Analytical Chemistry 2018-The Effect Of Gravitational Waves And Dark Matter In Daily Life- Edward H Jimenez- Central University Of Ecuador
Notice bibliographique
Résumé
Dark matter interacts with baryonic matter through gravitational force and weak force. There are reasons to believe it does not interact directly with the strong nuclear force. Moreover, if dark matter is hidden in the nuclear surface, then it can be detected through a variation of the effective K-edge cross section. On the contrary, if it is hidden inside the nuclear core, then it must produce a variation of the nuclear viscosity. The Femtoscope and low-energy x-ray spectroscopy allow us to measure the K-edge resonance and, at the same time, the absence or not of dark matter. We present two methods on the use of K-edge XANES spectroscopy for organic and inorganic compounds, one theoretical and one experimental. We can determine the absence or not of dark matter in the atomic nucleus, essentially in Phosphorus, Xenon, Thulium and Chromium. The algorithms are sufficiently manageable. This allows us to illustrate that our experimental arrangement is in agreement with underground laboratories providing direct detection experiments such as SNOLAB, Gran Sasso, Canfranc, Deep Underground Science and Engineering Laboratory and the China Jinping Underground Laboratory. On the other hand, after processing the information of 12000 cancer patients, who have received doses of radiation with energies of the order of 6 MeV, we review all the treatment protocols before an irradiation. We have detected in a single file, recorded in radiography and digital information, where a part of the LINAC moved at a speed close to light in a vacuum, indicating a possible existence of gravitational waves. The coefficient ΔL / L = 0.00005, is higher than the value measured on 2017 by Nobel Prize in physics, which is ΔL / L = 10-18.The Laser Interferometer Space Antenna (LISA) will enable astrophysicists to observe gravitational waves emitted by black holes as they collide with or capture other black holes. LISA will consist of three spacecraft orbiting the sun in a constant triangle formation. Gravitational waves passing through will distort the sides of the triangle slightly, and these minimal distortions can be detected by laser beams connecting the spacecraft. LISA could therefore add a new sense to scientists' perception of the universe and enable them to study phenomena invisible in different light spectra. Scientists from the Center for Theoretical Astrophysics and Cosmology of the University of Zurich, together with colleagues from Greece and Canada, have now found that LISA will not only be able to measure these previously unstudied waves, but could also help to unveil secrets about dark mark Biography Edward H Jimenez has a PhD in Applied Mathematics from the University of Saint Etienne in France, his Bachelor is in Nuclear Physics and his masters are in Game Theory and Artificial Intelligence. Currently, he is a professor at the Central University of Ecuador in the Faculty of Chemical Engineering, and has worked for 19 years in the oil industry in the area of catalysis and nanotechnology of Si / Al / P using x-ray spectroscopy. He has published more than 20 papers with referee and 6 books of high impact in Ecuador. Nicolas Recalde, has worked for 15 years in cancer radiotherapy at Georgetown University Medical Center and Inova Health System, USA. He was Chief Medical Physicist at Potomac Radiation Center in Virginia, USA. He is a diplomate of the American Board of Radiology and a member of the American Association of Physicists in Medicine.
Récupéré en direct depuis OpenAlex et désinversé. Les résumés ne sont pas conservés dans cette base de données : les index inversés représentent 8,6 Go des 9,3 Go de texte de la base, et le serveur dispose de 13 Go libres.
Comment cette classification a été obtenuedéplier
Prédiction machine sur la base complète
Imitation des enseignantsNi prévalence calibrée, ni vérité terrain. Validation humaine à venir. Le volet Gemma est une étiquette directe du modèle pour chaque travail de la base, lue sur la notice réduite au titre. Le volet Codex est un classifieur appris des 10 348 étiquettes directes de Codex et calibré sur les taux pondérés de l'échantillon; les champs sans appui suffisant ne portent aucun appel Codex. Le mode candidate est l'union des deux volets; le consensus est leur intersection. Ces sorties portent le statut machine_predicted_unvalidated et ne sont pas des étiquettes humaines.
Scores du classifieur distillé par catégorie (deux têtes)
| Catégorie | Codex | Gemma |
|---|---|---|
| Métarecherche | 0,002 | 0,002 |
| Méta-épidémiologie (sens strict) | 0,001 | 0,000 |
| Méta-épidémiologie (sens large) | 0,001 | 0,000 |
| Bibliométrie | 0,002 | 0,001 |
| Études des sciences et des technologies | 0,002 | 0,001 |
| Communication savante | 0,004 | 0,002 |
| Science ouverte | 0,001 | 0,002 |
| Intégrité de la recherche | 0,001 | 0,001 |
| Charge utile insuffisante (le modèle a refusé de juger) | 0,028 | 0,004 |
Scores machine (provisoires)
Les deux têtes enseignantes du modèle étudiant, lues sur ce travail. Un score ordonne la base pour la relecture; il n'affirme jamais une catégorie, et le statut de validation accompagne chaque rangée tel quel.
Scores de référence d'un modèle non mature (critères de maturité non atteints, 7 itérations). Un score ordonne; il n'affirme jamais une catégorie.
score_only:v0-immature-baseline · tel quel depuis la passe de notation : score_only signifie que le nombre peut ordonner les travaux, et qu'aucune étiquette de catégorie n'en découleClassification
machine, non validéePrédiction automatique; un appel candidat d’une seule source (Gemma direct ou Codex distillé), pas un consensus.
Le détail, modèle par modèle et score par score, se trouve en fin de page sous « Comment cette classification a été obtenue ».