemiological data.Svrha rada je prikaz više hipoteza o biološkom djelovanju ne-termalnih razina radiofrekventnog/mikrovalnog (RF/MW) zračenja i rasprava o rezultatima vlastitih istraživanja na životinjama i in vitro. Istraživanje djelovanja elektromagnetskih polja na organizam uključilo je proučavanje hematopoieze u štakora povremeno izloženih ne-termalnom radiofrekventnom/mikrovalnom (RF/MW) zračenju tijekom supkroničnog pokusa. Rezultati su pokazali neravnotežu u proliferaciji i diferencijaciji stanica koštane srži što se odrazilo na stanične parametre u krvi štakora. U primijenjenim uvjetima zračenja nađeno je da RF/MW može privremeno destabilizirati metabolizam melatonina bez štetnog utjecaja na zdravlje životinja. Razmatrana je mogućnost aktivacije prilagodbenog mehanizma na stres izazvan zračenjem jer smatramo da su nađene promjene prije znak adaptacije nego štetnog učinka zračenja. Pristup temeljnim mehanizmima biološkog djelovanja RF/MW zračenja uključio je istraživanje parametara staničnog rasta, sposobnosti stvaranja kolonija, vijabilnosti te polarnih i nepolarnih proteinskih struktura citoskeleta nakon ozračivanja stanica. Reverzibilne promjene staničnih svojstava koje su nađene upućuju na značajnu opstrukciju staničnog rasta. Za razliku od nepolarnih intermedijarnih proteina, unutarstanična polarna vlakna mikrotubula i aktina su, ovisno o vremenu izloženosti, pokazala značajna oštećenja uzrokovana zračenjem. Statistički značajno promijenjeni parametri smatrani su biomarkerima izloženosti. Istaknuta je potreba za budućim istraživanjima koja uključuju epidemiološke, laboratorijske i dozimetrijske studije

The Shaqadud Archaeological Project (Sudan): exploring prehistoric cultural adaptations in the Sahelian hinterlands

The authors present preliminary results from a new research project based in Jebel Shaqadud, Sudan. Their findings highlight the potential for this region's archaeological record to expand our understanding of the adaptation strategies used by human groups in arid north-east African environments away from rivers and lakes during the Holocene. Furthermore, they present exceptionally early radiocarbon dates that push postglacial human occupation in the eastern Sahel back to the twelfth millennium BP