scholarly journals PDG57 THE IMPACT OF GENERIC MARKET EXCLUSIVITY BY THE PATENT-REGISTRATION LINKAGE SYSTEM IN KOREA

2019 ◽  
Vol 22 ◽  
pp. S172
Author(s):  
H. Woo ◽  
S. Bae
2021 ◽  
Vol 10 (1) ◽  
pp. 78-97
Author(s):  
Kristie Briggs

PurposeThis paper examines the relationship between the originality of a pharmaceutical innovation and its patent quality. Greater patent quality has been shown in the extant literature to enhance market value, which better enables firms to recoup research and development (R&D) expenditures incurred during the innovation process. Understanding how originality improves patent quality can assist policymakers, when determining the optimal length of pharmaceutical patent protection and/or market exclusivity.Design/methodology/approachThe relationship between originality and patent quality is empirically investigated using a tobit, as well as a zero-inflated negative binomial, estimation approach to account for prevalence of patents receiving zero forward citations. Moderating effects of joint innovation, innovation by a university researcher and innovation by an established innovator on originality are also considered.FindingsThere is a robust and positive relationship between patent originality and quality in the pharmaceutical sector. This relationship is positively moderated by joint patent ownership with a university. As such, innovators that target originality in new drug development (especially those collaborating with universities) should, according to extant literature, see greater increases in their market value.Originality/valuePolicymakers can use information on the originality of a new drug to discern the optimal length of market exclusivity needed to enable the innovator to recoup expenditures related to R&D. Better predictions of the timing for which firms can recoup R&D expenditures will equip policymakers with knowledge about the appropriate timing to introduce competition into the market, which is critical to reducing the price of pharmaceuticals to consumers.


Author(s):  
Steven Simoens

This paper aims to report on the ‘Innovation through generics’ roundtable, which was convened at the European Parliament in April 2008 to discuss the role of generic medicines in stimulating innovation in the pharmaceutical sector. The roundtable identified a number of factors that hamper generic market entry in Europe and, thus, inhibit competition and innovation in the pharmaceutical sector. These factors include the decline in true innovation in the pharmaceutical sector; shortcomings in current patent and registration systems; pricing and reimbursement delays for generic medicines; greater intellectual property protection and market exclusivity for originator medicines than in the United States; price linkage between generic and originator medicines in some member states; and a lack of demand-side measures that encourage physicians, pharmacists and patients to use generic medicines. There is a need for a pan-European policy relating to patents, registration, pricing and reimbursement, prescribing and dispensing of medicines. In particular, the creation of an internal market will benefit European healthcare by helping to drive down costs. The overall goal should be to support competition and true innovation and, thus, provide sustainable healthcare for patients throughout Europe.


2018 ◽  
Vol 37 (5) ◽  
pp. 732-737 ◽  
Author(s):  
Ameet Sarpatwari ◽  
Reed F. Beall ◽  
Abdurrahman Abdurrob ◽  
Mengdong He ◽  
Aaron S. Kesselheim

1962 ◽  
Vol 14 ◽  
pp. 415-418
Author(s):  
K. P. Stanyukovich ◽  
V. A. Bronshten

The phenomena accompanying the impact of large meteorites on the surface of the Moon or of the Earth can be examined on the basis of the theory of explosive phenomena if we assume that, instead of an exploding meteorite moving inside the rock, we have an explosive charge (equivalent in energy), situated at a certain distance under the surface.


1962 ◽  
Vol 14 ◽  
pp. 169-257 ◽  
Author(s):  
J. Green

The term geo-sciences has been used here to include the disciplines geology, geophysics and geochemistry. However, in order to apply geophysics and geochemistry effectively one must begin with a geological model. Therefore, the science of geology should be used as the basis for lunar exploration. From an astronomical point of view, a lunar terrain heavily impacted with meteors appears the more reasonable; although from a geological standpoint, volcanism seems the more probable mechanism. A surface liberally marked with volcanic features has been advocated by such geologists as Bülow, Dana, Suess, von Wolff, Shaler, Spurr, and Kuno. In this paper, both the impact and volcanic hypotheses are considered in the application of the geo-sciences to manned lunar exploration. However, more emphasis is placed on the volcanic, or more correctly the defluidization, hypothesis to account for lunar surface features.


1997 ◽  
Vol 161 ◽  
pp. 197-201 ◽  
Author(s):  
Duncan Steel

AbstractWhilst lithopanspermia depends upon massive impacts occurring at a speed above some limit, the intact delivery of organic chemicals or other volatiles to a planet requires the impact speed to be below some other limit such that a significant fraction of that material escapes destruction. Thus the two opposite ends of the impact speed distributions are the regions of interest in the bioastronomical context, whereas much modelling work on impacts delivers, or makes use of, only the mean speed. Here the probability distributions of impact speeds upon Mars are calculated for (i) the orbital distribution of known asteroids; and (ii) the expected distribution of near-parabolic cometary orbits. It is found that cometary impacts are far more likely to eject rocks from Mars (over 99 percent of the cometary impacts are at speeds above 20 km/sec, but at most 5 percent of the asteroidal impacts); paradoxically, the objects impacting at speeds low enough to make organic/volatile survival possible (the asteroids) are those which are depleted in such species.


1997 ◽  
Vol 161 ◽  
pp. 189-195
Author(s):  
Cesare Guaita ◽  
Roberto Crippa ◽  
Federico Manzini

AbstractA large amount of CO has been detected above many SL9/Jupiter impacts. This gas was never detected before the collision. So, in our opinion, CO was released from a parent compound during the collision. We identify this compound as POM (polyoxymethylene), a formaldehyde (HCHO) polymer that, when suddenly heated, reformes monomeric HCHO. At temperatures higher than 1200°K HCHO cannot exist in molecular form and the most probable result of its decomposition is the formation of CO. At lower temperatures, HCHO can react with NH3 and/or HCN to form high UV-absorbing polymeric material. In our opinion, this kind of material has also to be taken in to account to explain the complex evolution of some SL9 impacts that we observed in CCD images taken with a blue filter.


1997 ◽  
Vol 161 ◽  
pp. 179-187
Author(s):  
Clifford N. Matthews ◽  
Rose A. Pesce-Rodriguez ◽  
Shirley A. Liebman

AbstractHydrogen cyanide polymers – heterogeneous solids ranging in color from yellow to orange to brown to black – may be among the organic macromolecules most readily formed within the Solar System. The non-volatile black crust of comet Halley, for example, as well as the extensive orangebrown streaks in the atmosphere of Jupiter, might consist largely of such polymers synthesized from HCN formed by photolysis of methane and ammonia, the color observed depending on the concentration of HCN involved. Laboratory studies of these ubiquitous compounds point to the presence of polyamidine structures synthesized directly from hydrogen cyanide. These would be converted by water to polypeptides which can be further hydrolyzed to α-amino acids. Black polymers and multimers with conjugated ladder structures derived from HCN could also be formed and might well be the source of the many nitrogen heterocycles, adenine included, observed after pyrolysis. The dark brown color arising from the impacts of comet P/Shoemaker-Levy 9 on Jupiter might therefore be mainly caused by the presence of HCN polymers, whether originally present, deposited by the impactor or synthesized directly from HCN. Spectroscopic detection of these predicted macromolecules and their hydrolytic and pyrolytic by-products would strengthen significantly the hypothesis that cyanide polymerization is a preferred pathway for prebiotic and extraterrestrial chemistry.


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