Beuermann, Klaus Peter

[["dc.bibliographiccitation.firstpage","671"],["dc.bibliographiccitation.issue","2"],["dc.bibliographiccitation.journal","Astronomy and Astrophysics"],["dc.bibliographiccitation.lastpage","681"],["dc.bibliographiccitation.volume","451"],["dc.contributor.author","Euchner, F."],["dc.contributor.author","Jordan, S."],["dc.contributor.author","Beuermann, Klaus"],["dc.contributor.author","Reinsch, K."],["dc.contributor.author","Gansicke, B. T."],["dc.date.accessioned","2018-11-07T09:50:53Z"],["dc.date.available","2018-11-07T09:50:53Z"],["dc.date.issued","2006"],["dc.description.abstract","Aims. We analyse the magnetic field geometry of the magnetic DA white dwarf PG1015+014 with our Zeeman tomography method. Methods. This study is based on rotation-phase resolved optical flux and circular polarization spectra of PG1015+014 obtained with FORS1 at the ESO VLT. Our tomographic code makes use of an extensive database of pre-computed Zeeman spectra. The general approach has been described in Papers I and II of this series. Results. The surface field strength distributions for all rotational phases of PG1015+014 are characterised by a strong peak at 70 MG. A separate peak at 80MG is seen for about one third of the rotation cycle. Significant contributions to the Zeeman features arise from regions with field strengths between 50 and 90 MG. We obtain equally good simultaneous fits to the observations, collected in five phase bins, for two different field parametrizations: (i) a superposition of individually tilted and off-centred zonal multipole components; and (ii) a truncated multipole expansion up to degree l = 4 including all zonal and tesseral components. The magnetic fields generated by both parametrizations exhibit a similar global structure of the absolute surface field values, but differ considerably in the topology of the field lines. An effective photospheric temperature of T-eff = 10 000 +/- 1000 K was found. Conclusions. Remaining discrepancies between the observations and our best-fit models suggest that additional small-scale structure of the magnetic field exists which our field models are unable to cover due to the restricted number of free parameters."],["dc.identifier.doi","10.1051/0004-6361:20064840"],["dc.identifier.fs","45028"],["dc.identifier.isi","237272100027"],["dc.identifier.purl","https://resolver.sub.uni-goettingen.de/purl?gs-1/9385"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/35801"],["dc.notes.intern","Merged from goescholar"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","Edp Sciences S A"],["dc.relation.issn","1432-0746"],["dc.relation.orgunit","Fakultät für Physik"],["dc.title","Zeeman tomography of magnetic white dwarfs - III. The 70-80 Megagauss magnetic field of PG1015+014"],["dc.title.original","9385"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dc.type.version","published_version"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","229"],["dc.bibliographiccitation.lastpage","239"],["dc.bibliographiccitation.seriesnr","206"],["dc.contributor.author","Beuermann, S."],["dc.contributor.author","Buback, M."],["dc.contributor.author","Gadermann, M."],["dc.contributor.author","Juergens, M."],["dc.contributor.author","Gunzler, F."],["dc.date.accessioned","2018-11-07T10:52:55Z"],["dc.date.available","2018-11-07T10:52:55Z"],["dc.date.issued","2004"],["dc.description.abstract","Free-radical terpolymerizations of styrene, methyl methacrylate, and glycidyl methacrylate were carried out in a tubular reactor in the presence of 20 wt.% CO2 at temperatures between 120 and 180degreesC and pressures of 300 and 350 bar. The number average molecular weights, M-N, were mostly between 2000 and 3000 g(.)mol(-1) and polydispersity indices around 2. In part of the experiments molecular weights were controlled by n-dodecyl mercaptan serving as the chain-transfer agent. PREDICI modeling indicates that the targeted molecular weights of M(N)similar to2500 g(.)mol(-1) and polydispersities around 2 may also be reached by using an initiator cocktail, a mixture of two initiators with significantly different decomposition rate coefficients. The predictions are confirmed experimentally."],["dc.identifier.doi","10.1002/masy.200450218"],["dc.identifier.isi","000220207400019"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/49224"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","Wiley-VCH"],["dc.publisher.place","Weinheim"],["dc.relation.conference","5th Conference on Polymer Reaction Engineering"],["dc.relation.crisseries","Macromolecular Symposia"],["dc.relation.eventend","2003-05-23"],["dc.relation.eventlocation","Quebec City, Canada"],["dc.relation.eventstart","2003-05-18"],["dc.relation.isbn","3-527-31039-8"],["dc.relation.ispartof","Polymer reaction engineering V"],["dc.relation.ispartofseries","Macromolecular symposia; 206"],["dc.title","Continuous styrene - methyl methacrylate - Glycidyl methacrylate terpolymerizations in homogeneous mixtures with supercritical carbon dioxide"],["dc.type","conference_paper"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","143"],["dc.bibliographiccitation.issue","1-2"],["dc.bibliographiccitation.journal","New Astronomy Reviews"],["dc.bibliographiccitation.lastpage","148"],["dc.bibliographiccitation.volume","44"],["dc.contributor.author","Gansicke, B. T."],["dc.contributor.author","van Teeseling, A."],["dc.contributor.author","Beuermann, Klaus"],["dc.contributor.author","Reinsch, K."],["dc.date.accessioned","2018-11-07T11:25:18Z"],["dc.date.available","2018-11-07T11:25:18Z"],["dc.date.issued","2000"],["dc.description.abstract","Recent observational results on supersoft X-ray binaries are reviewed, with emphasis on the galactic source QR And and on the enigmatic LMC source RX J0439.8-6809. (C) 2000 Elsevier Science B.V. All rights reserved."],["dc.identifier.doi","10.1016/S1387-6473(00)00028-2"],["dc.identifier.isi","000090017800026"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/56592"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","Elsevier Sci Ltd"],["dc.publisher.place","Oxford"],["dc.relation.conference","Cataclysmic Variables: a 60th Birthday Symposium in Honour of Brian Warner"],["dc.relation.eventlocation","OXFORD UNIV, OXFORD, ENGLAND"],["dc.relation.issn","1387-6473"],["dc.title","Supersoft X-ray binaries: an observational update"],["dc.type","conference_paper"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","31"],["dc.bibliographiccitation.lastpage","42"],["dc.bibliographiccitation.seriesnr","182"],["dc.contributor.author","Beuermann, S."],["dc.date.accessioned","2018-11-07T10:29:14Z"],["dc.date.available","2018-11-07T10:29:14Z"],["dc.date.issued","2002"],["dc.description.abstract","The combination of pulsed laser initiated polymerizations (PLP) with analysis of the generated polymer by size-exclusion chromatography (SEC) yields reliable individual rate coefficients for polymerizations of a large number of monomers in bulk and in solution. PLP-SEC experiments carried out in the presence of scCO(2) as a solvent show no unambiguous trend: while a significant reduction of k(p) is seen for some monomers, e.g. acrylates, k(p) for monomers such as vinyl acetate and styrene is not affected. It is suggested that the influence of CO2 on acrylate k(p) is not a true kinetic effect and that the experimental findings may be understood in terms of the occurrence of local monomer concentrations in the vicinity of the propagating radical. It is discussed that such local monomer concentrations may also contribute to a better understanding of why k(p) increases with ester size within the acrylate or within the methacrylate family, and why k(p) frequently is influenced by the initiating laser pulse repetition rate."],["dc.identifier.doi","10.1002/1521-3900(200206)182:1<31::AID-MASY31>3.0.CO;2-7"],["dc.identifier.isi","000176800700004"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/43595"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","Wiley-VCH"],["dc.publisher.place","Weinheim"],["dc.relation.conference","3rd International Symposium on Free-Radical Polymerization: Kinetics and Mechanism II Ciocco"],["dc.relation.crisseries","Macromolecular Symposia"],["dc.relation.eventend","2001-06-09"],["dc.relation.eventlocation","Lucca, Italy"],["dc.relation.eventstart","2001-06-03"],["dc.relation.isbn","3-527-30472-X"],["dc.relation.ispartof","Plenary and invited lectures presented at the 3rd IUPAC-sponsored International Symposium on Free-Radical Polymerization: Kinetics and Mechanism"],["dc.relation.ispartofseries","Macromolecular symposia; 182"],["dc.title","Propagation kinetics in free-radical polymerizations"],["dc.type","conference_paper"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","L141"],["dc.bibliographiccitation.issue","2"],["dc.bibliographiccitation.journal","The Astrophysical Journal Letters"],["dc.bibliographiccitation.lastpage","L144"],["dc.bibliographiccitation.volume","613"],["dc.contributor.author","Gansicke, B. T."],["dc.contributor.author","Jordan, S."],["dc.contributor.author","Beuermann, Klaus"],["dc.contributor.author","de Martino, Domitilla"],["dc.contributor.author","Szkody, P."],["dc.contributor.author","Marsh, T. R."],["dc.contributor.author","Thorstensen, J."],["dc.date.accessioned","2018-11-07T10:44:59Z"],["dc.date.available","2018-11-07T10:44:59Z"],["dc.date.issued","2004"],["dc.description.abstract","We report the detection of Zeeman-split Lyalpha absorption pi and sigma(+) lines in the far-ultraviolet Hubble Space Telescope/Space Telescope Imaging Spectrograph (STIS) spectrum of the magnetic cataclysmic variable RX J1554.2 + 2721. Fitting the STIS data with magnetic white dwarf model spectra, we derive a field strength of B similar or equal to 144 MG and an effective temperature of 17,000 K less than or similar to T-eff less than or similar to 23,000 K. This measurement makes RX J1554.2 + 2721 only the third cataclysmic variable containing a white dwarf with a field exceeding 100 MG. Similar to the other high-field polar AR UMa, RX J1554.2 + 2721 is often found in a state of feeble mass transfer, which suggests that a considerable number of high-field polars may still remain undiscovered."],["dc.identifier.doi","10.1086/425141"],["dc.identifier.isi","000224303300015"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/47397"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","Iop Publishing Ltd"],["dc.relation.issn","1538-4357"],["dc.relation.issn","0004-637X"],["dc.title","A 150 MG magnetic white dwarf in the cataclysmic variable RX J1554.2+2721"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","93"],["dc.bibliographiccitation.issue","1-2"],["dc.bibliographiccitation.journal","New Astronomy Reviews"],["dc.bibliographiccitation.lastpage","98"],["dc.bibliographiccitation.volume","44"],["dc.contributor.author","Beuermann, Klaus"],["dc.date.accessioned","2018-11-07T11:24:46Z"],["dc.date.available","2018-11-07T11:24:46Z"],["dc.date.issued","2000"],["dc.description.abstract","Recent theoretical and observational progress has substantially improved the definition of the lower main sequence and established a new basis fur a comparison of main sequence stars and the secondaries in CVs. The evolutionary sequences of Kolb & Baraffe (1999) imply that the secondaries in many CVs are expanded compared with main sequence stars of the same mass as a consequence of unusually high mass transfer rates and/or pre-CV nuclear evolution. We show that the location of the secondaries of all well-studied CVs in the spectral type period diagram implies that they are consistent with having near-solar metallicities. We show, furthermore, that the surface brightness of K/M stars depends on gravity and metallicity and present new Barnes-Evans relations valid fur dwarfs of near-solar metallicity and the secondaries in CVs of the galactic disk population. Distances derived by the surface brightness method agree with recent measurements of the trigonometric parallaxes of a few selected systems. (C) 2000 Elsevier Science B.V. All rights reserved."],["dc.identifier.doi","10.1016/S1387-6473(00)00020-8"],["dc.identifier.isi","000090017800018"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/56481"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","Elsevier Sci Ltd"],["dc.publisher.place","Oxford"],["dc.relation.conference","Cataclysmic Variables: a 60th Birthday Symposium in Honour of Brian Warner"],["dc.relation.eventlocation","OXFORD UNIV, OXFORD, ENGLAND"],["dc.relation.issn","1387-6473"],["dc.title","Secondary stars in CVs - the observational picture"],["dc.type","conference_paper"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","930"],["dc.bibliographiccitation.issue","2"],["dc.bibliographiccitation.journal","Monthly Notices of the Royal Astronomical Society"],["dc.bibliographiccitation.lastpage","949"],["dc.bibliographiccitation.volume","425"],["dc.contributor.author","Gozdziewski, Krzysztof"],["dc.contributor.author","Nasiroglu, Ilham"],["dc.contributor.author","Slowikowska, Aga"],["dc.contributor.author","Beuermann, Klaus"],["dc.contributor.author","Kanbach, Gottfried"],["dc.contributor.author","Gauza, Bartosz"],["dc.contributor.author","Maciejewski, Andrzej J."],["dc.contributor.author","Schwarz, Robert"],["dc.contributor.author","Schwope, Axel D."],["dc.contributor.author","Hinse, Tobias C."],["dc.contributor.author","Haghighipour, Nader"],["dc.contributor.author","Burwitz, Vadim"],["dc.contributor.author","Slonina, Mariusz"],["dc.contributor.author","Rau, Arne"],["dc.date.accessioned","2018-11-07T09:06:41Z"],["dc.date.available","2018-11-07T09:06:41Z"],["dc.date.issued","2012"],["dc.description.abstract","In this paper, we investigate the eclipse timing of the polar binary HU?Aquarii that has been observed for almost two decades. Recently, Qian et al. attributed large (OC) deviations between the eclipse ephemeris and observations to a compact system of two massive Jovian companions. We improve the Keplerian, kinematic model of the light travel time effect and re-analyse the whole currently available data set. We add almost 60 new, yet unpublished, mostly precision light curves obtained using the time high-resolution photopolarimeter Optical Timing Analyzer (OPTIMA), as well as photometric observations performed at the Monitoring Network of Telescopes/North, Physics Innovations Robotic Astronomical Telescope Explorer and Carlos Sanchez Telescope. We determine new mid-egress times with a mean uncertainty at the level of 1?s or better. We claim that because the observations that currently exist in the literature are non-homogeneous with respect to spectral windows (ultraviolet, X-ray, visual and polarimetric mode) and the reported mid-egress measurements errors, they may introduce systematics that affect orbital fits. Indeed, we find that the published data, when taken literally, cannot be explained by any unique solution. Many qualitatively different and best-fit two-planet configurations, including self-consistent, Newtonian N-body solutions may be able to explain the data. However, using high-resolution, precision OPTIMA light curves, we find that the (OC) deviations are best explained by the presence of a single circumbinary companion orbiting at a distance of similar to 4.5?au with a small eccentricity and having similar to 7 Jupiter masses. This object could be the next circumbinary planet detected from the ground, similar to the announced companions around close binaries HW?Vir, NN?Ser, UZ?For, DP?Leo, FS?Aur or SZ?Her, and planets of this type around Kepler-16, Kepler-34 and Kepler-35."],["dc.identifier.doi","10.1111/j.1365-2966.2012.21341.x"],["dc.identifier.isi","000307888300008"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/25611"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","Wiley-blackwell"],["dc.relation.issn","0035-8711"],["dc.title","On the HU Aquarii planetary system hypothesis"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","2151"],["dc.bibliographiccitation.issue","16"],["dc.bibliographiccitation.journal","Macromolecular Chemistry and Physics"],["dc.bibliographiccitation.lastpage","2160"],["dc.bibliographiccitation.volume","205"],["dc.contributor.author","Asua, J. M."],["dc.contributor.author","Beuermann, S."],["dc.contributor.author","Buback, M."],["dc.contributor.author","Castignolles, P."],["dc.contributor.author","Charleux, B."],["dc.contributor.author","Giess, Rene MarkusGilbert, Robert G."],["dc.contributor.author","Hutchinson, Robin A."],["dc.contributor.author","Leiza, J. R."],["dc.contributor.author","Nikitin, A. N."],["dc.contributor.author","Vairon, J. P."],["dc.contributor.author","van Herk, A. M."],["dc.date.accessioned","2018-11-07T10:43:59Z"],["dc.date.available","2018-11-07T10:43:59Z"],["dc.date.issued","2004"],["dc.description.abstract","Propagation rate coefficients, k(P), for free-radical polymerization of butyl acrylate (BA) previously reported by several groups are critically evaluated. All data were determined by the combination of pulsed-laser polymerization (PLP) and subsequent polymer analysis by size exclusion (SEC) chromatography. The PLP-SEC technique has been recommended as the method of choice for the determination of k(P) by the IUPAC Working Party on Modeling of Polymerization Kinetics and Processes. Application of the technique to acrylates has proven to be very difficult and, along with other experimental evidence, has led to the conclusion that acrylate chain-growth kinetics are complicated by intramolecular transfer (backbiting) events to form a mid-chain radical structure of lower reactivity. These mechanisms have a significant effect on acrylate polymerization rate even at low temperatures, and have limited the PLP-SEC determination of k(P) of chain-end radicals to low temperatures (<20 degreesC) using high pulse repetition rates. Nonetheless, the values for BA from six different laboratories, determined at ambient pressure in the temperature range of -65 to 20 degreesC mostly for bulk monomer with few data in solution, fulfill consistency criteria and show excellent agreement, and are therefore combined together into a benchmark data set. The data are fitted well by an Arrhenius relation resulting in a pre-exponential factor of 2.21 x 10(7) L (.) mol(-1) (.) s(-1) and an activation energy of 17.9 kJ (.) mol(-1). It must be emphasized that these PLP-determined k(P) values are for monomer addition to a chain-end radical and that, even at low temperatures, it is necessary to consider the presence of two radical structures that have very different reactivity. Studies for other alkyl acrylates do not provide sufficient results to construct benchmark data sets, but indicate that the family behavior previously documented for alkyl methacrylates also holds true within the alkyl acrylate family of monomers. [GRAPHICS] Arrhenius plot of propagation rate coefficients, k(P), for BA as measured by PLP-SEC."],["dc.identifier.doi","10.1002/macp.200400355"],["dc.identifier.isi","000225139500002"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/47174"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","Wiley-v C H Verlag Gmbh"],["dc.relation.issn","1022-1352"],["dc.title","Critically evaluated rate coefficients for free-radical polymerization, 5 - Propagation rate coefficient for butyl acrylate"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.artnumber","002"],["dc.bibliographiccitation.journal","e-Polymers"],["dc.contributor.author","Beuermann, S."],["dc.contributor.author","Buback, M."],["dc.contributor.author","Drache, M."],["dc.contributor.author","Nelke, D."],["dc.contributor.author","Schmidt-Naake, G."],["dc.date.accessioned","2018-11-07T10:51:49Z"],["dc.date.available","2018-11-07T10:51:49Z"],["dc.date.issued","2004"],["dc.description.abstract","The differences in solubility of poly(vinyl acetate) (PVAc) and poly(methyl acrylate) (PMA) were addressed by applying atomistic Monte Carlo simulation techniques. Polymer segments consisting of nine monomer units serve as model compounds for polymer chains. As a measure of intermolecular interactions with the solvent environment, cohesion energies of the polymer segments embedded in either the corresponding monomer or in CO2 were calculated. Only in case of PMA segments in CO2 environment, specific interactions between polymer segments were identified. This finding is in agreement with experimental results on phase behaviour and propagation kinetics."],["dc.identifier.isi","000188374000001"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/48970"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","European Polymer Federation"],["dc.relation.issn","1618-7229"],["dc.title","Solvation of poly(methyl acrylate) and poly(vinyl acetate) by CO2 studied via atomistic Monte Carlo simulation techniques"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","184"],["dc.bibliographiccitation.issue","1"],["dc.bibliographiccitation.journal","Macromolecules"],["dc.bibliographiccitation.lastpage","193"],["dc.bibliographiccitation.volume","39"],["dc.contributor.author","Beuermann, S."],["dc.contributor.author","Buback, M."],["dc.contributor.author","Hesse, P."],["dc.contributor.author","Lacik, Igor"],["dc.date.accessioned","2018-11-07T10:26:49Z"],["dc.date.available","2018-11-07T10:26:49Z"],["dc.date.issued","2006"],["dc.description.abstract","The propagation rate coefficient, k(p), for free-radical polymerization of nonionized methacrylic acid (MAA) in aqueous solution has been studied via pulsed laser polymerization (PLP) in conjunction with aqueous-phase size-exclusion chromatography (SEC). The PLP-SEC experiments were carried out between 20 and 80 degrees C within the entire concentration range from dilute solution containing 1 wt % MAA up to bulk MAA polymerization. The k(p) values which are determined under the assumption that the relevant monomer concentration at the radical site is identical to the known overall MAA concentration decrease by about 1 order of magnitude between 1 and 100 wt % MAA. This significant lowering is almost entirely due to a reduction in the Arrhenius preexponential factor, A(k(p)), whereas the activation energy, E-A(k(p)), stays essentially constant. The decrease in A(k(p)) is assigned to intermolecular interactions between the transition state (TS) structure for MAA propagation and an MAA environment being significantly stronger than the ones between this TS structure and an H2O environment. In an MAA-rich environment, the barrier to rotational motion of the relevant degrees of motion of the TS thus experiences enhanced friction, which is associated with a lowering of the preexponential factor and thus of k(p),"],["dc.identifier.doi","10.1021/ma051954i"],["dc.identifier.isi","000234500100030"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/43124"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","Amer Chemical Soc"],["dc.relation.issn","0024-9297"],["dc.title","Free-radical propagation rate coefficient of nonionized methacrylic acid in aqueous solution from low monomer concentrations to bulk polymerization"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dspace.entity.type","Publication"]]