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1 scribing entropy and velocity "thermodynamic relativity".
2 ntersection of quantum mechanics and general relativity.
3 rresponding to linear adaptations of special relativity.
4 mpatible with the predictions from numerical relativity.
5 ck hole confirms a key prediction of general relativity.
6 the definition of causality in the theory of relativity.
7 pond to a possible anisotropic adaptation of relativity.
8 ame addition rule derived from thermodynamic relativity.
9 ecial relativity, or simply, the anisotropic relativity.
10 re a surprisingly identical description with relativity.
11 ising path - the new theory of thermodynamic relativity.
12 haracter in quantum mechanics and in general relativity.
13 nd explained by Einstein's theory of special relativity.
14 s of quantum mechanics and classical general relativity.
15 tal physics and specific features of General Relativity.
16 light by a dense cluster of stars in general relativity.
17 , consistent with that expected from general relativity.
18 c frame dragging, is a prediction of general relativity.
19  that confirmed Einstein's general theory of relativity.
20 inal paper introducing the general theory of relativity.
21 tal constant variation and improved tests of relativity.
22 ves and phase shifts associated with general relativity.
23  the strong equivalence principle of general relativity.
24 nd laboratory tests of quantum mechanics and relativity.
25 tronomers and described by classical general relativity.
26 h approximately 10x increase in longitudinal relativity.
27 (R) theory, which is an extension of general relativity.
28 ions of gravity on large scales from general relativity.
29 f space-time in Einstein's general theory of relativity.
30 ur independent strong-field tests of general relativity.
31 cetime as predicted by the general theory of relativity.
32 y, in contrast, has its deep base in general relativity.
33 ears before completing his general theory of relativity.
34 imics the effects of a point mass in general relativity.
35 ct predicted by Einstein's theory of general relativity.
36 our choices, we often suffer from two tragic relativities.
37 ed melanoma on the basis of the phase II/III RELATIVITY-047 and phase III CheckMate 067 trials, respe
38 data, in combination with the results of the RELATIVITY-047 trial(1), provide further confirmation of
39 descriptive efficacy and safety results from RELATIVITY-047 with a median follow-up of 33.8 months.
40 g (RELATIVITY-098) versus advanced melanoma (RELATIVITY-047), where LAG-3(+) T cells were enriched in
41                          Minimum follow-ups (RELATIVITY-047, 33 months; CheckMate 067, 36 months) wer
42                                     Based on RELATIVITY-047, nivolumab plus relatlimab is approved fo
43                                              RELATIVITY-060 did not meet its primary end point of imp
44                   Open-label phase II study (RELATIVITY-060) to investigate the efficacy and safety o
45 resected melanoma, the phase 3, double-blind RELATIVITY-098 trial compared adjuvant nivolumab plus re
46 ng LAG-3(+) T cells in the adjuvant setting (RELATIVITY-098) versus advanced melanoma (RELATIVITY-047
47                                      General relativity(1) predicts that short-orbital-period binarie
48 uch networks promise better tests of general relativity(1-3), dark-matter searches(4) and gravitation
49  provide the basis of a broader framework of relativity: (1) no privileged reference frame with zero
50 re consistent with expectations from general relativity(5).
51 ions from Newtonian gravity(3-6) and general relativity(7).
52     We introduce the theory of thermodynamic relativity, a unified theoretical framework for describi
53 e curves are striking predictions of general relativity allowing for time-travel.
54 techniques that variationally include scalar relativities and spin-orbit coupling directly at the mol
55 ate for testing Einstein's theory of general relativity and alternative theories of gravity in the st
56                                   In General Relativity and for nuclear matter, Lambda and the f-mode
57 to be applicable when the effects of special relativity and general relativity are important.
58  original paper, including a tension between relativity and nonlocal effects predicted by quantum mec
59 ce principle is at the foundation of General Relativity and of most gravitational theories.
60 panions have allowed unique tests of general relativity and provided evidence for gravitational radia
61 ill enable the study of the union of general relativity and quantum mechanics once they become sensit
62                                              Relativity and quantum mechanics show that even a single
63 l clock that obeys the principles of general relativity and quantum mechanics, such a picture is, at
64       Singularities in the general theory of relativity and the lack of a quantum theory of gravity s
65                 Einstein's theory of special relativity and the principle of causality imply that the
66 tle forces signifying physics beyond General Relativity and the Standard Model.
67 tor stars, enable stringent tests of general relativity, and constrain the behavior of matter at dens
68  using classical electrodynamics and special relativity, and expressed in the Fourier domain, as a fu
69 ory reconciles quantum mechanics and special relativity, and plays a central role in many areas of ph
70 lating to individual differences, linguistic relativity, and the relation of perceptual and semantic
71 so responsible for the postulates of special relativity, and therefore its counterintuitive aspects o
72 he effects of special relativity and general relativity are important.
73  Quantum mechanics and the general theory of relativity are two pillars of modern physics.
74 f velocities in Einstein's isotropic special relativity, as in two extreme cases, while intermediate
75 ack holes through stringent tests of general relativity, as well as insights into the role of black h
76                                      Special relativity asserts that physical phenomena appear the sa
77                                While special relativity assumes that there is no fundamental length-s
78 ing a generalized framework of the theory of relativity, based on the kappa-addition formulation, whi
79                 This is the first example of relativity being decisive for the nature of an observed
80  may open the possibility of probing general relativity beyond our local universe.
81 s, astrophysics, quantum physics and general relativity, can be connected by the same universal geode
82 ping (EHM), connect the equations of general relativity, chaos and quantum mechanics via a universal
83 ear adaptations of relativity; thermodynamic relativity constitutes a new path of generalization, as
84 e perspectives of a variety of stakeholders (relativity), discusses core concepts in how costs are cl
85 ns of Einsteinian gravity (classical general relativity) do not require one to fix a specific equatio
86 rmulations of the linear anisotropic special relativity; e.g., the asymmetric Lorentz transformation,
87 on, thereby providing support for linguistic relativity effects in the grammatical domain.
88 gy and mass, developed the theory of special relativity, explained the photoelectric effect, and desc
89                          Using thermodynamic relativity for velocities, we start from the kappa-addit
90                 Einstein's general theory of relativity from 1915(1) remains the most successful desc
91       Binary pulsars are affected by general relativity (GR), causing the spin axis of each pulsar to
92                                      General relativity(GR) is the current description of gravity in
93   One hundred years after its birth, general relativity has become a highly successful physical theor
94                 Attempts to quantize general relativity have led to many rival models of quantum grav
95                         These predictions of relativity have previously been observed with atomic clo
96                                         This relativity ia a signature of an indefinite metric, where
97 ron stars from quark stars, and test general relativity in a nuclear structure-independent fashion.
98        This is the first study to generalize relativity in a thermodynamic context, leading naturally
99 ial and to test Einstein's theory of general relativity in an unexplored regime.
100 dark matter detectors(6-12) and new tests of relativity in the lab(13-16).
101 has allowed us to test the theory of general relativity in the strong-field regime.
102 ory properly incorporates quantum theory and relativity, in particular, at regimes where space-based
103 vide new evidence for correctness of general relativity, in particular, in the strong field limit.
104  a unique astrophysical tool to test general relativity, inform on matter in extreme conditions, and
105                           Although numerical relativity is accurate(5-7), it is too time-consuming to
106  predictions of Einstein's special theory of relativity is also perhaps the best known formula in all
107          A cornerstone of Einstein's special relativity is Lorentz invariance-the postulate that all
108                             A consequence of relativity is that in the presence of an electric field,
109                           A tenet of special relativity is that no particle can exceed the speed of l
110     One consequence of the special theory of relativity is that no signal can cause an effect outside
111                                      General relativity is the essential foundation of the standard m
112 ts amount and distribution, assuming general relativity is valid.
113  enormous--given the degree to which special relativity is woven into the theoretical fabric of moder
114  metric theories of gravity, such as general relativity, is that a clock in a gravitational potential
115 l systems (i.e., electrodynamics and general relativity), it was not realized that light could posses
116 hen, we show how the developed thermodynamic relativity leads to the addition of entropies in nonexte
117    At the intersection of quantum theory and relativity lies the possibility of a clock experiencing
118 ysics or point toward a breakdown of general relativity on cosmological scales.
119 tups do not take into account the effects of relativity on quantum properties.
120 ter Einstein published the general theory of relativity, one of its most important predictions was ve
121 physics experiments such as tests of general relativity or searches for electron electric dipole mome
122 t physical meaning, like the ones of special relativity or thermodynamics, and it articulates a stron
123 synchronous adaptation of Einstein's special relativity, or simply, the anisotropic relativity.
124                 Einstein's theory of general relativity predicts that a clock at a higher gravitation
125                        The general theory of relativity predicts that a star passing close to a super
126                                    Numerical relativity simulations across different groups consisten
127 ications and quantum clocks at regimes where relativity starts to kick in.
128                 Einstein's theory of general relativity states that clocks at different gravitational
129 nts unfold in a fixed order while in general relativity temporal order is influenced by the distribut
130 ativity - the one derived from thermodynamic relativity that corresponds to linear Lorentz transforma
131 urvature, an underlying principle of general relativity that has come under scrutiny in connection wi
132 sms, thereby embodying a mechanistic "neural relativity" that may clarify how episodic memories are l
133 clude that the broadest formalism of special relativity - the one derived from thermodynamic relativi
134                                   In general relativity, the metric is influenced by matter, and is e
135                                   In general relativity, the picture of space-time assigns an ideal c
136                     In the general theory of relativity, the weak equivalence principle (WEP) require
137 erimental cornerstones of Einstein's special relativity theory and is well understood(3,4) in the con
138 ing from the merger of quantum mechanics and relativity theory) has provided a clear understanding of
139  to anisotropic and nonlinear adaptations of relativity; thermodynamic relativity constitutes a new p
140 cal objects; a direct consequence of general relativity, they were first directly observed in 2015.
141 ently developed the framework of anisotropic relativity through a perhaps surprising path - the new t
142  range from satellite clocks testing general relativity to portable clocks for inertial navigation sy
143 is a curved manifold as portrayed by general relativity, translation in space can be accomplished sim
144         Modern tests of Einstein's theory of relativity try to measure so-far-undetected violations o
145                             Although general relativity underlies modern cosmology, its applicability
146 n-relativistic quantum mechanics and special relativity via their "mysteries" is the restricted Loren
147 hysical consequence of the general theory of relativity, was found even before this theory was formul
148 bution to both quantum mechanics and special relativity, we approach another anniversary--that of Ein
149 the BP of Au increases by about 800 K due to relativity, which is in line with the strong relativisti
150 is affected by gravity (described by general relativity) with the implication that the charge is redu
151 s agrees with the value predicted by general relativity within an uncertainty of 0.05%, the most prec
152  models show that these growth and mortality relativities would account for the common life history p
153  = 0.88 +/- 0.17, is consistent with general relativity (Y = 1) and excludes a Newtonian model (Y = 0

 
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