{"id":16492,"date":"2020-03-06T03:56:34","date_gmt":"2020-03-06T03:56:34","guid":{"rendered":"https:\/\/www.radiation-dosimetry.org\/que-es-la-energia-de-ionizacion-definicion\/"},"modified":"2020-06-29T10:16:04","modified_gmt":"2020-06-29T10:16:04","slug":"que-es-la-energia-de-ionizacion-definicion","status":"publish","type":"post","link":"https:\/\/www.radiation-dosimetry.org\/es\/que-es-la-energia-de-ionizacion-definicion\/","title":{"rendered":"\u00bfQu\u00e9 es la energ\u00eda de ionizaci\u00f3n? Definici\u00f3n"},"content":{"rendered":"<div class=\"su-quote su-quote-style-default\">\n<div class=\"su-quote-inner su-u-clearfix su-u-trim\">Qu\u00e9 es la energ\u00eda de ionizaci\u00f3n.\u00a0La energ\u00eda de ionizaci\u00f3n, tambi\u00e9n llamada potencial de ionizaci\u00f3n, es la energ\u00eda necesaria para eliminar un electr\u00f3n del \u00e1tomo neutro.\u00a0Dosimetr\u00eda de radiaci\u00f3n<\/div>\n<\/div>\n<div class=\"su-divider su-divider-style-dotted\"><\/div>\n<div class=\"lgc-column lgc-grid-parent lgc-grid-100 lgc-tablet-grid-100 lgc-mobile-grid-100 lgc-equal-heights lgc-first lgc-last\">\n<div class=\"inside-grid-column\">\n<div class=\"su-spacer\"><\/div>\n<h2>Energ\u00eda de ionizaci\u00f3n<\/h2>\n<p><strong>La energ\u00eda de ionizaci\u00f3n<\/strong>\u00a0, tambi\u00e9n llamada\u00a0<strong>potencial de ionizaci\u00f3n<\/strong>\u00a0, es la energ\u00eda necesaria para\u00a0<strong>eliminar un electr\u00f3n<\/strong>\u00a0del \u00e1tomo neutro.<\/p>\n<p>X + energ\u00eda \u2192 X\u00a0<sup>+<\/sup>\u00a0+ e\u00a0<sup>&#8211;<\/sup><\/p>\n<p>donde X es cualquier \u00e1tomo o mol\u00e9cula capaz de ionizarse, X\u00a0<sup>+<\/sup>\u00a0es ese \u00e1tomo o mol\u00e9cula con un electr\u00f3n eliminado (ion positivo), y e\u00a0<sup>&#8211;<\/sup>\u00a0es el electr\u00f3n eliminado.<\/p>\n<p>Hay una energ\u00eda de ionizaci\u00f3n por cada electr\u00f3n sucesivo eliminado.\u00a0Los electrones que rodean el n\u00facleo se mueven en \u00f3rbitas bastante bien definidas.\u00a0Algunos de estos electrones est\u00e1n m\u00e1s unidos en el \u00e1tomo que otros.\u00a0Por ejemplo, solo se requieren 7.38 eV para eliminar el electr\u00f3n m\u00e1s externo de un \u00e1tomo de plomo, mientras que se requieren 88,000 eV para eliminar el electr\u00f3n m\u00e1s interno.<\/p>\n<ul>\n<li><strong>La energ\u00eda de ionizaci\u00f3n<\/strong>\u00a0es m\u00e1s baja para los metales alcalinos que tienen un solo electr\u00f3n fuera de una cubierta cerrada.<\/li>\n<li><strong>La energ\u00eda de ionizaci\u00f3n<\/strong>\u00a0aumenta a trav\u00e9s de una fila en el m\u00e1ximo peri\u00f3dico para los gases nobles que tienen conchas cerradas.<\/li>\n<\/ul>\n<p>Por ejemplo, el sodio requiere solo 496 kJ \/ mol o 5.14 eV \/ \u00e1tomo para ionizarlo.\u00a0Por otro lado, el ne\u00f3n, el gas noble, que lo precede inmediatamente en la tabla peri\u00f3dica, requiere 2081 kJ \/ mol o 21.56 eV \/ \u00e1tomo.<\/p>\n<p>La energ\u00eda de ionizaci\u00f3n asociada con la eliminaci\u00f3n del primer electr\u00f3n se usa con mayor frecuencia.\u00a0El\u00a0<em>n<\/em>\u00a0energ\u00eda \u00ba ionizaci\u00f3n se refiere a la cantidad de energ\u00eda requerida para quitar un electr\u00f3n de la especie con una carga de (\u00a0<em>n<\/em>\u00a0-1).<\/p>\n<p>1ra energ\u00eda de ionizaci\u00f3n<\/p>\n<p>X \u2192 X\u00a0<sup>+<\/sup>\u00a0+ e\u00a0<sup>&#8211;<\/sup><\/p>\n<p>2da energ\u00eda de ionizaci\u00f3n<\/p>\n<p>X\u00a0<sup>+<\/sup>\u00a0\u2192 X\u00a0<sup>2+<\/sup>\u00a0+ e\u00a0<sup>&#8211;<\/sup><\/p>\n<div class=\"lgc-column lgc-grid-parent lgc-grid-100 lgc-tablet-grid-100 lgc-mobile-grid-100 lgc-equal-heights  lgc-first lgc-last\">\n<div class=\"inside-grid-column\">\n<p><span>3ra energ\u00eda de ionizaci\u00f3n<\/span><\/p>\n<p><span>X\u00a0<\/span><sup><span>2+<\/span><\/sup><span>\u00a0\u2192 X\u00a0<\/span><sup><span>3+<\/span><\/sup><span>\u00a0+ e\u00a0<\/span><sup><span>&#8211;<\/span><\/sup><\/p>\n<p><span>Por ejemplo, solo se requieren 7.38 eV para eliminar el electr\u00f3n m\u00e1s externo de un \u00e1tomo de plomo, mientras que se requieren 88,000 eV para eliminar el electr\u00f3n m\u00e1s interno.<\/span><\/p>\n<figure id=\"attachment_16766\" class=\"wp-caption aligncenter\" aria-describedby=\"caption-attachment-16766\"><a href=\"https:\/\/www.radiation-dosimetry.org\/wp-content\/uploads\/2019\/12\/Ionization-energy-first-min.png\"><img loading=\"lazy\" class=\"size-full wp-image-16766 lazy-loaded\" src=\"https:\/\/www.radiation-dosimetry.org\/wp-content\/uploads\/2019\/12\/Ionization-energy-first-min.png\" alt=\"Energ\u00eda de ionizaci\u00f3n\" width=\"1139\" height=\"432\" data-lazy-type=\"image\" data-src=\"https:\/\/www.radiation-dosimetry.org\/wp-content\/uploads\/2019\/12\/Ionization-energy-first-min.png\" \/><\/a><figcaption id=\"caption-attachment-16766\" class=\"wp-caption-text\"><span>Fuente: wikipedia.org Licencia: CC BY-SA 3.0<\/span><\/figcaption><\/figure>\n<\/div>\n<\/div>\n<div class=\"lgc-column lgc-grid-parent lgc-grid-100 lgc-tablet-grid-100 lgc-mobile-grid-100 lgc-equal-heights  lgc-first lgc-last\">\n<div class=\"inside-grid-column\">\n<div class=\"su-spacer\"><\/div>\n<h2><span>Electronvoltio &#8211; Unidad de energ\u00eda<\/span><\/h2>\n<figure id=\"attachment_16549\" class=\"wp-caption alignright\" aria-describedby=\"caption-attachment-16549\"><a href=\"https:\/\/www.radiation-dosimetry.org\/wp-content\/uploads\/2019\/12\/electronvolt-definition-min.png\"><img loading=\"lazy\" class=\"size-medium wp-image-16549 lazy-loaded\" src=\"https:\/\/www.radiation-dosimetry.org\/wp-content\/uploads\/2019\/12\/electronvolt-definition-min-188x300.png\" alt=\"Electronvolt - definici\u00f3n\" width=\"188\" height=\"300\" data-lazy-type=\"image\" data-src=\"https:\/\/www.radiation-dosimetry.org\/wp-content\/uploads\/2019\/12\/electronvolt-definition-min-188x300.png\" \/><\/a><figcaption id=\"caption-attachment-16549\" class=\"wp-caption-text\"><span>Electronvolt es igual a la energ\u00eda obtenida por un solo electr\u00f3n cuando se acelera a trav\u00e9s de 1 voltio de diferencia de potencial el\u00e9ctrico.\u00a0El trabajo realizado en la carga viene dado por la carga multiplicada por la diferencia de voltaje, por lo tanto, el trabajo W en el electr\u00f3n es: W = qV = (1.6 x 10-19 C) x (1 J \/ C) = 1.6 x 10-19 J .<\/span><\/figcaption><\/figure>\n<p><strong><span>Electronvoltio (unidad: eV)<\/span><\/strong><span>\u00a0.\u00a0Los electronvoltios son una unidad tradicional de energ\u00eda, particularmente en\u00a0<\/span><a title=\"F\u00edsica At\u00f3mica y Nuclear\" href=\"https:\/\/www.nuclear-power.com\/nuclear-power\/reactor-physics\/atomic-nuclear-physics\/\"><span>f\u00edsica at\u00f3mica y nuclear<\/span><\/a><span>\u00a0.\u00a0Electronvolt es igual a la energ\u00eda obtenida por un solo electr\u00f3n cuando se\u00a0<\/span><strong><span>acelera a<\/span><\/strong><span>\u00a0trav\u00e9s de\u00a0<\/span><strong><span>1 voltio<\/span><\/strong><span>\u00a0de\u00a0diferencia de\u00a0<\/span><strong><span>potencial el\u00e9ctrico<\/span><\/strong><span>\u00a0.\u00a0El trabajo realizado sobre la carga est\u00e1 dada por los tiempos de carga la diferencia de voltaje, por lo tanto el trabajo W en electrones es: W = qV = (1,6 x 10\u00a0<\/span><sup><span>-19<\/span><\/sup><span>\u00a0C) x (1 J \/ C) =\u00a0<\/span><strong><span>1,6 x 10\u00a0<\/span><sup><span>-19<\/span><\/sup><span>\u00a0J<\/span><\/strong><span>\u00a0.\u00a0Como se trata de una unidad muy peque\u00f1a, es m\u00e1s conveniente utilizar m\u00faltiplos de electronvoltios: kiloelectrvoltios (keV), megaelectrvoltios (MeV), gigavoltios (GeV), etc.\u00a0Desde que Albert Einstein demostr\u00f3 que<\/span><a title=\"Conservaci\u00f3n de Mass-Energy - Equivalencia de Mass-Energy\" href=\"https:\/\/www.nuclear-power.com\/laws-of-conservation\/law-of-conservation-of-energy\/conservation-of-mass-energy-mass-energy-equivalence\/\"><span>masa y energ\u00eda<\/span><\/a><span>\u00a0son\u00a0<\/span><strong><span>equivalentes y convertibles<\/span><\/strong><span>\u00a0una en la otra, el electronvoltio es tambi\u00e9n una unidad de masa.\u00a0Es com\u00fan en la f\u00edsica de part\u00edculas, donde las unidades de masa y energ\u00eda a menudo se intercambian, expresar la masa en unidades de eV \/ c\u00a0<\/span><sup><span>2<\/span><\/sup><span>\u00a0, donde c es la velocidad de la luz en el vac\u00edo (de E = mc\u00a0<\/span><sup><span>2<\/span><\/sup><span>\u00a0).\u00a0Por ejemplo, se puede decir que el\u00a0<\/span><strong><span>prot\u00f3n<\/span><\/strong><span>\u00a0tiene una masa de\u00a0<\/span><strong><span>938.3 MeV<\/span><\/strong><span>\u00a0, aunque estrictamente hablando deber\u00eda ser\u00a0<\/span><strong><span>938.3 MeV \/ c\u00a0<\/span><sup><span>2<\/span><\/sup><\/strong><span>\u00a0.\u00a0Para otro ejemplo, una\u00a0<\/span><a title=\"Aniquilaci\u00f3n de positrones\" href=\"https:\/\/www.nuclear-power.com\/nuclear-power\/reactor-physics\/atomic-nuclear-physics\/fundamental-particles\/beta-particle\/positron-annihilation-2\/\"><span>aniquilaci\u00f3n electr\u00f3n-positr\u00f3n<\/span><\/a><span>\u00a0ocurre cuando un electr\u00f3n cargado negativamente y un positr\u00f3n cargado positivamente (cada uno con una masa de 0.511 MeV \/ c\u00a0<\/span><sup><span>2<\/span><\/sup><span>) chocar.\u00a0Cuando un electr\u00f3n y un positr\u00f3n chocan, se aniquilan, lo que resulta en la conversi\u00f3n completa de su masa en reposo a energ\u00eda pura (de acuerdo con la\u00a0<a title=\"E = mc2 Significado\" href=\"https:\/\/www.nuclear-power.com\/nuclear-power\/nuclear-energy\/emc2-meaning\/\">f\u00f3rmula\u00a0<\/a><\/span><a title=\"E = mc2 Significado\" href=\"https:\/\/www.nuclear-power.com\/nuclear-power\/nuclear-energy\/emc2-meaning\/\"><span>E = mc\u00a0<\/span><sup><span>2<\/span><\/sup><\/a><span>\u00a0) en forma de dos\u00a0<\/span><a title=\"Rayos Gamma \/ Radiaci\u00f3n Gamma\" href=\"https:\/\/www.nuclear-power.com\/nuclear-power\/reactor-physics\/atomic-nuclear-physics\/fundamental-particles\/photon\/gamma-ray\/\"><span>rayos gamma<\/span><\/a><span>\u00a0(fotones) de\u00a00.511 MeV opuestos\u00a0.<\/span><\/p>\n<p><strong><span>e\u00a0<\/span><\/strong><strong><sup><span>&#8211;<\/span><\/sup><\/strong><strong><span>\u00a0+ e\u00a0<\/span><\/strong><strong><sup><span>+<\/span><\/sup><\/strong><strong><span>\u00a0\u2192 \u03b3 + \u03b3 (2x 0.511 MeV)<\/span><\/strong><\/p>\n<ul>\n<li><span>1 eV = 1,603 x 10\u00a0<\/span><sup><span>-19<\/span><\/sup><span>\u00a0J<\/span><\/li>\n<li><span>1 eV = 3.83 x\u00a0<\/span><sup><span>10-20<\/span><\/sup><span>\u00a0cal<\/span><\/li>\n<li><span>1 eV = 1.52 x 10\u00a0<\/span><sup><span>-22<\/span><\/sup><span>\u00a0BTU<\/span><\/li>\n<\/ul>\n<p><a href=\"https:\/\/www.radiation-dosimetry.org\/wp-content\/uploads\/2019\/12\/conversion-megawattday-electronvolt-energy-units.png\"><img loading=\"lazy\" class=\"aligncenter size-large wp-image-16546 lazy-loaded\" src=\"https:\/\/www.radiation-dosimetry.org\/wp-content\/uploads\/2019\/12\/conversion-megawattday-electronvolt-energy-units-1024x291.png\" alt=\"conversi\u00f3n-megavatio, electronvoltio - unidades de energ\u00eda\" width=\"669\" height=\"190\" data-lazy-type=\"image\" data-src=\"https:\/\/www.radiation-dosimetry.org\/wp-content\/uploads\/2019\/12\/conversion-megawattday-electronvolt-energy-units-1024x291.png\" \/><\/a><\/p>\n<h2><strong><span>Ejemplo de energ\u00edas en electronvoltios<\/span><\/strong><\/h2>\n<ul>\n<li><a title=\"Neutrones t\u00e9rmicos\" href=\"https:\/\/www.nuclear-power.com\/nuclear-power\/reactor-physics\/atomic-nuclear-physics\/fundamental-particles\/neutron\/thermal-neutron\/\"><strong><span>Los neutrones t\u00e9rmicos<\/span><\/strong><\/a><span>\u00a0son neutrones en equilibrio t\u00e9rmico<\/span><strong><span>\u00a0con un medio circundante de temperatura 290K (17 \u00b0 C o 62 \u00b0 F)<\/span><\/strong><span>\u00a0.\u00a0La energ\u00eda m\u00e1s probable a 17 \u00b0 C (62 \u00b0 F) para la distribuci\u00f3n Maxwelliana es<\/span><strong><span>\u00a00.025 eV<\/span><\/strong><span>\u00a0(~ 2 km \/ s).<\/span><\/li>\n<li><span>La energ\u00eda t\u00e9rmica de una mol\u00e9cula est\u00e1 a temperatura ambiente aproximadamente\u00a0<\/span><strong><span>0.04 eV<\/span><\/strong><span>\u00a0.<\/span><\/li>\n<li><span>Aproximadamente\u00a0<\/span><strong><span>1 eV<\/span><\/strong><span>\u00a0corresponde a un\u00a0<strong><a title=\"Fot\u00f3n - Part\u00edcula fundamental\" href=\"https:\/\/www.nuclear-power.com\/nuclear-power\/reactor-physics\/atomic-nuclear-physics\/fundamental-particles\/photon\/\">fot\u00f3n<\/a><\/strong><\/span><strong><span>\u00a0infrarrojo<\/span><\/strong><span>\u00a0de longitud de onda de 1240 nm.<\/span><\/li>\n<li><span>Los fotones de luz visible tienen energ\u00edas en el rango 1.65 eV (rojo) &#8211; 3.26 eV (violeta).<\/span><\/li>\n<li><span>La primera\u00a0<\/span><a title=\"\u00bfQu\u00e9 es la resonancia nuclear? - N\u00facleo compuesto\" href=\"https:\/\/www.nuclear-power.com\/nuclear-power\/reactor-physics\/nuclear-engineering-fundamentals\/neutron-nuclear-reactions\/compound-nucleus-reactions\/what-is-nuclear-resonance-compound-nucleus\/\"><span>resonancia<\/span><\/a><span>\u00a0en la\u00a0reacci\u00f3n\u00a0n +\u00a0<\/span><a href=\"https:\/\/www.nuclear-power.com\/nuclear-power-plant\/nuclear-fuel\/uranium\/uranium-238\/\"><sup><span>238<\/span><\/sup><span>\u00a0U<\/span><\/a><span>\u00a0es\u00a0<\/span><strong><span>a 6.67 eV<\/span><\/strong><span>\u00a0(energ\u00eda del neutr\u00f3n incidente), que corresponde al primer\u00a0<\/span><strong><span>nivel virtual en\u00a0<\/span><\/strong><strong><sup><span>239<\/span><\/sup><\/strong><strong><span>\u00a0U<\/span><\/strong><span>\u00a0, tiene un ancho total de solo 0.027 eV, y la vida media de este estado es 2.4 \u00d7 10\u00a0<\/span><sup><span>-14<\/span><\/sup><span>\u00a0s.<\/span><\/li>\n<li><span>La energ\u00eda de ionizaci\u00f3n del hidr\u00f3geno at\u00f3mico es de\u00a0<\/span><strong><span>13,6 eV<\/span><\/strong><span>\u00a0.<\/span><\/li>\n<li><span>El carbono 14 se desintegra en nitr\u00f3geno 14 a trav\u00e9s de\u00a0<\/span><a href=\"http:\/\/radiation-dosimetry.org\/ionizing-radiation\/beta-decay\/\"><span>la desintegraci\u00f3n beta<\/span><\/a><span>\u00a0(desintegraci\u00f3n beta pura).\u00a0Las\u00a0<\/span><a title=\"Part\u00edcula Beta\" href=\"https:\/\/www.nuclear-power.com\/nuclear-power\/reactor-physics\/atomic-nuclear-physics\/fundamental-particles\/beta-particle\/\"><span>part\u00edculas beta<\/span><\/a><span>\u00a0emitidas\u00a0tienen una energ\u00eda m\u00e1xima de 156 keV, mientras que su energ\u00eda media ponderada es de\u00a0<\/span><strong><span>49 keV<\/span><\/strong><span>\u00a0.<\/span><\/li>\n<li><span>Los fotones de rayos X m\u00e9dicos de diagn\u00f3stico de alta energ\u00eda tienen energ\u00edas cin\u00e9ticas de aproximadamente\u00a0<\/span><strong><span>200 keV.<\/span><\/strong><\/li>\n<li><strong><span>El talio 208,<\/span><\/strong><span>\u00a0que es uno de los nucleidos en la\u00a0cadena de descomposici\u00f3n de\u00a0<\/span><a title=\"Uranio 232\" href=\"https:\/\/www.nuclear-power.com\/nuclear-power-plant\/nuclear-fuel\/uranium\/uranium-232\/\"><strong><sup><span>232<\/span><\/sup><span>\u00a0U<\/span><\/strong><\/a><span>\u00a0,\u00a0<\/span><strong><span>emite\u00a0<\/span><\/strong><strong><a href=\"https:\/\/www.nuclear-power.com\/nuclear-power\/reactor-physics\/atomic-nuclear-physics\/fundamental-particles\/photon\/gamma-ray\/\"><span>rayos gamma<\/span><\/a><\/strong><strong><span>\u00a0de 2.6 MeV que son muy en\u00e9rgicos y altamente penetrantes.<\/span><\/strong><\/li>\n<li><span>La energ\u00eda cin\u00e9tica t\u00edpica de\u00a0<\/span><a title=\"Part\u00edcula alfa\" href=\"https:\/\/www.nuclear-power.com\/nuclear-power\/reactor-physics\/atomic-nuclear-physics\/fundamental-particles\/alpha-particle\/\"><strong><span>la part\u00edcula alfa<\/span><\/strong><\/a><span>\u00a0de la desintegraci\u00f3n radiactiva es de aproximadamente\u00a0<\/span><strong><span>5 MeV<\/span><\/strong><span>\u00a0.\u00a0Es causado por el mecanismo de su producci\u00f3n.<\/span><\/li>\n<li><strong><span>La\u00a0<\/span><a title=\"Liberaci\u00f3n de energ\u00eda de la fisi\u00f3n\" href=\"https:\/\/www.nuclear-power.com\/nuclear-power\/fission\/energy-release-from-fission\/\"><span>energ\u00eda total liberada<\/span><\/a><\/strong><span>\u00a0en un reactor es de\u00a0<\/span><strong><span>aproximadamente 210 MeV<\/span><\/strong><span>\u00a0por\u00a0<\/span><a href=\"https:\/\/www.nuclear-power.com\/nuclear-power-plant\/nuclear-fuel\/uranium\/uranium-235\/uranium-235-fission\/\"><sup><span>235<\/span><\/sup><span>\u00a0U de fisi\u00f3n<\/span><\/a><span>\u00a0, distribuida como se muestra en la tabla.\u00a0En un reactor,\u00a0<\/span><strong><span>la energ\u00eda recuperable promedio<\/span><\/strong><span>\u00a0por fisi\u00f3n es de\u00a0<\/span><strong><span>aproximadamente 200 MeV<\/span><\/strong><span>\u00a0, siendo la energ\u00eda total menos la energ\u00eda de la energ\u00eda de los\u00a0<\/span><a href=\"https:\/\/www.nuclear-power.com\/nuclear-power\/reactor-physics\/atomic-nuclear-physics\/fundamental-particles\/antineutrino\/\"><span>antineutrinos<\/span><\/a><span>\u00a0que se irradian.<\/span><\/li>\n<li><span>El rayo c\u00f3smico puede tener energ\u00edas de\u00a0<\/span><strong><span>1 MeV &#8211; 1000 TeV<\/span><\/strong><span>\u00a0.<\/span><\/li>\n<\/ul>\n<\/div>\n<\/div>\n<div class=\"lgc-column lgc-grid-parent lgc-grid-100 lgc-tablet-grid-100 lgc-mobile-grid-100 lgc-equal-heights  lgc-first lgc-last\">\n<div class=\"inside-grid-column\"><\/div>\n<\/div>\n<\/div>\n<\/div>\n<p>&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;&#8230;.<\/p>\n<p>Este art\u00edculo se basa en la traducci\u00f3n autom\u00e1tica del art\u00edculo original en ingl\u00e9s. Para m\u00e1s informaci\u00f3n vea el art\u00edculo en ingl\u00e9s. Puedes ayudarnos. Si desea corregir la traducci\u00f3n, env\u00edela a: translations@nuclear-power.com o complete el formulario de traducci\u00f3n en l\u00ednea. Agradecemos su ayuda, actualizaremos la traducci\u00f3n lo antes posible. Gracias.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Qu\u00e9 es la energ\u00eda de ionizaci\u00f3n.\u00a0La energ\u00eda de ionizaci\u00f3n, tambi\u00e9n llamada potencial de ionizaci\u00f3n, es la energ\u00eda necesaria para eliminar un electr\u00f3n del \u00e1tomo neutro.\u00a0Dosimetr\u00eda de radiaci\u00f3n Energ\u00eda de ionizaci\u00f3n La energ\u00eda de ionizaci\u00f3n\u00a0, tambi\u00e9n llamada\u00a0potencial de ionizaci\u00f3n\u00a0, es la energ\u00eda necesaria para\u00a0eliminar un electr\u00f3n\u00a0del \u00e1tomo neutro. X + energ\u00eda \u2192 X\u00a0+\u00a0+ e\u00a0&#8211; donde X &#8230; <a title=\"\u00bfQu\u00e9 es la energ\u00eda de ionizaci\u00f3n? Definici\u00f3n\" class=\"read-more\" href=\"https:\/\/www.radiation-dosimetry.org\/es\/que-es-la-energia-de-ionizacion-definicion\/\" aria-label=\"M\u00e1s en \u00bfQu\u00e9 es la energ\u00eda de ionizaci\u00f3n? Definici\u00f3n\">Leer m\u00e1s<\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":[],"categories":[50],"tags":[],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v15.4 - https:\/\/yoast.com\/wordpress\/plugins\/seo\/ -->\n<title>\u00bfQu\u00e9 es la energ\u00eda de ionizaci\u00f3n? Definici\u00f3n<\/title>\n<meta name=\"description\" content=\"Qu\u00e9 es la energ\u00eda de ionizaci\u00f3n. La energ\u00eda de ionizaci\u00f3n, tambi\u00e9n llamada potencial de ionizaci\u00f3n, es la energ\u00eda necesaria para eliminar un electr\u00f3n del \u00e1tomo neutro. 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