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Davesne 100%

first results on finite nuclei Skyrme N2LO functionals:

https://www.pdf-archive.com/2017/10/11/davesne/

11/10/2017 www.pdf-archive.com

JDIT-2016-0618-021 98%

2057-3782 (Online) http://www.openmedscience.com REVIEW ARTICLE NMR-Active Nuclei for Biological and Biomedical Applications Simon G.

https://www.pdf-archive.com/2017/05/30/jdit-2016-0618-021/

30/05/2017 www.pdf-archive.com

Tews 93%

Epelbaum et al., PPNP (2006) and RMP (2009) • Systematic basis for nuclear forces, naturally includes many-body forces • Very successful in calculations of nuclei and nuclear matter Ø Local chiral interactions • Can be constructed up to N2LO Gezerlis, IT, et al., PRL &

https://www.pdf-archive.com/2017/10/11/tews/

11/10/2017 www.pdf-archive.com

PPapakon 90%

The shortest path to nuclei Panagiota Papakonstantinou Rare Isotope Science Project – IBS Daejeon, S.Korea A nuclear energy-density functional inspired by an effective field theory Panagiota Papakonstantinou Rare Isotope Science Project – IBS Daejeon, S.Korea An ab initio energy density functional (?) Panagiota Papakonstantinou Rare Isotope Science Project – IBS Daejeon, S.Korea A triangle of interests Giant and Pygmy Resonances;

https://www.pdf-archive.com/2017/10/11/ppapakon/

11/10/2017 www.pdf-archive.com

ENDOMETRIUM AND MYOMETRIUM 88%

Loose stroma, greater distance from each other with edema – increases as the secretory phase progresses Secretory activity is most prominent during the third week of the menstrual cycle, when the basal vacuoles progressively push past the nuclei By the 4th week, the secretions are discharged into the gland lumens.

https://www.pdf-archive.com/2014/03/08/endometrium-and-myometrium/

08/03/2014 www.pdf-archive.com

Theory of Everything 82%

pair or grouping of particles, or Astros as galaxies, etc.) are created and reside in the orbits (inside the peripheral magnetic fields) of the atoms and stars, but not in their nuclei (*).

https://www.pdf-archive.com/2016/10/14/theory-of-everything/

14/10/2016 www.pdf-archive.com

J.M. Lattimer and M. Prakash. The Physics of Neutron Stars 79%

Z∞ dÑ ≡ intergalactic neutron star on shrooms HIM = −∞ Introduction The term neutron star as generally used today refers to a star with a mass M on the order of 1.5 solar masses (M ), a radius R of ∼ 12 km, and a central density nc as high as 5 to 10 times the nuclear equilibrium density n0 ' 0.16 fm−3 of neutrons and protons found in laboratory nuclei.

https://www.pdf-archive.com/2019/12/12/jm-lattimer-and-m-prakash-the-physics-of-neutron-stars/

12/12/2019 www.pdf-archive.com

Atomic model 76%

pair or grouping of particles, etc.) are created and reside in the orbits (inside the peripheral magnetic fields) of the atoms and stars, but not in their nuclei (*).

https://www.pdf-archive.com/2016/10/14/atomic-model/

14/10/2016 www.pdf-archive.com

JDIT-2017-0120-025 71%

The first article of 2016 to be published online in the Journal of Diagnostic Imaging in Therapy was on the subject ‘NMR-Active Nuclei for Biological and Biomedical Applications’, by Simon G.

https://www.pdf-archive.com/2017/05/30/jdit-2017-0120-025/

30/05/2017 www.pdf-archive.com

2017DBS Antibody Flyer 102017 web 71%

MyoD1 MOC-31 MyoD1 stains the nuclei of myoblasts in developing muscle tissues.

https://www.pdf-archive.com/2017/10/30/2017dbs-antibody-flyer-102017-web/

30/10/2017 www.pdf-archive.com

Henry Eyring. The Activated Complex in Chemi 70%

However, after this is done, the nuclei themselves can be assumed to move under the influence of these forces according to classical mechanics.

https://www.pdf-archive.com/2019/11/10/henry-eyring-the-activated-complex-in-chemi/

10/11/2019 www.pdf-archive.com

Cosmos Model 67%

atomic nuclei to electrons;

https://www.pdf-archive.com/2016/10/14/cosmos-model/

14/10/2016 www.pdf-archive.com

GammaSpectr revised Diehl 66%

Spectral signatures in the MeV regime originate from transitions in the nuclei of atoms (rather than in their electron shell).

https://www.pdf-archive.com/2014/02/11/gammaspectr-revised-diehl/

11/02/2014 www.pdf-archive.com

JDIT-2014-1030-006 66%

In contrast, poorly differentiated NETS have atypical, sheet-like, diffuse and irregular nuclei, less cytoplasmic secretory granules and limited biomarker immunoexpression.

https://www.pdf-archive.com/2017/05/30/jdit-2014-1030-006/

30/05/2017 www.pdf-archive.com

Dichiarazione TARI Padova utenza domestica.1474970816 64%

Posto auto coperto, cantina, altre pertinenze mq_____________ Che il numero complessivo delle persone, compreso il dichiarante, che occupano i locali oggetto della presente denuncia è pari a _________________ di cui non residenti_____________________________________________________ Dati dei componenti residenti appartenenti a nuclei famigliari anagraficamente distinti e non residenti (3) Cognome e Nome Luogo e data di nascita Codice fiscale 2 – CESSAZIONE 1 1 Data cessazione (vendita/rilascio locali) _____/_____/____ Immobile arredato 1 Utenze a rete attive DATI PROPRIETARIO Di proprietà di ___________________________________ C.F.____________________________________________ Residente in ______________________Via/P.zza___________________________________ n.______ Cap ________ _______________________________________________________________________________________________ 1 3 – VARIAZIONE DI SUPERFICIE/NUMERO COMPONENTI/ALTRO 1 VARIAZIONE DI SUPERFICIE (Allegare planimetria catastale dell’immobile) 1 VARIAZIONE NUMERO COMPONENTI ALTRO_____________________________________________________________________________________ Che il numero complessivo delle persone, compreso il dichiarante, che occupano i locali oggetto della presente denuncia è pari a _________________ di cui non residenti_____________________________________________________ Dati dei componenti residenti appartenenti a nuclei famigliari anagraficamente distinti e non residenti (3) Cognome e Nome Luogo e data di nascita Codice fiscale 1 Abitazione a disposizione per uso stagionale e discontinuo 1 4 – RIDUZIONI/AGEVOLAZIONI Residenza per più di 6 mesi all’anno per lavoro all’estero, riduzione n.

https://www.pdf-archive.com/2017/02/28/dichiarazione-tari-padova-utenza-domestica-1474970816/

28/02/2017 www.pdf-archive.com

Review of Basic Neuroscience 63%

 Raphe nuclei functions (see serotonin p7).

https://www.pdf-archive.com/2018/01/19/review-of-basic-neuroscience/

19/01/2018 www.pdf-archive.com

Internal Thermosense In Vertebrates 61%

• Anterior Hypothalamus • Spinal Cord • Abdominal Viscera • Great Veins Internal Thermoreceptors • Anterior Hypothalamus • Predominantly found in Pre-Optic Area (POA) • Posterior Nuclei of Hypothalamus receives projections from the POA • Predominantly warm-sensitive, in opposition to external thermoreceptors • “Anterior senses, posterior acts” • Thought to integrate information about local brain temperature and other body temperatures and to control the level of output for thermoregulatory responses based on cues Internal Thermoreceptors Thermal sensitivity range of transient receptor potential ion channels in mammals.

https://www.pdf-archive.com/2017/06/09/internal-thermosense-in-vertebrates/

09/06/2017 www.pdf-archive.com

Bira vK 61%

light nuclei  Unitarity: bosonic clusters  Unitarity:

https://www.pdf-archive.com/2017/10/11/bira-vk/

11/10/2017 www.pdf-archive.com

Furnstahl 61%

constituent quarks Multiple phenomenologies ab initio CI DFT collective models Resolution Constituent quarks Meson exchange models Cluster models Collective models Nuclei as Fermi liquids Nuclear pairing

https://www.pdf-archive.com/2017/10/11/furnstahl/

11/10/2017 www.pdf-archive.com

Presentazione Ionizzatore 61%

Per quanto detto prima 1 mole di H2O=20g dunque per ottenere 100 g di H2 occorrerà fornire al sistema 459 * 100= 459000 kj/L, ovvero 459000000 j/L , questo significa che per ottenere 100g di H+ in 1 ora fornendo al sistema 1A occorrerà una differenza di potenziale V =459000000/1(60*60)=127.5 Kv 2 Ionizzatore H2 In questa fase vengono preparati i nuclei di idrogeno da accelerare.

https://www.pdf-archive.com/2020/04/18/presentazione-ionizzatore/

18/04/2020 www.pdf-archive.com

Light and photons 61%

But for the moment we will only consider them as sub-atomic particles that can be grouped together forming higher ones, until the bigger accumulation of sub-atoms get to be the essential components of the atom, such as nuclei, electrons, neutrinos, etc.

https://www.pdf-archive.com/2018/03/30/light-and-photons/

30/03/2018 www.pdf-archive.com

DE180096.PDF 60%

Allegato 24a Profilo longitudinale di linea - Allegato 25a Stazione di partenza – sezioni - Allegato 33 Realizzazione di nuclei di rimboschimento - Allegato 34 Planimetria con proposte di intervento Sezione con visualizzazione degli interventi - particolari di progetto dei cavalletti in legname;

https://www.pdf-archive.com/2018/05/11/de180096/

11/05/2018 www.pdf-archive.com

NeuReport 58%

neutrinos pass out of the core unimpeded (2.3 seconds) 1 Single proton nuclei bound within can be modelled by considering unlike photons which take thousands of years to travel ν¯e + p+ → n0 + e+ .

https://www.pdf-archive.com/2013/01/14/neureport/

14/01/2013 www.pdf-archive.com

NUCL1530 58%

                Exploring careers in nuclear/radiological and health physics Atomic nuclei and its structure Environmental radioactivity General principles of radiation machines Survey on radiation detection methodologies Overview of fission and fusion processes Discussions on radioactive waste Medical and Industrial use of radiation Nuclear power systems and technologies (Nuclear reactors) Principles of CANDU reactor Nuclear fuel cycle Safety management concepts and safety culture Defense in depth concepts and relationships to reactor design Control, cool, contains concepts and safety design approaches Practice human performance and factors related to nuclear technologies &

https://www.pdf-archive.com/2016/05/26/nucl1530/

26/05/2016 www.pdf-archive.com

kortelainen 55%

● 28 rms radii ● 8 oes energies ● Optimization of Skyrme-like ED with respect of 12 parameters at the deformed HFB level NM NM NM NM −1 ρc , E / A , K , asym , Lsym , M s J Cρ0 Δ ρ , Cρ1 Δ ρ , V n0 , V 0p ,C ρ0 ∇ J ,C ρ∇ 1 UNEDF0 input data consisted of masses of deformed and spherical nuclei, charge radii, and pairing gaps ● Only time-even part of the EDF was adjusted for all UNEDF’s ● Orsay, 2-6.10.2017 Energy density optimization:

https://www.pdf-archive.com/2017/10/11/kortelainen/

11/10/2017 www.pdf-archive.com