neutron temperature 中文意思是什麼

neutron temperature 解釋
中子溫度
  • neutron : n. 【物理學】中子。n. -ics 中子（物理）學。
  • temperature : n. 1. 溫度，氣溫。2. 體溫。3. 〈口語〉發燒，高燒。
  1. There has been many papers to discuss the in - medium quark and gluon condensates in nuclear matter which use the models with su ( 2 ) l su ( 2 ) r sym - metry. now, we make use of the chiral model su ( 3 ) l su ( 3 ) n including the baryon octet to discuss the quark condensate < qq > in strange matter, where q is an up or down quark field. on the one hand, from the experimetal data, it is found that < qq > vac = - ( 225 25mev ) 3, on the other hand, with the hellmann - feynman theorem, quark condensate can be evaluated on the hadronic level. in this paper, we will investigate the quark condensate in strange matter with the chiral symmetry su ( 3 ) l x su ( 3 ) rspontaneous breaking lagrangian to obtain the variation of the quark condensate in the strange matter when the baryon number change. it can be applied to understand the neutron stars when the neutron star are considered to be constructed by the strange matter. because nertron stars are homogeneous and at very low temperature, we will use the mean - field approximation and zero temperature throughout this paper

    鑒于已有大量文獻討論了核物質中的夸克凝聚，本文將討論在奇異物質中的夸克凝聚。而在介質中的夸克凝聚的基本公式可由hellmann - feynman理論導出，所以運用手征對稱自發破缺拉氏量以及平均場近似，我們就可以討論在奇異物質中的夸克凝聚，由所計算的結果表明： （ 1 ）奇異物質中的夸克凝聚隨奇異物質密度的增大而單調減小。 （ 2 ） -凝聚的出現對衰減率有影響。
  2. The experimental study of fuel ion temperature and neutron yield for directly driven implosion

    激光直接驅動內爆中子產額實驗診斷
  3. When the energy distribution of secondary neutron are represented by evaporation spectrum ( lf = 9 ), care must be taken in describing the nuclear temperature near the threshold

    通過分析發現，評價次級中子能譜數據所採用的蒸發譜模型大都忽略了能級密度參數與激發能之間的關聯。
  4. It is called thermal neutron because the average kinetic energy of the neutron is directly proportional to the temperature

    指核反應堆在穩定的裂變率下達到自持鏈式反應的狀態。
  5. The neutron flux extracted to different angles has been calculated. finally, the heat depositions in the target, the reflector and the moderator have been calculated. based on these results, the temperature and stress distribution hi tungsten target under different cooling condition have been calculated too

    最後計算了靶、反射體以及不同慢化器（水、液態氫、液態甲烷）中的熱量沉積，並以此為依據，利用工程軟體ideas進一步計算了各種冷卻條件下，靶中溫度場與應力場分佈。
  6. This kind of detector has many merits as follows : fast response time, large output current, fine linear response, high sensitivity to many particles including neutron, charged particle, x - ray, gamma - ray, visible light, and being able to work at indoor temperature

    這種探測器具有時間響應快，輸出電流大，對多種粒子如中子、帶電粒子、 x射線、射線、可見光都具有高靈敏度，而且響應的線性性好，可在室溫工作等特點。
  7. The large nuclear temperature evaluation would violate conservation of energy, and may lead a negative neutron kerma factor

    這就可能使評價核溫度太高而導致平均次級中子能量（ ? ）過大，破壞了能量守恆，而導致了負kerma因子。
  8. The results show that the contribution of direct capture is primary in the interested temperature range of astrophysics. toward the 12c ( n, y ) 13c reaction, our calculations are good agreement with a recent experiment at low energy. a obvious enhancement of the cross section of 12c ( n, y ) 13c first excited state has been found, and it supports that the first excited state 1 / 2 + of 13c is a neutron halo state which has been found experimentally by our department group

    對于第一個核反應，我們計算了直接俘獲過程以及兩個共振態的俘獲截面和總截面，我們的計算結果顯示，在天體感興趣的溫度范圍內，直接俘獲過程對總截面的貢獻是主要的；對于第二個反應，我們的計算結果與已有的實驗結果符合的較好，其中~ （ 12 ） c （ n ， ） ~ （ 13 ） c的第一激發態計算結果顯示出截面有明顯增大，這從理論上支持了我所關于~ （ 13 ） c第一激發態具暈結構的實驗發現，這是國際上第一次在激發態中發現暈結構。
  9. The temperature range of quasisoft x - ray sources falls just right for an accreting black hole that is more massive than a stellar - mass black hole. however, we should be cautioned that in principle, the low temperatures of many quasisoft x - ray sources can be explained by stellar - mass black holes, neutron stars, and even white dwarfs under very specific physical conditions

    就以類軟射線源的溫度范圍來說，雖然它完全符合那些比恆星型黑洞更大的吸積黑洞，但有一點不能忽略，就是這個溫度在理論上也可以是由恆星型黑洞中子星甚至白矮星在一些特殊物理情況下產生。
  10. In respect of sic devices, an analytical model of 6h - sic jfet to well match the experimental results is proposed. the radiation response of sic jfet in room temperature to 300 c is simulated with the analysis for the neutron irradiation effect such as carrier removal, mobility degradation and space charge density decrease

    對sicjfet的電參數如電子濃度，遷移率，電阻率和空間電荷區密度在中子輻照下的變化進行了分析，提出了中子輻照下6h - sicjfet的器件模型，利用此模型對sicjfet在室溫和300時的輻照響應進行模擬的結果和實驗值相符。
  11. ( 3 ) through the study of electrical property of irradiated rutile by high - dose neutron, the curse of relationship of conductivity and temperature has been abtained. according to this relationship, the conducting behavior in diflrent temperature is also studied

    本論文工作還對高注t中子輻照后金紅石晶體的電學特性進行了研究，得到了它在空氣和真空中的電阻與溫度的關系，分析了各個溫區的導電機制。
  12. Optimized in lightweight, compactness and high temperature sustaining the shielding materials for neutron and gamma radiation were designed based on genetic algorithms

    摘要為研製兼具質地輕、體積小、耐高溫等特點的新型中子、混合輻射屏蔽材料，用遺傳演算法建立了屏蔽材料優化設計方法。
  13. Under condition of floating power supply pluse width modulation autocontrol is used to stabilize operation of neutron generater in high temperature circumstance

    在懸浮式系統中採用脈寬調制式氣壓自動控制，保證了中子發生器能在高溫條件下穩定工作。
  14. Interact of fast - neutron irradiation defects and oxygen impurity in cz - silicon was investigated in this paper. the result suggested that oxygen precipitation formed at high temperature was promoted by fast - neutron irradiation obviously. compared with ntdczsi, fast neutron irradiation accelerated precipitation in czsi much more

    本文對快中子輻照直拉硅中的缺陷和氧的相互作用進行了研究，快中子輻照促進了直拉硅中的氧沉澱，與以往ntdczsi研究結果相比，其促進作用更加明顯。
  15. Sensors are used to detect the content of water and the temperature of grains, to measure the velocity of influx and to position the grains in the drying machines respectively. thermal sensors are thermocouples to monitor the temperature of heated air current and thermo resistances to measure the temperature of grains on different surfaces ; water sensors include neutron probes and condensates to measure the content of water of grains before and after drying respectively ; the velocity of flow of grains is measured by the indicators of flow

    溫度傳感器主要採用熱電偶和熱電阻，分別探測熱風溫度和乾燥機各個層面上的糧食溫度；水分傳感器主要採用中子式在線水分測量儀和電容式在線水分測量儀，中子式在線水分測量儀由於不受穀物解凍的影響，用來測量烘前穀物的水分，電容式在線水分測量儀用來測定烘后的糧食水分；在線流量計採用沖板式流量計，用來記錄排糧流量，統計產量。
  16. Because the neutrino energy loss rate in strange matter is much higher than that in neutron matter, the surface temperature of a young strange star is lower than that of an ordinary neutron star of the same age

    奇異星與中子星的表面熱輻射特性有顯著的不同。由於奇異物質發射較多中微子，所以能量損失速度較快，因此一顆年青的奇異星，表面溫度會比同年的中子星為低。
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