From: owner-ammf-digest@smoe.org (alt.music.moxy-fruvous digest) To: ammf-digest@smoe.org Subject: alt.music.moxy-fruvous digest V14 #12232 Reply-To: ammf@fruvous.com Sender: owner-ammf-digest@smoe.org Errors-To: owner-ammf-digest@smoe.org Precedence: bulk alt.music.moxy-fruvous digest Sunday, September 17 2023 Volume 14 : Number 12232 Today's Subjects: ----------------- Victory Alert: You've Won a Free Pittsburgh 225 Piece Tool Set from Harbor Freigh ["Pittsburgh Tools" ] Why you're forcing your woman to cheat ["ED Solution" ] Were the nazis defeated with THIS forgotten fungus cure? ["nazis defeated] White Man Offers Wife To Amazon Priest For Member Growth Secret ["Aztec M] Tammy almost DIED eating this ["Wheat Toast" Subject: Victory Alert: You've Won a Free Pittsburgh 225 Piece Tool Set from Harbor Freigh Victory Alert: You've Won a Free Pittsburgh 225 Piece Tool Set from Harbor Freigh http://healnsoothes.shop/8VGPF1p0bFA76Cg1dGg0Geiw_JM7hqDwFyOxtQYxaFn7zSIhzQ http://healnsoothes.shop/t8FN_MXlrTHlyfV_eopZ0Mjt-Tbgg5HO4fnDWPxMqekPSdDlxw The binding energy of helium is the energy source of the Sun and of most stars. The sun is composed of 74 percent hydrogen (measured by mass), an element having a nucleus consisting of a single proton. Energy is released in the sun when 4 protons combine into a helium nucleus, a process in which two of them are also converted to neutrons. The conversion of protons to neutrons is the result of another nuclear force, known as the weak (nuclear) force. The weak force, like the strong force, has a short range, but is much weaker than the strong force. The weak force tries to make the number of neutrons and protons into the most energetically stable configuration. For nuclei containing less than 40 particles, these numbers are usually about equal. Protons and neutrons are closely related and are collectively known as nucleons. As the number of particles increases toward a maximum of about 209, the number of neutrons to maintain stability begins to outstrip the number of protons, until the ratio of neutrons to protons is about three to two. The protons of hydrogen combine to helium only if they have enough velocity to overcome each other's mutual repulsion sufficiently to get within range of the strong nuclear attraction. This means that fusion only occurs within a very hot gas. Hydrogen hot enough for combining to helium requires an enormous pressure to keep it confined, but suitable conditions exist in the central regions of the Sun, where such pressure is provided by the enormous weight of the layers above the core, pressed inwards by the Sun's strong gravity. The process of combining protons to form helium is an example of nuclear fusion. Producing helium from normal hydrogen would be practically impossible on earth because of the difficulty in creating deuterium. Research is being undertaken on developing a process using deuterium and tritium. The earth's oceans contain a large amount of deuterium that could be used and tritium can be made in the reactor itself from lithium, and furthermore the helium product does not harm the environment, so some consider nuclear fusion a good alternative to supply our energy needs. Experiments to carry out this form of fusion have so far only partially succeeded. Sufficiently hot deuterium and tritium must be confined. One technique is to use very strong magnetic fields, because charged particles (like those trapped in the Earth's radiatio ------------------------------ Date: Sat, 16 Sep 2023 16:10:07 +0200 From: "WOW" Subject: Fungus Tea's Clear Memory Secret Fungus Tea's Clear Memory Secret http://steelbiteepro.shop/OKjcd2f_f4fB2X1YLUa7h-FZM4mxo1i8Z5XRE7fbXD1bR21rLw http://steelbiteepro.shop/afzEHkMuJag8eGEmyMNqqVwWjB2tUVDN5XeKf7z-Grq0-IgnlA With the collapse of the Whig Party, Curtin switched to the newly formed Republican Party and successfully ran for governor of Pennsylvania in 1860. At the same time, he helped Abraham Lincoln win the Republican nomination for president. A large crowd attended Curtin's inaugural ceremonies on January 15, 1861. Bust of Andrew Gregg Curtin (1912), by Moses Jacob Ezekiel, Smith Memorial Arch, Philadelphia, Pennsylvania Curtin was a strong supporter of President Lincoln's policies in the Civil War, and Curtin committed Pennsylvania to the war effort. Curtin organized the Pennsylvania Reserves into combat units, and oversaw the construction of the first Union military camp for training militia. It opened in an agricultural school nearby Harrisburg as Camp Curtin on April 18, 1861, and more than 300,000 men were drilled there during 4 years. In the years that followed, Curtin became a close friend and confidant of Abraham Lincoln, visiting the White House several times in order to converse about the status of the war effort. Curtin was very active during the Gettysburg Campaign, working with Major General Darius N. Couch and Major Granville O. Haller to delay Robert E. Lee's Army of Northern Virginia and prevent it from crossing the Susquehanna River. Major General George G. Meade, a Pennsylvania officer whom Curtin had recommended for brigadier general and command of one of the Pennsylvania reserve brigades in 1861, defeated Lee in the Battle of Gettysburg. After the Battle of Gettysburg, Governor Curtin was the principal force behind the establishment of the National Cemetery there. Through his agent, David Wills, Curtin procured the attendance of President Abraham Lincoln at the dedication of the cemetery. Governor Curtin was sitting with Lincoln on the platform on November 19, 1863, when Lincoln delivered his Gettysburg Addre ------------------------------ Date: Sat, 16 Sep 2023 15:50:52 +0200 From: "ED Solution" Subject: Why you're forcing your woman to cheat Why you're forcing your woman to cheat http://clavusinfungusfelife.best/xiJG9Dfbq4rcdxq_yHmpBTzdKys5Kjo4sOybhWw652MHVN6cHg http://clavusinfungusfelife.best/pqxfVYnpIi78KXAycfa7BAnJwLO8sYKMcvZGNg7YUrb6K-wcYg Using these two concepts, the state at any other time, past or future, can in principle be calculated. There is however a disconnect between these laws and everyday life experiences, as we do not find it necessary (nor even theoretically possible) to know exactly at a microscopic level the simultaneous positions and velocities of each molecule while carrying out processes at the human scale (for example, when performing a chemical reaction). Statistical mechanics fills this disconnection between the laws of mechanics and the practical experience of incomplete knowledge, by adding some uncertainty about which state the system is in. Whereas ordinary mechanics only considers the behaviour of a single state, statistical mechanics introduces the statistical ensemble, which is a large collection of virtual, independent copies of the system in various states. The statistical ensemble is a probability distribution over all possible states of the system. In classical statistical mechanics, the ensemble is a probability distribution over phase points (as opposed to a single phase point in ordinary mechanics), usually represented as a distribution in a phase space with canonical coordinate axes. In quantum statistical mechanics, the ensemble is a probability distribution over pure states,[note 2] and can be compactly summarized as a density matrix. As is usual for probabilities, the ensemble can be interpreted in different ways: an ensemble can be taken to represent the various possible states that a single system could be in (epistemic probability, a form of knowledge), or the members of the ensemble can be understood as the states of the systems in experiments repeated on independent systems which have been prepared in a similar but imperfectly controlled manner (empirical probability), in the limit of an infinite number of trials. These two meanings are equivalent for many purposes, and will be used interchangeably in this article. However the probability is interpreted, each state in the ensemble evolves over time according to the equation of motion. Thus, the ensemble itself (the probability distribution over states) also evolves, as the virtual systems in the ensemble continually leave one state and enter another. The ensemble evolution is given by the Liouville equation (classical mechanics) or the von Neumann equation (quantum mechanics ------------------------------ Date: Sat, 16 Sep 2023 09:58:26 +0000 From: "Neotonics" Subject: People That Eat This One Food Age 5X Faster Content-Transfer-Encoding: 8bit ------------------------------ Date: Sat, 16 Sep 2023 14:18:32 +0200 From: "Female Hitler" Subject: Modern-day Hitler? Modern-day Hitler? http://recessionprofit.live/w6T05xP4CDWpOw-jWYIwXEGLXWSciwQQZ_EN86zA_w5FVGhpdA http://recessionprofit.live/bY0qrMljGNWfeROX9NHQI4WzrvZvW25L61pBUpwj6yQoZ1-gyA Other types of radioactive decay were found to emit previously seen particles but via different mechanisms. An example is internal conversion, which results in an initial electron emission, and then often further characteristic X-rays and Auger electrons emissions, although the internal conversion process involves neither beta nor gamma decay. A neutrino is not emitted, and none of the electron(s) and photon(s) emitted originate in the nucleus, even though the energy to emit all of them does originate there. Internal conversion decay, like isomeric transition gamma decay and neutron emission, involves the release of energy by an excited nuclide, without the transmutation of one element into another. Rare events that involve a combination of two beta-decay-type events happening simultaneously are known (see below). Any decay process that does not violate the conservation of energy or momentum laws (and perhaps other particle conservation laws) is permitted to happen, although not all have been detected. An interesting example discussed in a final section, is bound state beta decay of rhenium-187. In this process, the beta electron-decay of the parent nuclide is not accompanied by beta electron emission, because the beta particle has been captured into the K-shell of the emitting atom. An antineutrino is emitted, as in all negative beta decays. If energy circumstances are favorable, a given radionuclide may undergo many competing types of decay, with some atoms decaying by one route, and others decaying by another. An example is copper-64, which has 29 protons, and 35 neutrons, which decays with a half-life of 12.7004(13) hours. This isotope has one unpaired proton and one unpaired neutron, so either the proton or the neutron can decay to the other particle, which has opposite isospin. This particular nuclide (though not all nuclides in this situation) is more likely to decay through beta plus decay (61.52(26)%) than through electron capture (38.48(26)%). The excited energy states resulting from these decays which fail to end in a ground energy state, also produce l ------------------------------ Date: Sat, 16 Sep 2023 20:13:03 +0000 From: "nazis defeated" Subject: Were the nazis defeated with THIS forgotten fungus cure? Dear, Can you really erase foot fungus in 4 short weeks? Sure, it sounds like BSb& But according to this Los Angeles doctor, itbs true. (Discover his antifungal secret here) [IMAGE] No, this isnbt another topical cream or medication filled with side-effects. In fact, this bForgotten Fungus Cureb is something youbve never heard ofb& Yet historians claim it helped the U.S. defeat the Nazis in WWII. Itbs revealed for the first time since 1944 right here (click here now). If youbre suffering from athletebs footb& ringwormb& jock itchb& or other nasty foot problemsb& I urge you to read this short article now. (Or you can skip straight to the bcureb by clicking here) Cynthia D. Orcutt B If you does't like this, please Click here 1908 Thomes Ave, Cheyenne, WY 82001 B B [IMAGE] ------------------------------ Date: Sat, 16 Sep 2023 19:10:57 +0200 From: "Aztec Manhood" Subject: White Man Offers Wife To Amazon Priest For Member Growth Secret White Man Offers Wife To Amazon Priest For Member Growth Secret http://singlecolombian.shop/qBqu5BFUFNmgt95f8Q_BU2ZijiDnDRaxiPICMmh0_lAo40LoMw http://singlecolombian.shop/5o9dR-TN6dBAHO3IXxenyRwbjHh0nDWZfkpXoA7W7bt686H9RQ All of these processes occur over time with characteristic rates. These rates are important in engineering. The field of non-equilibrium statistical mechanics is concerned with understanding these non-equilibrium processes at the microscopic level. (Statistical thermodynamics can only be used to calculate the final result, after the external imbalances have been removed and the ensemble has settled back down to equilibrium.) In principle, non-equilibrium statistical mechanics could be mathematically exact: ensembles for an isolated system evolve over time according to deterministic equations such as Liouville's equation or its quantum equivalent, the von Neumann equation. These equations are the result of applying the mechanical equations of motion independently to each state in the ensemble. These ensemble evolution equations inherit much of the complexity of the underlying mechanical motion, and so exact solutions are very difficult to obtain. Moreover, the ensemble evolution equations are fully reversible and do not destroy information (the ensemble's Gibbs entropy is preserved). In order to make headway in modelling irreversible processes, it is necessary to consider additional factors besides probability and reversible mechanics. Non-equilibrium mechanics is therefore an active area of theoretical research as the range of validity of these additional assumptions continues to be explored. A few approaches are described in the following subsections ------------------------------ Date: Sat, 16 Sep 2023 11:57:55 +0200 From: "Wheat Toast" Subject: Tammy almost DIED eating this Tammy almost DIED eating this http://mcgramfirearmholder.live/K0YhcqDk74uir0CvCo8VsJJv0mpcAH9QwQI2Vfo7T57On3RNvA http://mcgramfirearmholder.live/eT4iPQ13FNOvPaEuiqaOib7NsbqW218noD-4o4_dZPXc0Vhgtg The binding energy of helium is the energy source of the Sun and of most stars. The sun is composed of 74 percent hydrogen (measured by mass), an element having a nucleus consisting of a single proton. Energy is released in the sun when 4 protons combine into a helium nucleus, a process in which two of them are also converted to neutrons. The conversion of protons to neutrons is the result of another nuclear force, known as the weak (nuclear) force. The weak force, like the strong force, has a short range, but is much weaker than the strong force. The weak force tries to make the number of neutrons and protons into the most energetically stable configuration. For nuclei containing less than 40 particles, these numbers are usually about equal. Protons and neutrons are closely related and are collectively known as nucleons. As the number of particles increases toward a maximum of about 209, the number of neutrons to maintain stability begins to outstrip the number of protons, until the ratio of neutrons to protons is about three to two. The protons of hydrogen combine to helium only if they have enough velocity to overcome each other's mutual repulsion sufficiently to get within range of the strong nuclear attraction. This means that fusion only occurs within a very hot gas. Hydrogen hot enough for combining to helium requires an enormous pressure to keep it confined, but suitable conditions exist in the central regions of the Sun, where such pressure is provided by the enormous weight of the layers above the core, pressed inwards by the Sun's strong gravity. The process of combining protons to form helium is an example of nuclear fusion. Producing helium from normal hydrogen would be practically impossible on earth because of the difficulty in creating deuterium. Research is being undertaken on developing a process using deuterium and tritium. The earth's oceans contain a large amount of deuterium that could be used and tritium can be made in the reactor itself from lithium, and furthermore the helium product does not harm the environment, so some consider nuclear fusion a good alternative to supply our energy needs. Experiments to carry out this form of fusion have so far only partially succeeded. Sufficiently hot deuterium and tritium must be confined. One technique is to use very strong magnetic fields, because charged particles (like those trapped in the Earth's radiatio ------------------------------ Date: Sat, 16 Sep 2023 14:34:22 +0200 From: "Breathing Method" Subject: How to breathe away" Alzheimer's memory loss? How to breathe away" Alzheimer's memory loss? http://medigardenkit.cyou/tT0xKTaUR1YPLAgy5nZ94_TK8NthlNvC78X5Pag8b63gb4w46g http://medigardenkit.cyou/7nqFeoJdMLdIA5UzNvk7meYcpqWgPfBBCgls1jqtztC0MrnSPQ Other types of radioactive decay were found to emit previously seen particles but via different mechanisms. An example is internal conversion, which results in an initial electron emission, and then often further characteristic X-rays and Auger electrons emissions, although the internal conversion process involves neither beta nor gamma decay. A neutrino is not emitted, and none of the electron(s) and photon(s) emitted originate in the nucleus, even though the energy to emit all of them does originate there. Internal conversion decay, like isomeric transition gamma decay and neutron emission, involves the release of energy by an excited nuclide, without the transmutation of one element into another. Rare events that involve a combination of two beta-decay-type events happening simultaneously are known (see below). Any decay process that does not violate the conservation of energy or momentum laws (and perhaps other particle conservation laws) is permitted to happen, although not all have been detected. An interesting example discussed in a final section, is bound state beta decay of rhenium-187. In this process, the beta electron-decay of the parent nuclide is not accompanied by beta electron emission, because the beta particle has been captured into the K-shell of the emitting atom. An antineutrino is emitted, as in all negative beta decays. If energy circumstances are favorable, a given radionuclide may undergo many competing types of decay, with some atoms decaying by one route, and others decaying by another. An example is copper-64, which has 29 protons, and 35 neutrons, which decays with a half-life of 12.7004(13) hours. This isotope has one unpaired proton and one unpaired neutron, so either the proton or the neutron can decay to the other particle, which has opposite isospin. This particular nuclide (though not all nuclides in this situation) is more likely to decay through beta plus decay (61.52(26)%) than through electron capture (38.48(26)%). The excited energy states resulting from these decays which fail to end in a ground energy state, also produce l ------------------------------ Date: Sat, 16 Sep 2023 17:36:50 +0200 From: "Mute Tinnitus" Subject: Sit On The Edge Of Your Bed And Do This To Mute Tinnitus Sit On The Edge Of Your Bed And Do This To Mute Tinnitus http://steelbiteepro.shop/r3sohg4Ur9ZXmKm01lQEzWxVPFPJH_DMHWtw3ThtKcpCkzucYA http://steelbiteepro.shop/fKDVfpJnnghZpBXThtKqzZ0FhLQFU7wmBWVZ7Lsg0NW5e7zFFw The Monte Carlo method is a stochastic method popularized by physics researchers Stanis?aw Ulam, Enrico Fermi, John von Neumann, and Nicholas Metropolis. The use of randomness and the repetitive nature of the process are analogous to the activities conducted at a casino. Methods of simulation and statistical sampling generally did the opposite: using simulation to test a previously understood deterministic problem. Though examples of an "inverted" approach do exist historically, they were not considered a general method until the popularity of the Monte Carlo method spread. Perhaps the most famous early use was by Enrico Fermi in 1930, when he used a random method to calculate the properties of the newly discovered neutron. Monte Carlo methods were central to the simulations required for the Manhattan Project, though they were severely limited by the computational tools of the time. Therefore, it was only after electronic computers were first built (from 1945 on) that Monte Carlo methods began to be studied in depth. In the 1950s they were used at Los Alamos for early work relating to the development of the hydrogen bomb, and became popularized in the fields of physics, physical chemistry, and operations research. The RAND Corporation and the U.S. Air Force were two of the major organizations responsible for funding and disseminating information on Monte Carlo methods during this time, and they began to find a wide application in many different fields. Uses of Monte Carlo methods require large amounts of random numbers, and it was their use that spurred the development of pseudorandom number generators, which were far quicker to use than the tables of random numbers which had been previously used for statistical samplin ------------------------------ Date: Sun, 17 Sep 2023 07:00:00 +0300 From: reham nomeer Subject: =?UTF-8?B?2KfZh9mF2YrYqSDYp9mE2KPYs9in2YTZitioINin2YTYrdiv2YrYq 9ipINin2YTYs9io?= =?UTF-8?B?2LnYqSDZhNiq2YLZitmK2YUg2KfZhNij2K/Yp9ihINmB2Yog2YbYuNin2YUg 2KfZhNmF2YjYp9ix2K8g?= =?UTF-8?B?2KfZhNio2LTYsdmK2Kkg2KfZhNiz2LnZiNiv2Yog2YTZhNiq2YHYp9i12YrZ hDogMDAyMDEwMjM5OTA5?= =?UTF-8?B?MDE=?= X'YX3YX'Y X9YY YY YX1X-YX) X'YYY YX(X1YX'X*X) *X'YX/X'X1 X'YX9X1X(Y X) YYX*YYY X) X'YX'X/X'X1Y X) X*YX/Y YYY* *X4YX'X/X) YY X'X3 YX$X4X1X'X* X'YX'X/X'X! X'YX1X&Y X3Y X) **KPI* *X'YX#X3X'YY X( X'YX-X/Y X+X) X'YX3X(X9X) YX*YY Y Y X'YX#X/X'X! 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X'YX'X4X*X1X'Y YY YX0Y X'YYX,YYX9X) YX%Y YX'Y X*YYY X1X3X'X&Y X'YX%YYX*X1YYY X) YYYX'X X#X1X3Y X1X3X'YX) X%YYX*X1YYY X) X%YY ahadhrorg22+unsubscribe@googlegroups.com. YX9X1X6 YX0Y X'YYYX'YX4X) X9YY X'YYY X(X X'YX*YY X%YY https://groups.google.com/d/msgid/ahadhrorg22/CAEcxT4sBhGnUBmgNnxL1m4RuKaS2a8eLzNj%2B19ZgbPYx8W-%2BqQ%40mail.gmail.com. ------------------------------ End of alt.music.moxy-fruvous digest V14 #12232 ***********************************************